THE CIRCLES OF PROPORTION AND THE HORIZONTAL INSTRVMENT.
The Former shewing the maner how to work Proportions both simple and compound: and the ready and easy resolving of Quaestions both in Arithmetic, Geometrie, & Astronomie: And is newly increased with an Additament for Navigation. All which Rules may also be wrought with the penne by Arithmetic, and the Canon of Triangles.
The Later teaching how to work most Quaestions, which may be performed by the Globe: and to delineat Dialls upon any kind of Plaine.
Invented, and written in Latine by W. O. Translated into English, and set out for the public benefit, by WILLIAM FORSTER.
LONDON, Printed by Augustine Mathewes, and are to bee sold by Nic: Bourne at the Royall Exchange. 1633.
TO THE HONOVRABLE AND RENOWNED FOR vertue, learning, and true valour, Sir KENELME DIGBYE Knight.
THE excellent accomplishments wherwith you are adorned both of vertue, and learning, and particularly in the Mathematicall Sciences, together with the Honourable respect the Author hereof beareth vnto your Worth, and his desire to testifie the same, hath made mee presume to present vnto you, and vnder the happy auspice of your renowned name, to publish to the world this Treatise: the owning whereof though I may not chalenge to my selfe, yet the birth and production, whereby it hath a being to the benefit of others, is, as vnto a second parent, due vnto me.
For being in the time of the long vacation 1630, in the Country, at the house of the Reuerend, [Page] and my most worthy friend, and Teacher, Mr. William Oughtred (to whose instruction I owe both my initiation, and whole progresse in these Sciences.) I vpon occasion of speech told him of a Ruler of Numbers, Sines, & I angents, which one had be spoken to be made (such as is vsually called Mr. Gunters Ruler) 6 feet long, to be vsed with a payre of beame-compasses. ‘He answered that was a poore invention, and the performance very troublesome: But, said he, seeing you are taken with such mechanicall wayes of Instruments, I will shew you what deuises I haue had by mee these many yeares.’ And first, hee brought to mee two Rulers of that sort, to be vsed by applying one to the other, without any compasses: and after that hee shewed mee those lines cast into a circle or Ring, with another moueable circle vpon it. I seeing the great expeditenesse of both those wayes; but especially, of the latter, wherein it farre excelleth any other Instrument which hath bin knowne; told him, I wondered that hee could so many yeares conceale such vsefull inuentions, not onely from the world, but from my selfe, to whom in other parts and mysteries of Art, be had bin so liber all. ‘He answered, [Page] That the true way of Art is not by Instruments, but by Demonstration: and that it is a preposterous course of vulgar Teachers, to begin with Instruments, and not with the Sciences, and so in-stead of Artists, to make their Schollers only doers of tricks, and as it were Iuglers: to the despite of Art, losse of precious time, and betraying of willing and industrious wits, vnto ignorance, and idlenesse. That the vse of Instruments is indeed excellent, if a man be an Artist: but contemptible, being set and opposed to Art. And lastly, that he meant to commend to me, the skill of Instruments, but first he would haue me well instructed in the Sciences.’ He also shewed me many notes, and Rules for the vse of those circles, and of his Horizontall Instrument, (which he had proiected about 30 yeares before) the most part written in Latine. All which I obtained of him leaue to translate into English, and make publique, for the vse, and benefit of such as were studious, & louers of these excellent Sciences.
Which thing while I with mature, and diligent care (as my occasions would giue me leaue) went about to doe: another to whom the Author in a louing confidence discouered this intent, vsing [Page] more hast then good speed, went about to preocupate; of which vntimely birth, and preuenting (if not circumuenting) forwardnesse, I say no more: but aduise the studious Reader, onely so farre to trust, as he shal be sure doth agree to truth & Art.
And thus most noble Sir, without any brauing flourishes, or needlesse multiplying of tautologized and erroneous praecepts, in naked truth, and in the modest simplicity, of the Author himselfe (whose knowne skill in the whole Systeme of Mathematicall learning, will easily free him from the suspicion of hauing the way made for him, and the subiect vnuailed, to help his sight) I haue notwithstanding vnder the protection of your courteous fauour, and learned iudgement, persisted in my long conceiued purpose, of presenting this tractate to the publique view, and light. Wishing withall vnto you encrease of deserued honor, and happines.
Thos that desire farther instructions in the use of th [...]s Instruments or other parts of the Mathematiques may repaire to W Forster at the Red bull ouer against St Clements Church yard with out Temple bar
THE FIRST PART OF THIS BOOKE, Shewing the vse of the First side of the Instrument, for the working of Proportions both simple and compounded, and for the ready and easie resolving of questions both in Arithmetique, Geometrie, and Astronomie, by Calculation.
CHAP. I. Of the Description, and vse of the Circles in this First side.
1 THere are two sides of this Instrument. On the one side, as it were in the plaine of the Horizon, is delineated the proiection of the Sphare. On the other side there are divers kindes of Circles, divided after many severall waies; [Page 2] together with an Index to be opened after the manner of a paire of Compasses. And of this side we will speake in the first place.
2 The First, or outermost circle is of Sines, from 5 degrees 45 minuts almost, vntill 90. Every degree till 30 is divided into 12 parts, each part being 5 min: from thence vntill 50 deg: into sixe parts which are 10 min: a peece: from thence vntill 75 degrees into two parts which are 30 minutes a peece. After that vnto 85 deg: they are not divided.
3 The Second circle is of Tangents, from 5 degrees 45 min: almost, untill 45 degrees. Every degree being divided into 12 parts which are 5 min: a peece.
4 The Third circle is of Tangents, from 45 degrees untill 84 degrees 15 minutes. Each degree being divided into 12 parts, which are 5 min: a peece.
5 The Sixt circle is of Tangents from 84 degrees till about 89 degrees 25 minutes.
The Seventh circle is of Tangents from about 35. min: till 6 degrees.
The Eight circle is of Sines, from about 35 minutes til 6 degrees.
6 The Fourth circle is of Vnaequall Numbers, which are noted with the Figures 2, 3, 4, 5, 6, 7, 8, 9, 1. Whether you vnderstand them to bee single Numbers, or Tenns, or Hundreds, or Thousands, &c. And every space of the numbers till 5, is divided into 100 parts, but after 5 till 1, into 50 parts.
The Fourth circle also sheweth the true or naturall Sines, and Tangents. For if the Index bee applyed to any Sine or Tangent, it will cut the true Sine or Tangent in the fourth circle. And wee are to knowe that if the Sine or Tangent be in the First, or Second circle, the figures of the Fourth circle doe signifie so many thousands. But if the Sine or Tangent be in the Seventh or Eight circle, the figures in the Fourth circle signifie so many hundreds. And [Page 3] if the Tangent bee in the Sixt circle, the figures of the Fourth circle, signifie so many times tenne thousand, or whole Radij.
And by this meanes the Sine of 23°, 30′ will bee found 3987: and the Sine of it's complement 9171. And the Tangent of 23°, 30′ will be found 4348: and the Tangent of it's complement, 22998. And the Radius is 10000, that is the figure 1 with foure cyphers, or circles. And hereby you may finde out both the summe, and also the difference of Sines, and Tangents.
7 The Fift circle is of Aequall numbers, which are noted with the figures 1, 2, 3, 4, 5, 6, 7, 8, 9, 0; and every space is divided into 100 aequall parts.
This Fift circle is scarse of any use, but onely that by helpe thereof the given distance of numbers may be multiplied, or divided, as neede shall require.
As for example, if the space betweene 1⌊00 and 1⌊0833+ bee to bee septupled. Apply the Index vnto 1⌊0833+ in the Fourth circle, and it will cut in the Fift circle 03476+; which multiplyed by 7 makes 24333: then againe, apply the Index vnto this number 24333 in the Fift circle, and it will cut in the Fouth circle 1⌊7512+. And this is the space betweene 1⌊00 and 1⌊0833+ septupled, or the Ratio betweene 100, and 108⅓ seven times multiplied into it selfe.
And contrarily, if 1⌊7512 bee to bee divided by 7: Apply the Index vnto 1⌊7568 in the fourth circle, and it will cut in the fit circle 24333: which divided by 7 giveth 03476+. Then againe vnto this Number in the Fift circle apply the Index, and in the Fourth circle it wil cut vpon 1⌊0833+ for the Septupartion sought for.
The reason of which Operation is, because this Fift circle doth shew the Logarithmes of Numbers. For if the Index be applyed unto any number in the Fourth circle, it will in the Fift circle cut vpon the Logarithme of the same number, so that to the Logarithme found you praefixe a Caracteristicall [Page 4] (as Master Brigs termes it) one lesse then is the number of the places of the integers proposed (which you may rather call the Graduall Number). So the Logarithme of the number 2 will bee found 0.30103. And the Logarithme of the Number 43⌊6 will bee found 1.63949.
Numbers are multiplied by Addition of their Logarithmes: and they are Divided by Substraction of their Logarithmes.
8 In the middest among the Circles, is a double Nocturnall instrument, to shew the hower of the night.
9 The right line passing through the Center, through 90, and 45 I call the Line of Vnitie, or of the Radius.
10 That Arme of the Index which in euery Operation is placed at the Antecedent, or first terme', I call the Antecedent arme: and that which is placed at the consequent terme, I call the Consequent Arme.
CHAP. II. Of the Operation of the Rule of Proportion: and also of Multiplication, and Division.
1. Theoreme. IF of three numbers given, the first divide the second and the quotient multiply the third, the product shall be the fourth proportionall, to the three numbers given.
Theoreme. If of three numbers given, the second divide the first, and the quotient divide the third; this later quotient shall be the fourth proportionall, to the three numbers given.
Neither is it materiall whether of the two numbers after the first be second, or third.
2 And note that in Reciprocal proportion, that terme by which the question is made; But in Direct proportion the terme that is homogeneal thereto, is the first terme, or the Antecedent of the first ratio.
3 And therefore out of these foundations thus layd, (if you rightly conceive the nature of the Logarithmes) doth follow the finding out of the fourth proportionall by this Instrument: whereof this is the Rule.
Open the Armes of the Instrument to the distance of the first, and second number: then bring the Antecedent arme, or that which stood vpon the first number vnto the third, and so the consequent arme, keeping the same opening, will shew the fourth number sought for.
In which operation these foure things are diligently to be considered.
[Page 6] First, in constituting the places of each number in the fourth circle; whether the figures written in the spaces doe signifie Vnites, Tenns, or Hundreds, &c.
Secondly, if that arme which sheweth the fourth proportionall, doe reach beyond the line of the Radius; that then you doe account the fourth in a new circle or degree.
Thirdly, whether the fourth number sought, ought to be greater, or lesser then the third. For if a fourth number bee offered greater then the third, when it should be lesse, or lesse then the third when it should be greater; it is a signe that that number doth appertaine to a circle of another degree.
Fourthly, that looke what true distance was betweene the first and second, that the same bee supposed betweene the third and the fourth, and also on the same part.
4 And for because Multiplication and Division, have a certaine implicite proportion: we will speake of them in the first place.
5 In Multiplication, As an Vnite is to one of the factores (or numbers to be multiplied:) so is the other of the factores, to the product.
And the product of two numbers shall have so many places as there be in both the factores, if the lesser of them [Page 7] exceede so many of the first figures of the product: But if it doe not exceede, it will have one lesse.
6 And in Division, As the Divisor is to an Vnite; so is the Dividend, to the Quotient.
And the Quotient shall have so many places, as the Dividend hath more then the Divisor, if the Divisor exceede so many of the first figures of the Dividend: but if it doe not exceede, it shall have one place more.
7 Wherefore let this rule bee still carefully kept in minde: that In Multiplication the first terme of the implicite proportion is evermore 1: And in Division, the first terme is the Divisor.
And thus much concerning the operation of Proportion, Multiplication, and Division, I thought meete to admonish, least hereafter in Multiplying, or Dividing, or seeking out a fourth proportional, wee be constrained to repeate the same things many times over.
8 An example of Multiplication. How many pence are there in 47li. 9sh? For because 1 shilling containes 12 pence, and 1 pound containes 20 shillings, that is 240 pence: you shall multiply 47 by 240, and 9 by 12, and then adde together the products.
In the first Multiplication. 1 · 47 ∷ 240 · 11280 ·
For set the Armes of the Index at 1 and 47 in the fourth circle; and then bring the Antecedent arme (which stood at 1) vnto 240, and the Consequent arme will shew 11280.
Againe in the second Multiplication. 1 · 9 ∷ 12 · 108 ·
For set the two Armes of the Index at 1 and 9 in the fourth circle; and bring the Antecedent arme unto 12, and the Consequent arme will shew 108. Lastly, adde together 11280 and 108 and the summe 11388 will be the number of pence contained in the said summe of 47li, 9sh.
[Page 8] 9 An example of Division. How many pounds, and shillings are in 11388 pence? Divide 11388 by 240: the division is thus. 240 · 1 ∷ 11388 · 47⌊5—
For set the two Armes of the Index at 240, and 1 in the fourth circle: and then bring the Antecedent arme (which stood at 240) unto 11388; and the Consequent arme will shew 47 and almost an halfe.
But how many shillings that excesse doth containe wil appeare, if first you finde by Multiplication that 11280 pence are contained in 47li: which subducted from 11388 there will remaine for the excesse 108 pence. Afterwards by division you may seeke how many shillings are in 108 pence: the diuision is thus. 12 · 1 ∷ 108 · 9.
For set the Armes of the Index at 12 and 1: then bring the Antecedent arme (which stood at 12) unto 108; and the Consequent arme will shew 9.
9 Any Fraction given may bee reduced into Decimal parts, thus.
Set the Antecedent arme of the Index at the Denominator of the Fraction given, in the fourth circle, and the Consequent arme at the Numerator, then keeping the same distance, bring the Antecedent arme unto 1, and the consequent arme will shew the decimal parts.
So [...]40/ [...] is 0⌊75. And 19/48 is 0⌊396—
CHAP. III. Now follow certaine examples of Proportion.
Example I. IF 54 Elnes of Holland bee solde for 96 shillings, for how many shillings was 9 elnes sold? The termes given are 54 · 96 ∷ 9 ·
According to the 2 Chap. 3 Sect. Set one of the armes of the Index at the Antecedent terme 54 in the fourth circle, and the other arme at the consequent terme 96: then keeping that distance, bring the Antecedent arme vnto 9; and the consequent arme beyond the line of the Radius will shew 16 for the fourth proportionall, according to the considerations in the 2 Chap. Sect. 3.
Therefore 54 · 96 ∷ 9 · 16 · are proportionals. And 16 shillings is the price of 9 Elnes.
Example II. If 108 bushels of corne be sufficient for a company of Souldiers keeping a Fort, for 36 dayes, How many dayes will 12 bushels suffice that same number of Souldiers? The termes giuen are 108 · 36 ∷ 12 ·
Set one Arme of the Index at the Antecedent terme 108 in the fourth circle, and the other Arme at the consequent terme 12, (being mindfull of the considerations in the 2 Chap. 3 Sect.) then keeping that same distance, [Page 10] bring the Antecedent arme vnto 36; and the consequent arme will shew 4.
Therefore 108 · 36 ∷ 12 · 4 · shall bee proportionals. And 4 is the number of dayes sought for.
Example III. There is layd vp in a Fort so much corne as will suffice for 756 Souldiers which keepe that Fort, for 196 dayes: how many Souldiers will that same corne suffice for 364 dayes?
The Proportion is reciprocall, therefore the termes given are 364 ∶ 756 ∷ 196 ·
Set one Arme of the Index at the Antecedent terme 364, and the other Arme at the consequent 196: and keeping the same distance, bring the Antecedent arme vnto 756; and the consequent arme will shew 407+: And therefore for so many Souldiers will the corne laid vp suffice for 364 dayes, or 13 moneths.
Example IIII. There is a Tower whose height I would measure with a Quadrant.
I take two Stations in the same right line from the Tower: and at either Station having observed the height through the sights, I finde that the perpendicular cutteth in the nearer Station 28 degrees 7 minutes almost: and in the further Station 21 degr. 58 min. almost: and betweene both the Stations, the distance was 76 feet.
The Rule of measuring heights by two Stations is contained in these Theoremes.
Theor. As the difference of the Tangents of the arches cut in either station, is to the distance betweene [Page 11] the stations; so is the Tangent of the lesser arch, to the nearer distance from the Tower. Againe
Theor. As the Radius is to the Tangent of the greater arch; so is the nearer distance found, to the height.
And therefore because by the 1 Chap. 6 Sect. the Tangents of the arches 28°, 7′—, and 21° 58′—are 5342, and 4032 whose difference is 1310; the proportions will be
First, 1310 · 76 ∷ tang. 21°, 58′—· 234 ·
Wherefore 234 feet is the nearer distance.
Second Radius · tang. 28°, 7′— ∷ 234 · 125 ·
Wherefore 125 feet is the height sought for.
Example V. To finde the Declination of the Sunne the 9th day of May.
The place of the Sunne for every day, may be had nere inough out of this Table, by Adding vnto the place of the Sun in the beginning of that moneth so many degrees, as there are dayes past in that moneth: But if the number of degrees exceed 30, the excesse is to be accounted in the Signe next following.
Wherefore the 9th of May the place of the Sun is ♉ 20+9, that is ♉ 29: which is 59 degr. distant from the next Aequinoctiall point.
Ianuary | ♑ | 21 |
February | ♒ | 22 |
March | ♓ | 20 |
April | ♈ | 21 |
May | ♉ | 20 |
Iune | ♊ | 19 |
Iuly | ♋ | 18 |
August | ♌ | 13 |
Septemb. | ♍ | 18 |
October | ♎ | 17 |
Novemb | ♏ | 18 |
Decemb | ♐ | 19 |
[Page 12] These things being knowne, the Rule is delivered in this Theoreme.
Theor. As the Radius is to the sine of the sunnes distance from the next Aequinoctiall point; so is the sine of the sunnes greatest declination, to the sine of the declination sought for.
The proportion will be Radius · sine 59° ∷ sine 2 [...]°, 30′ · sine 19° [...]9′·
And so much is the Declination sought for.
Example VI. To finde the Right ascension of the Sunne, the 9th day of May.
Seeke the place of the Sunne for the day proposed in the former Table; and the Sunnes distance from the next Aequinoctial point, as in the former example.
These things being knowne, the Rule is by one of these two Theoremes.
Theor. As the Radius, is to the sine of the complement of the sunnes greatest declination; so is the the tangent of the sunnes distance from the next Aequinoctiall point, to the tangent of the distance of the right ascension of the sunne, from the same Aequinoctiall point. Or
Theor. As the tangent of the greatest declination of the Sunne, is to the Radius; so is the tangent of the declination of the sunne for the time proposed, vnto the sine of the right ascension of the sunne from the next Aequinoctial point.
The proportions will be either Radius · sine 66°, 30′ ∷ tang. 59° · tang 56° 46′ ·
Or, tang. 23°, 30′ · Radius ∷ tang. 19°, [...]9′ · sine [...]6° 4 [...]′▪
Of Continuall proportion, Or of Progression Geometricall.
1 THE Ratio of a Progression is the quotient of the consequent terme divided by his antecedent. And therefore in the Instrument it is the distance taken betweene the termes in the fourth circle, by the opening of the Index.
2 To Double, Triple, or Multiply how often soever any Ratio given, is nothing else but so often to put together the said space or distance between the termes, as is shewed in Chap 1. Sect. 7.
As for example, if the Ratio 60, to 65 be proposed to be septupled.
Set the Armes of the Index at 60, and 65: and then with the same opening, bring the Antecedent arme which was at 60, vnto 1, and the consequent arme will cut 1⌊08384 in the fourth circle, and 03476 [...] in the fift circle: this latter number being multiplied by 7 maketh 23444; vnto which number in the fift circle applying the Index, it will in the fourth circle cut 1⌊ [...]2, which is the multiplied number sought for.
But because in a little Instrument, the arch cut in the fift circle, cannot be estimated exactly: and a small error in the beginning often repeated, by multiplying is made great: it is the most safe way, to take the Logarithmes of the termes of the Ratio out of the Canon, and to multiply them by the number given: As I have done in these examples.
100 | 2.0000000 |
104 | 2.0170333 |
105 | 2.0211893 |
106 | 2.0253059 |
106⅔ | 2.0280287 |
107 | 2.0293838 |
107½ | 2.0314085— |
108 | 2.0334238— |
108⅓ | 2.0347621 |
108½ | 2.0354297+ |
108¼ | 2.0364293— |
109 | 2.0374265 |
110 | 2.0313927 |
Or if the Canon be wanting; you may come neerer the marke, if that first single opening of the Index being kept, and the Antecedent arme set at 1; you transferre the Antecedent Arme, unto that place which the consequent arme doth cutt; and the consequent arme will cut the same space duplicated. Then holding the consequent arme in that same place, open the Antecedent arme unto 1. and afterward with that duplicated opening, bring the Antecedent arme to the duplicated space, and the consequent arme will cut the space quadrupled. Thirdly, bring the Anticedent arme unto the quadrupled space and the consequent arme, keeping that duplicated opening, will cut the space sextupled. Lastly, having againe taken a single opening, bring the Antecedent arme unto the number, or space sextupled; and the consequent arme will shew the Ratio sought for septupled.
And this manner of working may bee observed for as many Multiplications as you please of any Ratio given.
[Page 15] 3. The Ratio, and first terme being given, to continue the same unto any number of termes.
Open the Armes of the Index, the one unto the Antecedent of the ratio given, and the other unto the consequent: then the same opening being kept, bring the Antecedent Arme vnto the first terme given, and the consequent arme will shewe the second terme: againe bring the Antecedent arme vnto the second terme found, and the consequent arme will shew the third. After that bring the Antecedent arme unto the third terme found, and the consequent arme wil shew the fourth. And in this manner you may proceed as farre as you please.
As for example, If a Progression in the ratio 2 unto 5, beginning at 8, Or if a Progression in the ratio 100 unto 108, beginning at 5, is to be instituted; the termes in either progression will be as followeth.
1 | 2 · 5 ∷ 8 · 20 |
2 | 20 |
3 | 50 |
4 | 125 |
5 | 312⌊5 |
6 | 781⌊25 |
7 | 1953⌊125 |
1 | 100 · 108 ∷ 5 · 5⌊4 |
2 | 5⌊4 |
3 | 5⌊832 |
4 | 6⌊29856 |
5 | 6⌊8024448 |
6 | 7⌊346640384 |
7 | 7⌊93437161472 |
[Page 16] 4 Theor; The ratio of any former terme, in a row of concinuall proportionals, vnto any of the termes following, is aequall to the ratio of the first terme unto the second, multiplied into it selfe according to the distance of that latter terme from the former.
As for example, The Ratio 5⌊4 unto 6⌊ [...]024448 which is the third terme from it, is aequall to the ratio of 100 vnto 108 triplicated, Or as the Cube of 100 unto the Cube of 108. Wherefore
5 The Ratio, and the first terme of the Progression being given, to finde out any other terme required.
First, multiply the ratio given into it selfe, according to the distance of the terme sought from the first terme, by the 2 sect: then say
As 1 is to that mul [...]ple found; so is the first terme, to the terme sought for.
Example, What will be the amount of 26th, in 7 yeares by Interest upon Interest, after the rate of 20 pence in the pound?
Because 1 pound which is 20 shillings containeth 60 groates, and 20 pence conteine 5 groates, the rate of the Interest will bee 60 unto 65, Or 100 unto 108⌊ [...] × [...] But the first terme is given 26, unto which there are to be acquired 7 other termes in continuall proportion.
First, by the 4 Chap: and 2 Sect. Let the ratio given be septuplicated, that is multiplied sevenfold into it selfe, which will be 1⌊552. Then set the consequent arme of the Index vnto the septuplicate number 1⌊552, and open the Antecedent arme vnto 1; and keeping the same opening, [Page 17] bring the Antecedent arme unto 26; and the consequent arme will shew 45⌊5312li the amount sought for.
6 The Ratio, and any other terme of the Progression being given, to finde the first terme.
First multiply the Ratio given into it selfe according to the difference of the terme given from the first terme. Then say
As that multuple is unto 1; so is the terme given, unto the first terme.
Example, what summe in 7 yeares did amount unto 45⌊5312li by Interest upon Interest after the rate of 100 unto 108⌊33+?
First the ratio being septuplicat, by the 4 Chap. 2 Sect. will be 1⌊7512. Then setting the Antecedent arme of the Index to that septuple 1⌊7512, open the consequent arme unto 1: and keeping the same opening, bring the Arme unto 45⌊5312li: and the consequent arme will shew 26, which was the stocke, or summe of money, from which that amount did arise.
7 The Ratio, the First terme, and any other terme of a Progression being given, to finde how many places the terme given is from the first terme.
First say, As the first terme is unto 1; so is the other terme given, unto the ratio multiplied into it selfe according to the distance of that terme from the first.
Wherefore according to 1 Chap. 7 Sect. and 3 Chap. 2 Sect. by helpe of the fift circle, see how often the ratio given, is contained in that multuple found.
Example, In how many yeares did 26li, by Interest [Page 18] upon Interest after the rate of 100 unto 108⌊33+ + increase unto 45⌊5312li?
First set the Antecedent arme of the Index at 26, and the consequent arme at 1: and keeping the same opening bring the Antecedent arme vnto 45⌊5312, and the consequent arme will shew 1⌊7 [...]12: to which in the fift circle answereth 24333. Then because unto the consequent terme of the ratio 108⌊33+ + there agrees in the fift circle 03476, divide 24333 by 03476, and the quotient will be 7, the number of yeares sought for.
8 The First terme, and any other terme of the Progression being given to finde the ratio of the Progression.
First say, As the first terme is unto 1: so is the other terme given, unto the ratio multiplied into it selfe according to the distance of that terme from the first.
Wherefore according to Chap. 1. Sect. 7, by helpe of the fift circle, Let the multuple found be divided by the distance of the terme from the first.
Example, 26li by Interest upon Interest in 7 yeares amounted unto 45⌊5312: what was the ratio of the Interest compared unto 100?
First set the Antecedent arme of the Index at 26, and the consequent arme at 1: and then keeping the same opening, bring the Antecedent arme unto 45⌊5312: and the consequent arme will shew 1⌊7 [...]12: unto which in the fift circle answereth 24333 and this number being divided by 7 will give 03476+: unto which agreeth in the fourth circle 108⌊33+ + the consequent terme of the Interest sought for.
9 Two numbers being given to finde as many Midle proportionals betweene them as you will.
[Page 19] Divide the distance of the greater number given from the lesser in the fourth circle iustly taken, according to Chap. 1. Sect. 7, by helpe of the fift circle into equall segments, one more then are the number of Midle proportionals sought for. All these segments added orderly to the first terme, doe distinguish the termes of the Progression which you seeke.
Example, Let there be foure Midle proportionals, sought out betweene 8 and 19⌊90656.
Apply the Index unto 8 in the fourth circle, and it will cut in the first circle 9039: also set the Index unto 19⌊91—in the fourth circle, and it will cut in the fift circle 2989; which number because it reaches beyond the Vnite [...]ne, is indeede 12989, according to Chap. 1. Sect. 7, and so is the distance iustly taken. Then subducting 9039 from 12989, there will remaine 3950: which divided by 4 + 1, the quotient will give 790. wherfore 9039 + 790, scil. 9829 in the fift circle doth agree with 9⌊6 in the fourth circle, which is the first midle proportionall. And 9039 + twise 790, scil. 10619 in the fift circle doth agree with 11⌊52 in the fourth circle, which is the second midle proportionall. And in this manner 13⌊824, and 16⌊5888 will be found the third and fourth midle proportionals.
10 Theor. If from the Ratio given, being multiplied in it selfe according to the number of termes, you subduct 1, and multiply the remainder, by the antecedent of the ratio. It will be
As the difference of the termes of the ratio, is unto the product; so is the first terme, to the sum of the Progression.
As for example if the Ratio of the Progression be R to S: and the difference of R taken out of S be D. and the first terme of the Progression α: and the whole summe of the termes Z it shall be, [Page 20] D · rat. multa— 1 in R ∷ α · Z.
Which is the very Theoreme it selfe expressed in Symboles of words: that it may more easily be fixed in the phantasie. Which proportion also wee must consider, doth hold both alternly, and conuersly.
This Theoreme may otherwayes be expressed, by the equality which the product of the two midle termes hath to the product of the two extreames, thus Ratio multiplicata—1 in R in α = Z in D.
This manner of setting downe Theoremes, whether they be Proportions, or Equations, by Symboles or notes of words, is most excellent, artificiall, and doctrinall. Wherefore I earnestly exhort every one, that desireth though but to looke into these noble Sciences Mathematicall, to accustome themselues unto it: and indeede it is easie, being most agreeable to reason, yea even to sence. And out of this working may many singular consectaries be drawne: which without this would, it may be, for ever lye hid. As in this present proportion: because it is D · rat. multa—1 in [...] ∷ α · Z · wherefore Rat. multa—1 in R · D ∷ Z · α · And α · Z ∷ D · rat. multa—1 in R
These are exceeding easie: but this following is more difficult, and requireth attention.
In the former equation it was Rat. multa—1 in R in α = Z in D
Now because Rat. multa—1 in R in α, and Rat. multa [...] in R in α—R in α, and Rat. multa in R—R in α, [Page 21] and Rat. multa in α—α in R, are equall one to another, and also to Z in D, these aequations shall also be consectarious. [...] and [...] and [...] and [...]
And besides these many more. The practise whereof I leave to the industry of the studious Reader, especially having delivered the whole Art of such operations in my Clavis Mathematica.
Some of these I have occasion to use in the sections following.
11. Therefore the Ratio of a Progression, and the first terme, and the number of termes being given, to finde the summe of the whole progression.
For this operation the rule, or Theoreme last before serveth: for by it [...]
[Page 22] Example. If an Annuity of 5li, be detained 7 yeares, what will be the amount thereof by interest upon interest after the rate of 100 unto 108?
Now because the Amount is the summe of the Progression, whereof the first terme is the annuitie, Multiply the ratio into it selfe according to the number of yeares, by Chap. 4. Sect. 2, and it will be 1⌊71382: from which if you subduct an vnite, there remaines 0⌊71382, which multiplied by 100 maketh 71⌊382: then set the Armes of the Index at 1 and 71⌊382; and bring the Antecedent arme which stood at 1, unto 5 the first terme: and the consequent arme will cut 356⌊915 (that is Rat. multa—1 in R in α) and lastly this number being divided by 108—100, scil. by 8, the quotient will give 44⌊6 [...]40, for the summe of the whole progression: and so much is the amount sought for.
12. The Ratio, the Number of Termes, and the Summe of a Progression being given, to find the first terme.
By the converse of the foregoing Theoreme, it is manifest, that Rat ∶ multa—1 in R · D ∷ Z · α ·
The declaration in words was in the 10 Sect.
Example. If an Annuitie detained 7 yeares by Interest upon Interest, after the rate of 100 unto 108, did increase unto 44⌊6140li. how much was that Annuitie?
Multiply the Ratio into it selfe according to the number of yeares (per cap. 4. sect. 2.) and the product will be 1⌊7 [...]82: from which if you subduct an Vnite, there remaines 0⌊7 [...]82: this being multipled by 100 doth make 71⌊ [...]82. Then say 71⌊382 · 8 ∷ 44⌊6140 · 5 · [Page 23] for the First terme: which was the Annuitie sought for.
13 The Ratio, the First terme, and the Summe of the Progression being given, to find the Number of termes.
By the Theoreme in the 10. Sect. it was α · Z ∷ D · rat. multa—1 in R ·
Wherefore set the Antecedent arme of the Index unto the Antecedent terme of the ratio, and the consequent arme unto the Summe of the Progression: and with that same opening, bring the Antecedent arme unto the difference of the termes of the ratio; and the consequent arme wil shew a number (that is Rat. mul.—1 in R;) which if you divide by the Antecedent terme of the ratio, and unto the quotient adde an Vnite, you shall have the ratio multiplied into it selfe according to the number of termes. Therefore taking the distance betweene the termes of the ratio, with the armes of the Index, measure by helpe of the fift circle (per Cap. 4. Sect. 7.) how often that distance may be found in the multiplied ratio: for so many are the termes of the progression.
Example. If an Annuitie of 5li detained by Interest upon interest after the rate of 100 to 108, increased unto 44⌊6140li. How many yeares was the Annuitie detained?
Set the Antecedent arme of the Index at 5, and the consequent arme at 44⌊6140, and with the same opening bring the Antecedent arme unto 8, and the consequent arme will shew 71⌊382 (that is Rat. multa—1 in R:) this number being divided by 100, will be 0⌊71382: and if unto the quotient you adde 1, you shall have 1⌊71 [...]82 (the ratio multiplied into it selfe according to the number of yeares:) unto which in the fift circle answereth 2338: [Page 24] but unto 108 in the fift circle there answereth 0334. divide therefore 2338 by 0334; and the quotient will be 7, for the number of yeares sought for.
Or such questions may be more easily performed by this Theoreme, which the industrious Reader may by himselfe practise. [...]
14 Theor. If the summe of the whole progression be divided by the ratio multiplied into it selfe according to the number of termes, the quotient will be the first terme; and that summe given will be the last terme, of another progression, having the same ratio but one terme more.
15 And because a summe of mony the amount whereof in any number of yeares given, by Interest upon interest, doth equall an Annuitie so long detained, is equivalent to the same Annuitie; and the amount of an Annuitie is the summe of a Progression continued from that Annuitie. If therefore an Annuitie for any number of yeares be divided by the ratio multiplied into it selfe according to the number of yeares; the quotient will be the just price of an Annuitie to endure for so long. And because by the 10 and 11 Sect. it hath beene shewed that [...].
Therefore by the 14 Sect. [...] will be equall to the price of an Annuitie in ready money, which shall be the Rule for the operation following.
[Page 25] Wherefore also Rat. multa—1 in R in α = Rat. multa in D in Pret. which proportion is thus enuntiated in words.
Theor. If from the Ratio multiplied into it selfe according to the Number of yeares you subduct an Vnite, and the remainder be multiplied continually by the Antecedent of the Ratio, and the Annuitie it selfe: And againe, If the Ratio multiplied into it selfe, according to the number of yeares be multiplied continually by the difference of the termes of the Ratio, and by the Price: both those products will be equall.
Example. An Annuitie of 5li, to endure for 7 yeares, is to be sold: what is it worth in ready money, after the Rate of 100 unto 108?
The Ratio multiplied into it selfe according to the number of yeares (per Cap. 4 Sect. 2) is 1⌊7138: subduct 1, and there will remaine 0⌊71382: which multiplied by 100 maketh 71⌊382. Then set the Antecedent arme of the Index at 1, and the consequent arme 71⌊382: and keeping that same opening, bring the Antecedent arme unto 5; and the consequent arme will shew 356⌊915; keepe this (for it is [...]. After that set the Antecedent arme of the Index at 1, and the consequent arme unto the multuple ratio 1⌊7138; and with the same opening bring the Antecedent arme unto 8; and the consequent arme will cut 13⌊7106, keepe this number also (for it is Rat. mul. in α). Lastly, place the Antecedent arme of the Index at 13⌊7106, and the consequent arme at 1; and with the same opening bring the Antecedent arme vnto 356⌊015: and the consequent arme will shew 26⌊032li. [Page 26] which is the iust Price of an Annuitie of 5li in readie money.
16 And by the last praecedent Theoreme or Rule, also [...] which Theoreme may bee enuntiated in words as was there shewed.
Example. An Annuitie for 7 yeares is bought for 26⌊032li. after the rate of 100 unto 108, by Interest upon interest: how much was that Annuitie?
The Ratio multiplied into it selfe for the number of 7 yeares (per Cap: 4, Sect. 2) is 1⌊7138: which multiplied continually by 8, and by the price, doth make 356⌊915. Divide this number found, by 71⌊382, (which is the multuple ratio) it selfe lesse by an Vnite, and multiplied by 100: and the quotient will be 5li, the Annuitie sought for.
17. Also by Ratiocination from that praecedent rule will follow this proposition [...] which is thus enuntiated in words.
Theor. If the product of the Antecedent of the ratio multiplied by the Annuitie be divided by it selfe, being diminished by the product of the difference of the termes of the ratio multiplied by the Price: the quotient will bee equall to the ratio multiplied into if selfe according to the number of yeares. As
If the ratio be 100 unto 108; the Annuitie 5li: and the price thereof 26⌊032li. Set the Antecedent arme of [Page 27] the Index at 1, and the consequent arme at 8, the difference of the termes of the ratio: and with the same opening bring the Antecedent arme unto 26⌊032—: and the consequent arme will shew 208⌊256: which subducted from 500, there will remaine 291⌊744, for the divisor. Set therefore the Antecedent arme of the Index at the divisor 291⌊744, and the consequent arme at 1: and with the same opening, bring the Antecedent arme unto the dividend 500: and the consequent arme will shew 1⌊71 [...]8, which is the ratio multiplied into it selfe according to the number of yeares. And by this number so found it will be easie (by helpe of the fift circle) the ratio of the Interest being given, to finde the continuance of the Annuitie.
Example. An Annuitie of 5il, was bought for 26⌊032li—, after the rate of 100 unto 108: how many yeares is it to last?
First seeke out the ratio multiplied into it selfe according to the number of yeares, which will be 1⌊71 [...]8, according as was even now shewed in this Sect. to this in the fift circle there answereth 2338: but unto 108 there answereth in the fift circle 0334. Divide therefore 2338 by 0334; and the quotient will be 7 for the number of yeares sought for.
CHAP. V. Of the Quadrating, and Cubing of Numbers, Sides or Rootes: and of the Extraction of the Quadrate, and Cubic side, or roote, out of Numbers, or Powers given.
1 IF a number, side, or roote be multiplied into it selfe; the product will be a Quadrat. And if a quadrate bee multiplied into his owne side, or roote, the product will be a Cube. Wherefore 1 · N ∷ N · Q · and 1 · N ∷ Q · C ·
2 If therefore a number be given to be Quadrated. Set the Antecedent arme of the Index at 1, and the consequent arme at the number given: then with the some opening bring the Antecedent arme to the number given; and the consequent arme will shew the Quadrat thereof.
And the number of figures in a Quadrat of a single root (or which doth not exceede 9) is easily found out by those Rules, that have beene before delivered concerning Multiplication. But if a side or root consist of more figures then one; for each figure after the first it acquireth two more places of figures. And if any of the figures of the root given be decimal parts, cut off from the Quadrat found, twice so many of the last figures for decimals.
Example 1. The Quadrat of the side 7 is required. Say 1 · 7 ∷ 7 · 49 Set therefore the Antecedent arme of the Index at 1, and the consequent arme at 7; and with that opening [Page 29] bring the Antecedent arme unto 7; and the consequent arme will shew 49 which is the Quadrat sought for.
Example 11. The Quadrat of the side 57 is required.
Set the Antecedent arme of the Index at 1; and the consequent arme at 57: then with that same opening bring the antecedent arme unto 57; and the consequent arme will shew 3249, which is the Quadrat sought for, consisting of foure places.
Example 111. The Quadrat of the side, or root 570 is required.
Having found as before, 3249 for the quadrat of the side 57: put thereunto two circles: and it will bee 324900, the quadrat sought for.
Example 1111. The quadrat of the side 574 is required.
Set the Antecedent arme of the Index at 1, and the corsequent arme at 574; and with the same opening bring the Antecedent arme unto 574; and the consequent arme will shew 329476, the quadrat sought for consisting of sixe figures: but the two last figures cannot at all be discerned by the Instrument.
3 If a number be given to be Cubed.
Set the Antecedent arme of the Index at 1, and the consequent arme at the number given; and with that same opening, bring the Antecedent arme unto the number given; and the consequent arme will shew the Quadrat; then bring the Antecedent arme unto the Quadrat, and the consequent arme with that same opening will shew the Cube of that side given.
The number figures in a Cube of a single side, or root which doth not exceede 9, is easily found by that which hath beene before delivered concerning Multiplication: [Page 30] But if the side, or root consist of more figures then one; for each figure after the first it obtaineth three more places of figures. And if any of the figures of the root given be decimal parts, cut off from the Cube found thrice so many of the last figures for decimal parts.
Example. The Cube of the side, or root 7 is required. Say, 1 · 7 ∷ 7 · 49 · againe 1 · 7 ∷ 49 · 343 ·
Set therefore the Antecedent arme of the Index at 1, and the consequent arme at 7; and with that opening bring the Antecedent arme unto 7, and the consequent arme will shew 49 the quadrat thereof: Then set the Antecedent arme at 49; and the consequent arme (with that first opening) will shew 343, which is the desired Cube of the side proposed.
Another example, The Cube of the side, or root 57 is required.
Set the Antecedent arme of the Index at 1, and the consequent arme at 57; and with that same opening bring the Antecedent arme unto 57; and the consequent arme will shew the quadrat 3249. Then set the Antecedent arme at 3249; and the consequent arme keeping the former opening will shew 185193, which is the required Cube of that side proposed, consisting of six places: but the two last figures cannot be known by the Instrument.
Example III. The Cube of the side 570 is required.
Hauing found as before the Cube of the side, or root 57 to be 185193: put thereunto three circles; and it will be 185 193000 the Cube sought for.
Examples of greater Cubes, it will be needlesse to set downe.
[Page 31] 4 The Extraction of the Square, or Quadrat root, or side, is done by helpe of the fift circle, after this manner.
Set the Index at the Quadrat proposed; and of that number which it cuts in the fift circle, take halfe: then set the Index at that halfe; and it will shew in the fourth circle, the side, or root sought for.
But you must know that if the number which is the Quadrat proposed, have onely two places of Integers, the side, or root consisteth of one figure. But if it have more places of Integers, dividing them by 2, the quotient will give the true number of figures in the root, if it measure it exactly; or one lesse then the true number if any thing remaine.
Example I. The side, or root of the Quadrat 49 is required.
Set the Index at 49 in the fourth circle, and it will cut in the fift circle 6902; indeede 1. 6902 having the graduall number 1 praefixed, because 1 in the fourth circle signifieth 10, one circuition thereof being finished: the halfe whereof is 0. 8451. Then set the Index at 0. 8451, in the fift circle; and it will cut in the fourth circle 7, the side, or root sought for.
Example II. The side, or root of the quadrat 3249 is required.
Set the Index at 3249 in the fourth circle, and it will cut in the fift circle 5118; indeede 3. 5118 prefixing the gradual number 3, because 1 in the fourth circle signifieth 1000, three circuitions thereof being finished: the halfe whereof is 1. 7559. Then set the Index at 7559, omitting the prefixed graduall number 1; and it will shew in the fourth circle 57 the side sought for, consisting of two figures, because 1 in the fourth circle signifieth 10.
[Page 32] Example III. The side of the quadrat 329476 is required.
Set the Index at 329476 in the fourth circle, and it will cut in the fift circle 5178; indeede 5. 5178 prefixing the graduall number 5, because 1 in the fourth circle signifieth 100000, five circuitions thereof being past over; the halfe whereof is 2. 7589; Then set the Index at 7589, omitting the graduall number 2 prefixed thereto; and it will shew in the fourth circle 574 the side, or root sought for, consisting of three figures, because 1 in the fourth circle doth signifie 100.
5 The Extraction of the Cubic roote, or side is done by helpe of the fift circle after this manner.
Set the Index at the Cube proposed; and that number which it cuts in the fift circle divide by 3. Then set the Index at that third part, and it will shew in the fourth circle the side, or roote sought for.
And you must know that if the Cube proposed have onely three places of Integers, the side, or roote thereof consisteth of one figure: But if it have more places of Integers; divide them by 3, the quotient will give the true number of the figures of the Root, if it measure it exactly; or one lesse then the true number if any thing remaine.
Example I. The side, or roote of the Cube 343 is required.
Set the Index at 343 in the fourth circle, and it will cut in the fift circle 5353; indeede 2. 5353 prefixing the graduall number 2, because 1 in the fourth doth signifie 100, two circuitions thereof being past over: the third part whereof is 8451. Then set the Index at 8451, and it will shew in the fourth circle 7, the side sought for.
[Page 33] Example II. The side, or roote of the Cube 185193 is required.
Set the Index at 185193 in the fourth circle; and it will cut in the fift circle 2677; indeede 5. 2677 prefixing the graduall number 5, because 1 in the fourth circle doth signifie 100000, five circuitions thereof being past over: the third part whereof is 1. 7599. Then set the Index at 7599, omitting the prefixed graduall number 1; and in the fourth circle it will shew 57, the side, or root sought for, consisting of two figures, because 1 in the fourth circle doth signifie 10.
Examples of greater Cubes it will be needlesse to set downe.
CHAP. VI. Of Duplicated, and Triplicated proportion. And first of Duplicated proportion.
Theoreme. LIke Plaines are in a Duplicated ratio, that is, As the Quadrats of their homologal sides. And therefore questions in the which the sides of like planes are compared, doe appertaine vnto this place.
And it is to be noted, that if three numbers be given, in which As the quadrat of the first, is unto the quadrat of the second; so ought the third to be unto a number sought for. Let it be thus done, As the first number, is to the second; so is the third to afourth; And againe As the first number, is to the second; so is the fourth now found, to the number sought for.
Example I. There are two like rectangle Areae, or plaines, the length of the greater, is 40 feete, the length of the lesser 24 feet: each of them paved with paving tiles; the greater hath 1200 tiles: how many shall the lesser have?
The Areae, or plaines are one to the other, as the quadrats of the longitudes given. And the proportion is direct. Say therefore 1600 (Q ∶ 40) · 576 (Q ∶ 24) ∷ 1200 · 432 · which is the number of tiles contained in the pavement of the lesser Areae, or plaine.
Example II. How many Acres of woodland measured with a Perch, of 18 feete, are there in 73 Acres of champane land, measured with a Perch of 16½ feete?
[Page 35] The measures given (18, 16½) being reduced into their lest termes, are as 12 unto 11: and the quadrats of these numbers, are, 144, and 121. And the Proportion is Reciprocall. Say therefore 144 (Q ∶ 12) · 121 (Q ∶ 11) ∷ 73 · and so many are the Acres of Wood land.
Of Triplicated proportion.
3 Theor. Like Solids are in a Triplicated ratio, that is, As the Cubes of their homologal sides. And therefore questions in which the sides of like solids are compared, doe appertaine unto this place.
4 If three numbers be given in the which, As the Cube of the first is to the Cube of the second; so is the third number to a number sought for. Let it be thus done, As the first number is to the second; so is the third to a fourth: Againe, As the first is to the second; so is the fourth now found unto a fift. And thirdly, As the first is to the second; so is that fift to the number sought for.
Example. If 4 [...]/100lib. of gunpowder, suffice to charge a Gun, whereof the concave diameter is inch 1½. How many pounds of powder will suffice to charge a Gunne, whose concave diameter is 7 inches?
The capacities are one to another, as the Cubes of the diameters. And the proportion is direct. Say therefore 3⌊375 (C ∶ 1⌊5) · 343 (C ∶ 7) ∷ 0⌊43 · 4 [...] + wherefore 43⌊ [...] lib. of Gunpowder, will bee needfull to be had.
[Page 36] Another example, 43⌊7lib. of Gunpowder are sufficient to charge a Gun, whose diameter in the concave is 7 inches: now there is another sort of Gunpowder, much more strong and forcible, that is in strength unto the former, as 5 vnto 2: How much of this stronger powder, will suffice to charge a Gun of 4 inches diameter?
Here are two operations: the first seekes out, how much of that stronger powder sufficeth to charge a Gun of 7 inches diameter: and the proportion is reciprocall, that is 5 · 2 ∷ 43⌊7 · 15⌊48
The second operation is like that in the former example. 343 (C ∶ 7) 64 (C ∶ 4) ∷ 15⌊48 · 3⌊ [...]
CHAP. VII. Concerning the Measuring of Circles, Cones, Cylinders, and Sphaeres.
1 ARchimedes in a peculiar Treatise found the proportion of the Diameter of a circle to the Circumference to bee a very smale deale greater then o [...] 7 unto 22: And of late Ludolph Ʋan Ceulen insisting in the same steps of Archimedes, hath more precisely found it to be of 1 vnto 3⌊141592653589793 but for our Instrument it will be sufficient to take the ratio of 1 vnto 3⌊1416, Or of 0⌊3183+ unto 1: leaving the diligent practizer, to more exactnesse, if he please to use his Pen.
And note that the Rules following are set downe in proportions, to be wrought as hath been taught in Chap. 2, Sect. 3. Wherein
- D, or Diam. signifieth the Diameter.
- Dq, or Q. Diam. the Quadrat of the Diameter.
- Dc, or C. Diam. the Cube of the Diameter.
- R, or Rad. the Radius, or Semidiameter.
- P, or Perif. the Periferie, or Circumference.
- Pq, the Quadrat of the Periferie.
- Long. the length.
- L the side, or latus
- Alt. the altitude.
- [...], sheweth that the two magnitudes betweene which it is set, are to be multiplied together.
In a Circle.
2. The Diameter of a circle being given, to finde the Periferia. Say, 7 · 22, Or 1 · 3⌊1416 ∷ Diam · Perif ·
Example. A circle is given, the Diameter whereof is 12, I would know the circumference, or Periferia of it. Say, 1 · 3⌊1416 ∷ 12 · 37⌊6992 ·
3 The Periferia of a circle being giuen, to finde the Diameter. Say, 22 · 7, Or 1 · 0⌊3183 + ∷ Perif · Diam ·
4 The Diameter of a circle being giuen, to finde the Area. Say, 7 × 4 · 22, Or 1 · 0⌊7854 ∷ Q ∶ Diam · Area · Or els 1 · 3⌊1416 ∷ Q ∶ Rad · Area ·
Example. A circle is giuen, the diameter whereof is 12, I would know the content, or Area of it. Say, 1 · 0⌊7854 ∷ 144 (Q ∶ 12) · 113⌊ [...]76 · Or 1 · 3⌊1416 ∷ 36 (Q ∶ 6) · 113⌊0176
5 The Area of a circle being giuen, to finde the Diameter. Say, 22 · 7 × 4, Or 1 · 1⌊27324 ∷ Area · Q ∶ Diam ·
Example. A circle is giuen, the content whereof is 113⌊0976, I would know the Diameter of it. Say, 1 · 1⌊27324 ∷ 113⌊0976 · 144 ·
[Page 39] 6 The Periferia of a circle being giuen, to finde the Area. Say, 22 × 4 · 7, Or 1 · 0⌊0795775 ∷ Q ∶ Perif · Area ·
7 The Area of a circle being giuen, to finde the Periferia. Say, 7 · 22 × 4, Or 1 · 12⌊ [...]6637 ∷ Area · Q ∶ Perif ·
In a Cone.
8 The side of a right Cone, and the Diameter of the base being giuen, to find the Superficies. Say, 7 · 22, Or 1 · 3⌊1416 ∷ ½ D × L · Superf ·
Example. A Cone is giuen, whereof the side is 18, and the diameter of the base 12, I would know the superficies of it. Say, 1 · 3⌊1416 ∷ 108 (½ D × L) · 33⌊ [...]2928 ·
9 The Axis, or height of a right Cone, and the Diameter of the base, being giuen, to find the Soliditie. Say, 7 × 4 · 22, Or 1 · 0⌊7854 ∷ Dq in 1/ [...] Axis · Soliditie ·
Example. A Cone is giuen, whereof the Axis is 18, and the Diameter of the base 12, I would know the Solidity. Say, 1 · 0⌊7854 ∷ 864 (Dq in 1/ [...] axis) · 678⌊2856 ·
In a Cylinder.
10 The side of a right Cylender and the Diameter being given, to finde the Superficies. say, 7 · 22, Or 1 · 3⌊1416 ∷ Diam ∶ × axem · Superfic.
11 The Side of a right Cilinder, and the Diameter being given, to finde the Soliditie. Say, 7 × 4 · 22, Or 1 · 0⌊7854 ∷ Dq × L · Soliditie ·
12 The Side of a right Cylinder, and the Circumference P, being given, to finde the Soliditie. Say, 22 × 4 · 7, Or 1 · 0⌊0795775 ∷ Pq × L · solidit ·
In a Sphaere.
13 The Axis, or Diameter of a Sphaere being given, to finde the Superficies. Say, 7 · 22, Or 1 · 3⌊1416 ∷ Dq · Superficies ·
14 The Superficies of a Sphaere being given, to finde the Axis. Say, 22 · 7, Or 1 · 0⌊31831 ∷ Superfic · Dq ·
15 The Segment of a Sphaere being given, to finde the Superficies. Say, 7 · 22, Or 1 · 3⌊1416 ∷ Q ∶ chord of ½ Segm. · Superfic ·
[Page 41] 16 The Axis, or Diameter of a Sphaere being giuen, to finde the Soliditie. Say, 7 × 6 · 22, Or 1 · 0⌊5236 ∷ Dc · Soliditie ·
Example. A Sphaere is giuen, whereof the Axis is 12, I would know the solidity of it. Say, 1 · 0⌊5236 ∷ 1728 (Dc) · 59 [...] ⌊6208 ·
17 The Soliditie of a Sphere being giuen, to finde the Axis. Say, 22 · 7 × 6, Or 1 · 1⌊90986 ∷ Soliditie · Dc ·
Example. A Sphaere is giuen, the Solidity whereof is 590⌊6208, I would know the Axis thereof. Say, 1 · 1⌊90986 ∷ 590⌊6208 · 1728 (Dc) ·
18 A Segment of a Sphere being giuen to finde the Soliditie. Say,
First. As the altitude of the other Segment, is to the altitude of the Segment giuen: so is that altitude of the other Segment increased by halfe the Axis, vnto a fourth. Then againe say, As 7×3 is to 22, Or as 1 is to 10472: so is the product of the quadrat of halfe the chord of the Periferia of that Segment, multiplied by that fourth, to the Soliditie. Viz. 7 × 3 · 22, Or 1 · 1⌊0472 ∷ Q ∶ chorde in quartam · Solidit ·
19 For note that a Sphaere, is equall to two Cones, having their height and the diamerer of their base, the same with the Axis of the Sphaere. Or which is all one, A Sphaere is two third parts, of a Cylinder, having the height and the diameter of the base the same with the Axis of the Sphaere.
CHAP. VIII. Concerning Plaine, and Solide Measures.
1 THe diuiding of the Carpenters ruler into Inches, and halfe, and quarters, and halfe quarters of Inches, that is of every Inch into eight parts, is most inartificiall, and vnfit for measuring, by reason of the manifold denominations, which must be brought into one, and is hard to bee done of them that are vnskilfull. I would wish therefore that euery Inch were diuided into 10 parts, or rather that the foot were diuided into 100 parts, which is best of all: for then there will neede no reduction. And all other divisions must bee reduced vnto this, by these Rules following.
2. If the measures be taken vpon a Ruler diuided into Inches and tenth parts of an Inch, first take out all the whole feet, and then diuide the Inches remaining, with their decimall parts if there be any by 12.
Example. How many feet and decimall parts of a foot, are in Inches 17⌊3?
First take out the whole foot which is 12 Inches, and there will remaine Inches 5⌊3: which being diuided by 12, you shall haue 442 thousand parts almost: wherefore Inches 17⌊3, is feet 1⌊442—. And contrariwise, feet 1⌊442—, shall be reduced into Inches 17⌊ [...], being multiplied by 12.
3. If the measure bee taken vpon a Ruler diuided into inches and halfe quarters, that is each inch into 8 parts, First you must reduce the eight parts into decimals of Inches, by diuiding the number of parts given by 8 the Denominator thereof: and afterward by the former [Page 43] Rule, reduce the Inches, and decimall parts, into decimall parts of a foot.
Example. How many feet, and decimall parts of a foot, are in 7 inches, and 5 eight parts?
First diuide the 5 eight parts by 8, and you shall haue 625 thousand parts: which being put to 7 inches, will make inches 7⌊625: Again diuide these by 12, as was shewed in the former rule: and the whole measure will be feete 0⌊635. And contrariwise feet 0⌊635, will be reduced into inches 7⌊625, being multiplied by 12.
4. I must aduise all those that haue occasion, to measure Plaines, or Solids, to make themselues very perfect in this kind of Reduction (because most Rulers they shall ordinarily meet withall, are diuided into inches, and halfe quarters) which will be very easie to them, if they doe but remember, that In diuision the first terme of the proportion implyed, is the Diuisor it selfe: but in Multiplication, the first terme is euermore 1. as hath beene shewed in Chap: 2, Sect: 7. And therefore, presuming on the diligence of the Practiser herein, I shall not neede in this kind of measuring, to speake any more of inches, but of feet and decimall parts of feet, as if the Ruler were so diuided.
Of Plaine measures.
5. A Parallelogram, or foure sided rectangle Superficies, being proposed, to find the length of a Superficiall foote.
Take with your Ruler the breadth thereof in feet, and decimals of a foot: and by the breadth so taken diuide 1. the quotient shall be the length of a superficiall foot.
Example. A boord is feet 1⌊17 broad, how much thereof will make a foot?
[Page 44] Diuide 1 by 1⌊17, the quotient will bee 0⌊855 almost: so much shall the length of a foot be, which multiplying the parts by 12, will giue inches 10⌊26. And againe those parts multiplied by 8, will giue 2 eight parts of an inch.
Example, II. In tileing, or healing they vse to reckon by the Square, which is 10 foot euery way, in all 100 [...]eet. There is roofe, feet 16⌊2 [...] broad, how much thereof maketh a Square?
Diuide 100 by 16⌊25 the quotient will be 6⌊ [...]4 almost: so much shall be the length of one square; which multiplying the parts by 12, will be 6 feet, and inches 1⌊8 [...]—almost. And againe those parts multiplied by 8, will giue somewhat more then 6 eight parts of an inch.
Example, III: In pauing they vse to reckon by the yard, which is 3 feet euery way, in all 9 feet. There is a roome to bee paued, which is feet 17⌊35 broad; how much thereof maketh a yard?
Diuide 9 by 17⌊35, the quotient will be 0⌊519 almost, the length of one yard.
6: A fower sided rectangle Superficies, with all the opposite sides parallell being proposed, to find the content.
Take with your Ruler both the breadth and length of and multiply the one number into the other.
Example, A board is feet 1⌊17 broad, and feet 16⌊32 long: how many feet doth it containe in all?
Multiply 16⌊3 [...] by 1⌊17 the product will be feete 19⌊ [...] almost: the whole quantity of that board.
Example. II. A certaine barne tiled, hath the breadth [Page 45] of the roofe feet, 16⌊2 [...], and the length of the barne is feet 47, how many squares of tiling hath it?
Double the length (that you may haue both sides of the roofe) and it will be 94, which being multiplied by 16⌊25, will giue feet 1527⌊ [...]. Againe diuide those feete by 100, so shall you haue squares 15⌊275.
Example. III. A certaine hall paued hath the breadth feet 17⌊35, and the length feet 30⌊5, how many yards doth it containe?
Multiply 17⌊35 by 30⌊5, the product will be feet 229⌊175. Diuide these by 9 and the quotient will bee yards 58⌊797.
7. A fower sided Superficies with the two sides of length onely parallel being proposed, to find the content thereof.
Take with your Ruler the length of the two parallell sides thereof: adde both those numbers together, multiply halfe that summe, by the breadth of the Superficies taken the nearest way over, and the product will bee the content thereof.
Example. A Trapezium, or fower sided figure is proposed, hauing two sides thereof parallell, the length of the longer parallel side is feete 18⌊75 and the length of the shorter side is feete 14⌊4 [...], the breadth thereof being taken the nearest way over is feete 12⌊5, I would know how many feete are contained in the whole Superficies?
The length of the parallell sides are feet 18⌊ [...]5, and 14⌊45, which added together make 33⌊ [...], halfe whereof is 16⌊ [...], which multiplied by the breadth 12⌊ [...], the product will be 207⌊5, so many feet are contained in the superficies of the Trapezium proposed.
[Page 46] 8. A fower sided Superficies which hath none of the sides parallel, as also euery plaine figure of more sides the fower being proposed, must with Diagoniall lines bee diuided into triangles. And note that euery such figure containeth so many triangles as it hath sides, abating two out of the number. Then those triangles are to be measured seuerally as followeth.
9 To find the content, or Area of a Triangle.
Take the perpendicular height, or neerest distance betweene the base or knowne side, and the angle opposite: and by that height multiply halfe the base, or multiply the whole base by halfe that perpendicular height: and the product shall be the content, of that Triangle.
But if it be an Aequilater triangle: say, 1000 · 433⌊0127 ∷ the side of the triangle · Area ·
10. To find the content of a segment of a Circle, whereof the Periferia is giuen in degrees and decimall parts.
First say, As 100000, is to 1745⌊32025: so is the Arch in degrees, to the Arch in the diuisions of the Radius. keepe this number found.
Againe by the 6 Sect: 1 chap: find out the true sinus of the Arch given. Then take the difference of these two numbers found, by subducting the Sinus out of the Arch. And lastly multiply halfe that difference by the Radius 100000, the product shall be the content of that segment.
[Page 47] 11 The chord of any arch, together with the Radius, or semidiameter of the whole circle being giuen, to finde out the Arch it selfe. Say,
At the Radius giuen, is to halfe the chord (reckoned in the fourth circle) so is 100000, to the sinus of halfe the arch (to be reckoned in the first, or eighth circle). Wherfore double the arch found, and so haue you the arch of the chord proposed.
12 To finde a Quadrat, or Square equall to a superficies giuen.
First, seeke out (as hath beene taught) the content of that superficies: then take the quadrat roote thereof by Chap. 5, Sect. 4.
Of Solid measures.
13 In a Columne, or Cylinder, hauing the base, to finde how much of it maketh a foot solid.
By a Columne I meane a solid body arising from a plaine base, the angular lines whereof are parallell, and equall: and if the angular lines make right angles with the base, it is a right Columne, and the length is the height thereof: but if they make oblique angles, it is an Oblique Columne, and the length is not the height, but the height is a perpendicular line let downe from the top of the Columne vnto the base, extended if neede bee: as in the [Page 48] Diagrame, the Solid ABCDEFGH, is an Oblique Columne, because the angular line EB, standeth obliquely vpon the side of the base BA, and indeede vpon the base it selfe. Wherefore the height of it shall be equall to the line FP, let fall from the top vnto the base extended.
And after this manner also a Cylinder, and a Pyramid, and a Cone is esteemed either right, or oblique, and the height taken accordingly.
First therefore the base is to be found, of what fashion soeuer it is, as hath euen now beene shewed, either in this Chapter, or in the last before: and then diuide 1 by that same base: the quotient shall bee, the height of a Section thereof, which is equall to one foot solid.
Example. A Columne, or peece of tymber, whose sides are all parallel, hath the breadth feete 1⌊75, and the thicknesse thereof is feet 1⌊25: which multiplied together the product will be 2⌊1875. Diuide therefore 1, by 2⌊1875: and the quotient shall be 0⌊457143 almost. And so much is the height of a solid foot, of that peece of timber.
14 Hauing the Base, and the height of a Columne, or Cylinder, to finde the whole content.
Multiply the base into the height, and the product shall be the content.
Example. A Columne hath the base feet 2⌊1875, and the height thereof is feet 17⌊34, how many feet are contained in the whole?
[Page 49] Multiply the base 2⌊1875, by 17⌊34 and the product will be 36⌊086875, so many solid feet are contained in that Columne.
And in this very manner may you finde the content of a Cylinder, hauing either the diameter, or circumference giuen, together with the height.
15 To measure tapering timber, the base, or bases thereof, together with the height being giuen.
A Tapering peece of timber, according as the base thereof is right lined, or circular, is either a Pyramide or a Cone, or else a segment of one of these two: If it be a compleat Pyramide, or Cone, it hath but one base, Multiply that base by ⅓ of the height, and the product shall be the content.
But if it be the segment of a Pyramide, or Cone, First finde out the bases at both the ends, and multiply the one by the other, and out of the product thereof extract the Quadrat root: then adde together both the bases, and that quadrat root, and multiply the Aggregate thereof by ⅓ of the height, the product shall be the content.
Example. There is a tapering peece of timber, the height whereof is feet 12⌊6, and the breadth of the base at the greater end is feet 1⌊75, and the thicknes is feet 1⌊32, which multiplied together, the product will be feet 2⌊3 [...] for the greater base: the breadth of the base at the lesser end is feet 1⌊2, and the thicknesse there, is feete 0⌊91, which multiplied together, the product will be feet 1⌊052 for the lesser base. Multiply the bases together, the product will be 2⌊52252, the quadrat root whereof is 1⌊588 almost, to which if you adde the summes of both the bases, the aggregate will be 4⌊99, which being multiplied by ⅓ of the height, scil. 4⌊2, the product will be feet 20⌊958, the content of the peece of timber.
[Page 50] 16 Wherfore that vulgar manner which Carpenters vse in measuring of tapering timber, is not true: for if a peece of timber be tapering, they measure it in the very midle, and take the base, or Section there, multiplying it by the whole length. Which their manner of working, Isay, is erroneous.
For first by practise a content will be giuen, euer lesse then the true content found according to the former Sect: which way of working is infallibly true, as is Analitically demonstrated, in my Clauis mathematica, Cha. 20, Sect: 15.
And secondly Isay, that the product of that middle base, or Section, multiplied by the length, shall bee lesse then the true content, by foure Pyramides, hauing for their bases, a rectangle vnder halfe the difference of the thicknesse at the ends, and a quarter of the difference of the breadths: and are as long as halfe the peece of timber: Or which is all one, by a Parallelepipedon, vnder halfe the differences of the breadthes, and thicknesses, at both ends, and a third part of the whole length.
Which that I may shew, suppose one quarter of a tapering peece of timber giuen, sawed in [...]unner, at halfe the breadth, and halfe the thicknesse be ABCDGFEH: the midle Section is IK [...]M. Measure vpon the greater base BN, and CO, equall to AF, and BY, and NZ, equall to FE. Diuide CT, and DO to the midst, in the points X, and Q, and draw the lines PQ, NO parallel to BC, [Page 51] and YZ, SX parallel to BG. Measure also FER, equall to GS, or KL. And so the Parallelegram BPTX, shall be equall to the middle Section IKLM. Lastly, draw the lines LO, LV, LZ, and KP, KN, and MX, MY.
I say that in this one quarter of the peece of timber, A solid hauing the bases equall to IKLM, and the length AB (which is the vsuall measuring of Carpenters) is lesse then the true content, by the Pyramide DSVOL, in which DO, or SV, is halfe the difference of thicknes, and DS, or VO, one quarter of the difference of breadths in both ends: and the height of it equall to halfe the length.
For the two solides AFEHIKLM, BNZYIKLM, are apparantly equall, againe the two solide wedges GSTPKL, PTVNKL are equall, and also the two solide wedges OCXVLM, VXYZLM are equall. Now if you turne ouer the wedge GSTPKL, vnto the lesser part AFEHIKLM, it will ouer-reach in thicknesse, at the lesser end the quantity of ER, and if you also turne ouer the wedge OCXVLM, vnto the lesser part, you shall find it to fill vp the former ouer-reaching, and to make an exact Parallelepipedon, the bases or ends whereof are equall to the middle Section IKLM. but ouer and aboue those two wedges turned ouer, you shall haue left the Pyramide DSVOL, which was to be proued.
And in like manner if a round tapering solide, or peece of timber, be measured by the middle Section, or circular base, I say, That the product thereof multiplied by the length, shall be lesse then the true content, by a Cylinder, the diameter of whose base, is equall to halfe the difference of the diameters of the two bases: and the length is one third part of the whole length.
CHAP. IX. Concerning the Measuring, or Gauging of Vessells.
AWine, or Beere vessell, whether Pipe, Hogshead, Barrell, Kilderkin, or Pirkin, and such like, is in forme of a Sphaeroides, hauing the two ends equally cut off: and accordingly may be measured thus.
Measure the two diameters of the Vessell, in inches, or else in tenth parts of a foote, the one at the bung hole, the other at the head, and also the length within. And by the diameters found, finde out the circles; then adde together two third parts, of the greater circle, and one third part of the lesse: Lastly, multiply the aggregate by the length: so shall you haue the content of the Vessell, either in Cubic inches, or cubic tenth parts of a foot.
Example. Suppose a vessell, having the Diameter at the bung 32 inches, and at the head 18 inches, and the length 40 inches. The quadrat of 32 is 1024. and the quadrat of 18 is 324: Say then euermore, 1 · 0⌊ [...]236 ∷ 1024 · 536⌊166, [...]/3 the circle at the bung · 1 · 0⌊ [...]618 ∷ 324 · 84⌊823, ⅓ circle at the head. Or else by Chap. 7, Sect. 4.
The aggregate of those two circles is 620⌊989, which being multiplied by 40, the length giueth 24839⌊56 cubic inches for the whole content of that vessell.
[Page 53] 2 Mr. Edm: Gunter in his second booke of the Crosse Staffe, Chap. 4. pretending to shew the manner of gauging Wine vessels, beginneth with these words.
‘The Vessels which are heere measured, are supposed to bee Cylinders, or reduced into Cylinders by taking the meane, betweene the Diameter at the head, and the Diameter at the boungue, after the usuall manner.’
And according to this supposition, teacheth to finde a Gauge point, For a gallon of wine, in that his imagined Cylindriacall vessell.
Because his words are cautelous, and subterfugious, wee must a little examine them; for if his way bee true, my Rule before set downe, though grounded vpon demonstration, cannot stand.
Well then, that reduction of a wine Vessell into a Cylinder, is either true, or false; if it bee true what neede those ambiguities of Vessels which are here measured: and are supposed to be, &c. and after the vsuall manner? if false why is it not noted, but deliuered as a Rule to confirme an error. And what meaneth, the meane betweene the Diameter at the head, and the Diameter at the boungue? is it the meane Geometricall, or Arithmeticall, that is the meane proportionall, or that which equally differeth from both? such shifting is vnworthy an Artist.
First therefore, Let it be the meane in respect of difference, which is equall to halfe the summe of the two Diameters: I say that the Vessell cannot truely be reduced to a Cylinder by such a meane Diameter. For seeing it is most apparent that such a Vessell, is greater in the middle then at the ends, the boords, or sides thereof, shall from the middle to the ends, goe either streight, and so the Vessel shall be as it were, two equall segments of Cones, set base to base: Or else arching, and so the Vessel shall (as before I sayd, and is commonly taken for a truth) bee a Sphaeroides, hauing the two ends equally cut of.
[Page 54] If it be considered as two segments of Cones: the measure by that meane Diameter, or midle Section is quite false, as hath beene demonstrated in the former Chapter, Sect: 16, 17. and will be giuen lesse then the true content, although the sides goe straight: much more then, if the sides goe arching; for that conuexnesse, must needs yeeld a greater capacity. And therefore in neither can that manner of Gauging be true.
Againe, if the meane Diameter be vnderstood to be the meane proportionall betweene the two Diameters, it is much more false, for betweene any two numbers, the meane Geometricall is lesse then the meane Arithmeticall.
Thus much I haue thought good in this place ingenuously to signifie to the inexpert Learner, that hee might not beguile himselfe with a prejudged opinion.
3. I haue shewed the measuring of vessels by the cubic inch: but our vsuall reckoning is by the Gallon, and parts thereof. Wee must therefore doe the best we can, to inquire the true quantitie of a Gallon in inch measure, which will bee difficult to doe exactly, both because the Standards vsually are not streight sided, but a little arching, neither doe they agree perfectly one with another: but what partly by experience, both mine owne, and others, which hath come to my sight; and partly by reasoning shall seeme to me most probable, I will not refuse to set downe.
4 Our English Gallon is vnderstood to bee either in Ale measure, or Wine measure: and these two measures not a little differing. And first we will inquire about our Ale measure.
I my selfe haue measured Bushels, and P [...]cks, which haue exactly beene fitted to the Standards, and haue still in my account found a Gallon to containe better then 270 [Page 55] cubic inches, indeed much about 272, or 273 as precisely as I could measure in a vessell not truely regular. Also my worthy friend Master William Twine, who hath vndergone great paines and charge, in finding out the true content of our English measures, gaue vnto me two severall measures of an Ale-gallon, and those in due consideration but little differing. The one was found out by a brassen vessell made in manner of a Parallelepipedon, the base whereof was exactly sixe inches square, and the sides diuided into inches and twentieth parts: into which vessell he powring out a standard Gallon of Queene Elizabeth, filled with water, found it therein to ari [...]e vnto 7 inches, and 6 tenth parts: which being computed maketh cubic inches 273⌊6. The other was found by taking the dimensions of that standard Gallon, which was made in forme of a segment of a Cone, but that the sides were a little arching: the dimensions were thus; the Diameter of the top was inches 6⌊5: the Diameter of the bottome was inches 5⌊ [...]: and the height of it was inches 9⌊8: which being cast vp by Chap: 8, Sect: 15, will be found to containe cubic inches 268⌊85: differing from the former, only cubic inches 4¾: which difference might well arise through the curuitie of the sides. These measures he did not only take himselfe, but to giue me satisfaction, shewed me the experience in the said Vessell and Standard: but the truth is, I obserued the Standard, besides the arching of the sides, to bee not exactly circular within, nor the brimme of an even height, nor the bottome plaine: and in taking the height of the water in the Vessell, our sight was not able to estimate the ascent thereof so precisely, that a spoonefull of water, more or lesse, could breed any sensible difference.
What therefore shall wee doe in this difficultie? indeede looke to the first ground, and principle of our English measuring, from Barley cornes. For the length of [Page 56] 3 Barley cornes taken out of the middle of the eare is an Inch, or Ʋncia, that is a twelfth part of a foot. 3 feete make a Yard: and 16 feet and an halfe, that is 5 yards and an halfe, a Perch, with which wee measure our land; for 40 perches is a Furlong, and 8 furlongs an English mile: and againe 40 square perches is a Roodland, 4 roodland make an Acre. So then a Perch which is feet 16½, or yards 5½ is as it were the beginning of all land measure in length: and a square Perch which is feete 272¼, is as it were the beginning of all land measure in the superficiall content.
Now therefore seeing in Vessels a gallon is as it were the beginning of Ʋessell measure (for a Pottell is but a diminatiue of it, and a quart, the quarter) it is not vnlikely that our wise Ancestors had such a consideration also in solide measures, that as a square Perch (the beginning of Superficiall land measure) did containe 372 square feete and a quarter; so a Gallon (the beginning of vessell measure) should containe 272 Cubic inches and a quarter. And the rather seeing that the ancient Geographers, diuide a foote into 4 Palmes, a palme being 3 of our inches, as 3 feete are a yard. So that as the side of a square Perch consisteth of yards 5½, a Gallon also should consist, of a number of Cubic inches the square side whereof is palmes 5½.
Wherefore sauing the exact truth when it shall appeare, and in the meane time the more probable reasons of other men, I make bold to tender this my coniecture, to the censures of more diligent Inquirers, That the measure of an English Ale gallon should be a square Vessell of inch 16½, or Palmes 5½ every way, and 1 inch deepe: that is 272⌊2 [...] Cubic inches.
5. And this my opinion may peraduenture receiue some confirmation by the inquiry of an English wiue Gallon.
[Page 57] M. Henry Briggs that learned Geometrician, and my very louing friend, made an experiment, with a Cubicall vessell, which was 12 inches euery way, which hauing filled with water carefully measured, found it to containe 7 gallons and an halfe wanting a moment, as hee himselfe long since, being then of Gresham Colledge, signified to me. Now if it had contained exactly 7 gallons, and an halfe, a wine gallon should haue beene 230⌊4 cubic inches, but because it wanted a little, the gallon must be somewhat bigger, for which moment therefore if you will put 6 hundred parts of an inch, the wine gallon shall containe 231 cubic inches.
Againe M. Gunter in the place before mentioned sheweth, that the common opinion is that at London, a Cylindriacall vessell, whose diameter is 38 inches, and length 66 inches, doth containe 324 gallons: wherefore by this account a gallon should bee 231 cubic inches almost exactly, which in both so neerely agreeing, wee may well conclude, That an English wine gallon doth containe 231 cubic inches.
It is also commonly receiued, that the reason of the greatnesse of an Ale gallon aboue the Wine gallon is, that because of the frothing of the Ale or Beere, the quantity becommeth lesse, and therefore such liquors that did not so yeeld froth, as Wine, Oyle, and the like, should in reason haue a lesser measure. If then we compare these two gallons together, we shall finde that 272⌊25 · 231 ∷ 16⌊5 · 14 · which abatement might to our Ancestors, in apportioning those measures, seeme to be reasonable.
[Page 58] 6 To finde how many Cubic tenth parts of a foot are in a gallon, both of beere, and Wine: or also in any number of Cubic inches.
Because there be in a Cubic foote, 1000 Cubic tenth parts, and 1728 Cubic inches, say, 1728 (C ∶ 12) · 1000 (C ∶ 10) ∷ 272⌊25 · 157⌊ [...]521— cubic tenth parts of a Beere gallon.
And 1728 (C ∶ 12) · 1000 (C ∶ 10) ∷ 231 · 133⌊6803— cubic tenth parts in a Wine gallon.
Also 1728 · 1000 ∷ 24839⌊56 · 14374⌊746, cubic tenth parts, are in the vessell measured in Sect. 1.
7 And according to these measures so found, you may easily finde the content of a pint, or quart, or peck, or bushell, which two last are to be reckoned in Ale measure.
8 The Content of a Vessell, being giuen in cubic inches, or in cubic tenth parts of a foot, to finde how many gallons it containeth.
This is easily done if you diuide the content giuen in inches, by 272⌊ [...]5 for Ale measure: and by 231, for Wine measure. But if the content be giuen in decimall parts of a foote diuide it by 157⌊5521—for Ale measure; and by 133⌊6803—for Wine measure.
Example. How many wine gallons are in a vessell containing 24839⌊56 cubic inches, or 14374⌊746 cubic tenth parts of a foote. Diuide 24839⌊56 by 231, or diuide 14374⌊746 by 133⌊68, and the quotient shall be 107⌊ [...]3 wine gallons.
CHAP. X. Concerning the Comparison of sundry Metals, in quantity and weight.
1 IF foure pieces of Metalls, whereof the third is of the same kinde with the first, and the fourth of the same kind with the second, are proportionall, their grauities also, or weights, shall be proportionall.
2. If there bee foure pieces of metall, whereof the third is of the same kind with the first, and the fourth of the same kinde with the second: and the first and second be of equall greatnesse, and the third and fourth of equall weight; the weights of the first and second, shall be reciprocall to the magnitudes of the third and fourth.
3. Two Sphaeres of the same matter are in weight, as the cubes of their Diameters, are in magnitude. Et contra.
4. Pieces of Metall if they bee of equall magnitude, haue their weights in direct proportion, as is here set downe: but if they be of equall weight, they haue their magnitudes in proportion reciprocall: According to the experiments of Marinus Ghetaldi, in his tractate called Archimedes promotus.
Gold. | 3990 | Brasse. | 1890 |
Arg. Viu. | 2850 | Iron. | 1680 |
Lead. | 2415 | Tinne. | 1554 |
Siluer. | 2030 |
5. To finde the Weight of a Sphaere of Tinne, hauing the Diameter 1 Inch, or else [...] tenth part of a foot.
Take a piece of Tinne, and turne it exactly in a Lathe, into a Cylinder, hauing both the Diameters of its base, and also the length equall, to the Diameter of the Sphere giuen. Then weight that Cylinder, that you may haue [Page 60] the weight thereof in graines: And lastly, take two third parts of the whole number of graines: for the weight of the Sphaere.
After this manner Marinus Ghetaldi found a Cylinder of 1 inch, or twelfth part of a foot thick, and long to weigh 1824 graines: whereof [...] is 1216, the weight of a Sphaere of that thicknesse.
Againe if you say, 1000 (C ∶ 10) · 1728 (C ∶ 12) ∷ 1216 · 2101⌊248
You shall haue the weight of a Sphaere whose Diameter is one tenth part of a foot.
Wherefore also a Cubed inch of Tinne weigheth 2322⌊4—, and a Cubed tenth part of a foote weigheth 4013⌊1—
And note that Mar: Ghetaldi vseth the ancient Roman foot, which by the measure set downe in his booke seemeth to be very little lesse, then our-vsuall English foot, if not exactly the same.
Note also that he diuideth one pound, into 12 ounces, and euery ounce into 24 Scruples, and euery Scruple into 24 graines: So that an ounce with him weigheth 576 graines: and a pound 6912. Whereas our English pound of Iroy weight by Assize, or Gold smiths weight, is but 5760 graines, and our ounce 480. But whether the Raguzean graine, be the same with our English, I leaue to be tryed by the diligent Practizer.
6 To finde the Weight of a Sphaere of Tinne, at any other Diameter assigned.
Multiply the Cube of the Diameter giuen by 1216, if it be in inch measure; or by 2101⌊248, if the measure be by decimall parts of a foot: and the product will be the weight of that Sphaere.
And contrariwise to find the Diameter of a Sphaere of Tinne, by the weight giuen in graines. Diuide the weight giuen in graines by 1216 if you would haue inch [Page 61] measure: or by 2101⌊248 if you would measure by decimall parts of a foot, and the quotient shall be the Cube of the Diameter.
7. To finde the Weight of a Sphaere of any Mettall, at any Diameter giuen, either in Inch measure, or in decimall parts of a foot.
First by Sect. 6, seeke the weight of a Sphaere of Tinne, at that Diameter: then by Sect. 4, say, As the proportionall number of Tinne, is to the proportionall number of that other Metall: so is the weight of the Sphaere of Tinne now found, to the weight of the Sphaere proposed.
Example. Suppose a Sphaere of Iron, whose Diameter is 3 inches; what shall be the weight thereof?
First, the weight of a Sphaere of Tinne, of 3 inches Diameter, will be found to be 32832 graines. Then say, 1554 · 1680 ∷ 32832 · 35494⌊054 graines the weight of the Sphaere proposed.
8 To finde the Diameter of a Sphaere of any Metall in inch measure, or decimall parts of a foot, the weight thereof being giuen.
First by the contrary of Sect. 6, seeke the Cube of the Diameter of a Sphere of Tinne of that weight. Then by Sect. 4, say reciprocally. As the proportionall number of that other Metall, is to the proportionall number of Tinne: so is the Cube of the Diameter now found, to the Cube of the Diameter of the Sphaere proposed.
Example. A Sphaere of Iron weigheth 35494⌊0 [...]4 grains: how many inches is the Diameter thereof?
First, the Cube of the Diameter of a Sphere of Tinne of 35494⌊054 graines weight, will be 29⌊18910695, then say, reciprocally, 1680 · 1554 ∷ 29⌊18910691 · 27—
The Cubic root whereof is 3, the Diameter of a Sphaere of Iron of that weight proposed.
CHAP. XI. Concerning the Ordering of Soldiers, in any kinde of rectangular forme of battaile.
1 BAttailes are considered either in respect of the number of men, or in respect of the forme of ground. As asquare battaile of men is that which hath an equall number of men, both in Rank and File, though the ground on which they stand, bee longer on the File, then on the Ranke. And a square battaile of ground is that which hath the Ranke as long as the F [...]le, though the men in Ranke be more then in File.
2. In respect of the number of men, it is called either asquare battaile, or a double battaile, or a battaile of the grand front, which is quadruple, or a battaile of any proportion, of the number in Ranke, to the number in File.
3. If it bee asquare battaile of men: Extract the quadrat root out of the whole number of men, and the same shall be the number of Souldiers, to be set in a Ranke.
Example. 576 Souldiers are to bee martialled in a square battaile, that so many may be in Ranke, as in File.
Take the quadrat root of 576, which is 24: the same shall be the number to be placed in a Ranke.
4. If it be a double battaile of man: Extract the quadrat root out of halfe the number of men, and the same doubled shall bee the number of Souldiers to bee set in a Ranke.
Example. 1458 Souldiers, are to be placed in a double battaile; so that twise so many may be in Rank as in File.
[Page 63] Take halfe the given number 1458, which is 729, the quadrat root whereof is 27: double it and you shall haue 54 men to be placed in a ranke.
5. If it be a quadruple battaile, which is called of the great front: Extract the quadrat root out of one quarter of the number of men, and the same quadrupled shall be the number of Souldiers to be set in a ranke.
Example. 1024 Souldiers are to bee martialled into a battaile of the grand front, so that fower times so many be in ranke as in file.
Take one quarter of 1024 the number given, which is 256, the quadrat root whereof is 16: quadruple it, and you shall haue 64 men to be placed in a ranke.
6. If a battaile bee required of any other forme, that is, if a Ratio be given, according to which the number of men in Ranke, shall be to the number in file. Multiply the two termes of the Ratio given: Then say As the product is to the quadrat of the terme which is for the ranke, or As the terme which is for the file, is to the terme which is for the ranke: so is the whole number of Souldiers, to the quadrat of the number of men to be placed in a ranke.
Example. 1944 Souldiers, are to be martialled so, that the number of the ranke, be to the number of the file, as 8 vnto 3, that is for 8 men in ranke, 3 are to be set in file.
First multiply the two termes of the Ratio 8 and 3, the product whereof is 24, also quadrat 8, the terme of the ranke, which will be 64. Then say, 3 · 8 ∷ 1944 · 5184 · out of which extract the quadrat root 72, and it will giue you the true number of the ranke.
7. In respect of the forme of ground, the battaile is [Page 64] either a square of ground, or longer one way then the other. For the distance, or order of Souldiers martialled in array, is distinguished either into Open order, or Order.
Open order is when the very centers of their places, are distant 7 feet asunder, both in ranke and file.
Order is when the centers of their places, are distant 3 feet and a halfe in ranke, and so much in file. Or else 3 feet and a halfe in ranke, and 7 feet in file: which last order, and whatsoeuer order else there is, in which the distance of the rankes one from another is greater, then the distance of files, causeth that a square of men, maketh not a square of ground, but the ground is longer on the file then on the ranke.
8 If it be a square battaile of ground, the centers of the distances being feet 3½ in ranke, and 7 feet in file. Because 3½ is halfe of 7, the ratio of the distances, is as 1 unto 2. And seeing the number in ranke, to the number in file, is reciprocall to the distances, the ratio of the number of men in ranke, to the number of men in file, shall be as 2 unto 1. And so the Rule shall be the same with that in Sect. 6, namely, As the terme of the file, is to the terme of the ranke; so is the whole number of Souldiers, to the true number of the ranke.
Example, 1352 Souldiers, are to bee set in a square of ground, that their distances may be feet 3½ in ranke, and 7 feet in file.
The Ratio of the ranke to the file, shall reciprocally be, as 7 to 3½, that is as 2 to 1. Say therefore 1 · 2 ∷ 1352 · 2704, the quadrat roote whereof 52 is the number of men to be set in a ranke.
9 If a battaile wherein the distance in ranke is vnequall to that in file, be longer one way then the other, according [Page 65] to any Ratio giuen: there is to be considered a double ratio, one reciprocall in respect of the distances, the other according to the forme of the ground. Wherefore to finde the Ratio of men in rank, to the men in file, Multiply the two termes of the ranke, for the ranke, and the two termes of the file, for the file. And then the Rule shall bee the same with that in Sect. 6, namely, As the terme of the file, is to the terme of the ranke: so is the number of Souldiers, to the quadrat of the true number of the ranke.
Example. 10290 souldiers, are to be set in a battaile, so that they may stand onely 3 feet asunder in ranke, and 7 feet in file, and the length of the ground for the ranke, to the length of the ground for the file, shall haue the ratio of 5 vnto 2.
First in respect of the distances, the Ratio of Rank to file, reciprocally is as 7 vnto 3. Secondly, in respect of the ground, the ratio of rank, to file, is as 5 to 2. Wherefore by multiplication of like termes, the true ratio of rank to file shall be 7 × 5 to 3 × 2, that is as 35 to 6. Say therefore 6 · 35 ∷ 10290 · 60025 the quadrat root whereof is 245, the number of men to be set in ranke.
10 If 1000 Souldiers, may be lodged in a square, of 300 feete, how many feete must the side of a square be, which will serue to lodge 5000? Say, 1000 · 5000 ∷ 300 × 300 · 450000 · the quadrat roote whereof 671—is the square side sought for.
And this is the order for resolution of all other questions of this sort.
CHAP. XII. A collection of the most necessarie Astronomicall operations,
1 BEfore wee deliuer the Rules of such operations, it will not be inconuenient, to set downe certaine Reductions, wherof we may haue frequent vse.
To reduce sexagesime parts into decimals. Diuide the sexagesimes giuen by 60.
Example. How many decimals are 34′, 12″?
Here are required two reductions, first of the seconds into decimals of minutes: then of the minutes with their decimals, into decimals of degrees, Thus 60 · 1 ∷ 12″ · 0⌊2 Againe 60 · 1 ∷ 34⌊′ · 0⌊57° Wherefore 34′, 12″ are equall to 0⌊57 of a degree.
And contrariwise to reduce decimall parts of degrees in sexagesimes. Multiply the decimall part giuen by 60.
Example. How many sexagesime parts are 0⌊57°? 1 · 60 ∷ 0⌊57° · 34⌊ [...]′ Againe 1 · 60 ∷ 0⌊2 · 12″
To reduce houres into degrees. Multiply the houres with their decimall parts by 15.
[Page 67] Example. How many degrees are 8Ho, 34′, 12″; that is by the former reduction 8⌊57Ho? thus 1 · 15 ∷ 8⌊57 · 128⌊55
Wherefore Houres 8, 34′, 12″ doe containe 128⌊55 degrees.
And contrariwise to reduce degrees into houres. Diuide the degrees with their decimall parts by 15.
Example. How many houres are in degrees 128⌊55? 15 · 1 ∷ 128⌊55 · 8⌊57
2 It is to be vnderstood, that if foure numbers are proportionall, their Order may be so transposed, that each of those termes, may bee the last in proportion. In this manner,
- I. As the first is to the second; so is the third to the fourth.
- II. As the third is to the fourth; so is the first to the second.
- III. As the second is to the first; so is the fourth to the third.
- IIII. As the fourth is to the third; so is the second to the first.
Wherfore euery proportion doth implicitly containe foure Orders, two descending, and two ascending, as may be seene by their combinations: By one of which orders, if of foure proportionall numbers, any three be giuen, that other which is vnknowne, may be found out.
[Page 68] Example. To finde out any of these,
termes | 1 As the Sine of the complement of the suns declination, |
2 is to the Sine of the compl. of his altitude; | |
3 So is the Sine of the Sunnes Azumith from the meridian, | |
4 to the Sine of the horary distance from the meridian. |
If the first, second, and third termes be giuen, the fourth shall be found out by the I order.
If the first, third, and fourth termes be giuen, the second shall be found out by the II order.
If the first, second, and fourth termes bee giuen, the third shall be found out by the III order.
If the second, third, and fourth termes be giuen, the first shall be found out by the IIII order.
3. To finde out any one of these.
termes | 1 As the Radius, or totall Sine |
2 is to the Sine of the distance, or longitude of the Sunne in the Ecliptic, from the next Aequinoctial point: | |
3 So is the Sine of the Sunnes greatest declination (which is the angle of the Ecliptic with the Aequinoctial), | |
4 To the Sine of the Sunnes declination in that longitude. |
[Page 69] 4. To finde out any one of these.
termes | 1 As the Radius, |
2 is to the Sine of the Sunnes right ascension, from the next aequinoctiall point: | |
3 So is the tangent of the Sunnes greatest declination, | |
4 to the tangent of the Sunnes declination in that place. |
5. To finde out any one of these.
termes | 1 As the Radius |
2 is to the Sine of the compl. of the Sunnes greatest declination: | |
3 So is the tangent of the longitude of the Sunne from the next aequinoctiall point. | |
4 to the tangent of the Right ascension of the Sunne, from the same aequinoctial point. |
6. To finde out any one of these.
termes | 1 As the Radius |
2 is to the Sine of the compl. of the longitude of the Sunne from the next aequinoctiall point; | |
3 So is the tangent of the Sunnes greatest declination, | |
4 to the tangent of the compl. of the angle of the Ecliptic with the Meridian. |
[Page 70] 7. To finde out any one of these.
termes | 1 As the Radius, |
2 is to the Sine of the Sunnes greatest declination: | |
3 So is the Sine of the compl. of the Sunnes right ascension from the next aequinoctial point, | |
4 to the Sine of the compl. of the Angle of the Ecliptic with the Meridian. |
8. To finde out any one of these.
termes | 1 As the Sine of the compl. of the Poles height, |
2 is to the Radius; | |
3 So is the Sine of the Sunnes declination, | |
4 to the Sine of the Sunnes Amplitude ortiue, that is the arch of the horizon from the place of the Sunnes rising or setting to the true East, or West point. |
9. To find out any one of these.
termes | 1 As the Radius, |
2 is to the Sine of the Sunnes greatest amplitude ortiue, which is in the Tropick: | |
3 So is the Sine of the longitude of the Sunne from the next aequinoctial point, | |
4 to the Sine of the Sunnes amplitude ortiue. |
[Page 71] Or also of these.
termes | 1 As the Sine of the compl. of the Poles height, |
2 is to the Sine of the compl. of the Sunnes greatest declination: | |
3 So is the Sine of the Sunnes longitude from the next aequinoctial point, | |
4 to the Sine of the Sunnes amplitude ortiue. |
10. To finde out any one of these.
termes | 1 As the Radius, |
2 is to the tangent of the height of the Pole. | |
3 So is the tangent of the Sunnes declination, | |
4 to the Sine of the Sunnes Ascensional difference. |
11. To finde out any one of these.
termes | 1 As the Radius |
2 is to the Sine of the height of the Pole: | |
3 So is the tangent of the Sunnes amplitude ortiue, | |
4 to the tangent of the Sunnes ascensionall difference, |
[Page 72] 12. To finde out any one of these.
termes | 1 As the Sine of the compl. of the Sunnes declination, |
2 is to the Radius: | |
3 So is the Sine of the compl. of the Sunnes amplitude ortiue, | |
4 to the Sine of the compl. of the Sunnes ascensionall difference. |
13. To finde out any one of these.
termes | 1 As the tangent of the height of the pole, |
2 is to the Radius: | |
3 So is the tangent of the Sunnes declination, | |
4 to the Sine of the Suns horary distance from the Meridian, being due East or West. |
14. To finde out any one of these.
termes | 1 As the Sine of the height of the pole |
2 is to the Radius: | |
3 So is the Sine of the Sunnes declination, | |
4 to the Sine of the Sunnes altitude being due East, or West. |
[Page 37] 15. To find out any one of these.
termes | 1. As the Radius, |
2 is to the Sine of the height of the Pole: | |
3 So is the Sine of the Sunnes declination, | |
4 to the Sine of the Sunnes altitude aboue the Horizon at sixe of the Clocke. |
16. To find out any one of these.
termes | 1 As the Radius, |
2 is to the Sine of the complement of the Poles height. | |
3 So is the tangent of the Sunnes declination. | |
4 to the tangent of the Sunnes Azumith from the North meridian, at 6 of the Clocke. |
17 The hower of the Sunnes Rising, and setting is found out by the Ascensionall difference. For if you reduce the degrees of the Ascensionall difference, into howers, it will shew you how much the Sunne riseth, or setteth before, or after 6 a Clock.
18. The Oblique ascension also of the Sunne is found out by the Ascensionall diff [...]rence. For if you subduct the Sunnes Ascensionall difference, out of the right ascension of the Sunne, from the beginning of Aries, for the sixe Northerne signes which are ♈, ♉, ♊, ♋, ♌, ♍, or if you adde it thereto, for the sixe Southerne Signes, which are ♎, ♏, ♐, ♑, ♒, ♓, you shall have the Sunnes oblique ascension.
19. The declination of the Sunne, and his Altitude aboue the Horizon at any time, together with the height of the Pole being giuen, to find the hower of the day. Say,
[Page 74] As the Radius, is to the Sine of the complement of the Sunnes declination.
So is the Sine of the compl. of the Poles height, to a fourth number. Keepe it,
Then out of the Sunnes distance from the North pole, subduct the complement of the Pole; and of that remaines, and the complement of the Sunnes altitude, take both the Summe, and also the difference. And say againe,
As the fourth before kept, is to the Sine of halfe that summe: so is the Sine of halfe the difference, vnto a number which being multiplied by the Radius, is equall to the quadrat, of the Sine of halfe the Angle of the Sunnes horary distance from the Meridian.
20. The declination of the Sunne, and his altitude aboue the Horizon at any time together with the height of the Pole being given, to find the Sunnes Azumith. Say,
As the Radius is to the Sine of the compl. of the Suns altitude. So the Sine of the compl. of the Poles height, is to a fourth, Keepe it,
Then out of the complement of the Sunnes altitude, subduct the complement of the Pole; and of that remaines, and the distance of the Sunne from the North Pole, take both the Sunne, and also the difference: and say againe,
[Page 75] As the fourth before kept, is to the Sine of halfe the summe: So is the Sine of halfe the difference, vnto a number which being multiplied by the Radius, is equall to the quadrat of the Sine of halfe the angle of the Sunnes horizontall distance from the Meridian.
21. To find the length of the Crepusculum, or Twilight.
Betweene the light of the day, and the darkenesse of the night, the Twilight is set by the wise Creator; that wee here vpon the earth might not in an instant, passe from one extreame into another, but by successiue degrees. The Twilight is nothing else but the refraction of the Sunnes beames, in the densitie of the aire. And Pet-Nonnius to find the length of the Twilight, watched the time after Sunne set, when the twilight in the West was shut in, so that no more light appeared there, then in any other part of the sky neere the Horizon: then by one of the knowen fixed Stars, having taken the true hower of the night, found by many obseruations, that at the time of shutting in the Twilight, the Sunne was vnder the Horizon 18 degrees, and vntill the Sunne was gone so low, the Twilight continued. Say therefore
As the Radius is to the Sine of the compl. of the Sunnes declination:
So the Sine of the compl. of the heigth of the Pole, is to a fourth, Keepe it.
Then out of the Sunnes distance from the South Pole, subduct the complement of the Pole; and of that remaines, [Page 76] and degrees 62, take both the Summe and also the difference; and say againe,
As the fourth kept, is to the Sine of halfe the summe: so is the Sine of halfe the difference, to a number which being multiplied by the Radius is equall to the quadrat of the Sine of halfe the angle of the Sunnes distance at the ending of the Twilight, from the high Noone next to it.
Wherefore if out of the whole angle conuerted into howers, you subduct halfe the diurnall arch, or the hower of the Sunnes setting, you shall haue the true length of the Crepusculum, or Twilight.
22. To find the length of the least Crepusculum in the yeare.
The Sunne being in the winter Tropic maketh the longest Crepusculum, of the whole winter halfe yeare, and from thence, as the dayes increase, the Crepuscula doe decrease vntill they come to bee shortest, which is in a certaine Parallel, betweene that Tropic, and the Aequinoctiall: the declination whereof is thus found out.
As the tangent of the complement of the Pole, is to the Sine thereof: So is the tangent of 9 degrees, to the Sine of the declination of the Parallell, in which the Sunne maketh the shortest Crepusculum of the whole yeare.
[Page 77] 23 But before the Crepusculum come to bee shortest, there is another Parallel, in which the Crepusculum is equall to that in the Aequinoctiall: the declination wherof is thus found out.
As the Radius is to the Sine of the altitude of the Pole: So is the Sine of 18 degrees to the Sine of declination of the Parallel in which the Sunne maketh the Twilight equall to that in the Aequinoctiall.
24. If an Arch of the Ecliptic, be equall to his Right ascension, one end thereof beeing knowne, to find out the other end. Say,
As the Sine of the Compl. of the declination of the arch giuen. is to the Radius: so is the Sine of the compl. of the greatest declination, to the Sine of the compl. of the other and.
25. To find the poynt of one quadrant of the Ecliptic, wherein the difference of longitudes cease to be greater, then the differences of the right ascensions.
Multiply the Sine of the complement of the greatest declination, by the Radius, and out of the product extract the quadrat root: the same shall bee the Sine of the complement of the declination sought for.
[Page 78] 26. To find the quantitie of the angles, which the circles of the 12 Howses make with the Meridian. Say
As the Radius is to the Tang. of 60 degr. for the 11th, 9th, 5th, and third howers, or to the Tang. of 30 deg. for the 12th, 8th, 6th, and second howses; so is the Sine of the complement of the Pole, to the tang. of the compl. of any howse with the Meridian.
And note that on the Easterne part of the vpper hemisphaere, there are three circles of Howses, the Horoscope, which is also the Horizon, and next to that is the circle of the 12th Howse, then the circle of the 11th Howse. On the Westerne part also, are three circles of Howses, the circle of the 7th Howse, which also is the Horizon, and next thereto the circle of the 8th Howse, then the circle of the 9th Howse. But the circle of the 10th Howse, is the very vpper Meridian it selfe. Contrary Howses are 1 and 7, 2, and 8: 3 and 9: 4 and 10: 5 and 11: 6 and 12.
27. Resolue the whole time from the Noone last past into degrees (by multiplying the howers with their decimall parts by 15, according to Sect: 1) which adde vnto the right Ascension of the Sunne: and you shall haue the right ascension of the point of the Aequator in the vpper Meridian, which is called the Right ascension of Medium coeli.
28. Adde 99 degrees to the Right ascension of Med. Caeli: and it shall be the degree of the Aequator then rising vpon the East Horizon.
[Page 79] 29. If the first quadrant of the Aequator doe arise, the beginning of γ is distant from the meridian Eastward, so much as is the distance of the Right ascension of Med. coeli, from 360. But if the second qua [...]rant of the Aequator doe arise, the beginning of γ, is distant from the Meridian Westward, so much as is the distance of ☉, from the Right ascension of Med. coeli.
And in both of them the lower angles of the Ecliptick with the Meridian, on the East side is obtuse, and on the West side acute: and the 90th degree of the Ecliptick, commonly called non agesimus gradus, is on the East part.
30. If the third quadrant of the Aequator doe arise, the beginning of ♎ is distant from the Meridian Eastward, so much as is the distance of the Right ascension of Med. coeli from 180. But if the fourth quadrant of the Aequator doe arise, the beginning of ♎, is distant from the Meridian Westward, so much as is the distance of 180, from the Right ascension of Med. coeli.
And in both of them the lower angle of the Ecliptick with the Meridian, on the East side is acute, and on the West side obtuse: and on the 90th degree is on the West part.
31. The point of the Ecliptick culminant in the Meridian, which is called Medium coeli, or Cor coeli, and is the cuspis of the 10th house, may be found by Sect. 5.
32. The declination of the said culminant point, may be found by Sect. 3. VVherefore also by adding or subducting that declination, to, or from the eleuation of the [Page 80] Aequator, (which is the complement of the Pole) the Altitude of Med. coeli may be had.
33. The Angle of the Ecliptick with the Maridian, may be found by Sect. 7.
34. To finde the Altitude of the 90 degr. Or the Angle of the Ecliptick with the horizon.
As the Radius is to the Sine of the compl. of the altitude of Med: coeli. So is the Sine of the angle of the Ecliptick with the Meridian, to the Sine of the compl. of the angle sought for.
35. To finde the Azumith of 90 degr. which is also the Amplitude ortiue of the Ascendent, or Horoscopus.
As the Radius, is to the Sine of the Altitude of Med. coeli. So is the tang. of the Angle of the Ecliptick with the Meridian, to the tang. of the compl. of the distance of that Azumith from the Meridian.
36. To finde the Horoscopus, or Ascendent degree of the Ecliptick, Or the Cuspis of the first house.
The Distance of the Azumith of 90 degrees from the Meridian, is equall to the Amplitude ortiue of the Ascendent degree. Wherefore the Ascendent degree [Page 80] or the Ecliptic, may thence bee found, by Sect: 8, or 9. Or else thus.
As the Radius is to the Sine of the complement of the angle of the Ecliptic with the Meridian: So is the tang. of the complement of the altitude of Med. Coeli, to the tangent of the distance of Med. coeli from the Ascendent degree.
37. To find the parts of the angle of the Ecliptic with the Meridian, cut with an arch perpendicular to the Circle of any of the Howses. Say
As the Radius is to the Sine of the compl. of the altitude of Med. coeli: so is the tangent of the circle of any Howse with the Meridian, to the tang: of the compl: of the part of that angle, which is next the Meridian
Then subduct that part found out of the whole Angle for the remaining or latter part.
38. To find the Distance of the cuspis of any howse, from Med: coeli. Say
As the Sine of the compl. of the later part of the angle of the Ecliptic with the Meridian, is to the Sine of the compl: of the former part of that angle: So is the tang▪ of the altitude of Med: coeli, to the tang: of the distance of the cuspis of that Howse sought for.
[Page 82] 39. To find the Altitude of the Pole aboue any of the circles of the Howses.
First find out the Angle which the circle of the Howse proposed maketh with the Meridian, by Sect: 23: And then say.
As the Radius is to the Sine of the angle of the circle of the Howse with the Meridian: So is the Sine of the height of the Pole aboue the Horizon of the place, to the Sine of the height of the Pole aboue that circle of position.
40. The longitude, and latitude of any fixed Starre being given, to find out the Right ascension, and Declination thereof.
The angle which the Circle of the Sunnes longitude maketh with the Meridian, at the Pole of the Ecliptic, I call the Angle of longitude.
And the angle which the Circle of the Sunnes Right ascension, maketh with the Meridian at the Pole of the world, I call the Angle of right Ascension. The condition and quantitie of which two angles, is thus found out.
In Starres of the Northerne latitude
If the longitude be in the I quadrant of the Ecliptic: subduct it out of 90: the remaines will bee the angle of longitude, acute. And the Angle of Right ascension, being found, must be added vnto 270.
If the longitude bee in the II quadrant: subduct 90 out of it: the remaines will bee the angle of longitude, acute. And the Angle of right ascension being found must be taken out of 270.
If the longitude bee in the III quadrant: subduct 90 out of it, the remaines will be the angle of longitude, obtuse. And the Angle of right ascension being found, must be taken out of 270.
If the longitude bee in the IIII quadrant, subduct it out of 90+360: the remaines will bee the angle of longitude, obtuse. And the Angle of right ascension being found, must be added vnto 270.
In Starres of the Southerne latitude
If the longitude be in the I quadrant, subduct 270 out of it + 360: the remaines will be the angle of longitude, obtuse. And the Angle of right ascension being found, must be taken out of 90.
If the longitude bee in the II Quadrant, subduct it out of 270: the remaines will bee the angle of longitude, obtuse. And the Angle of right ascension being found, must bee added to 90.
[Page 84] If the longitude be in the III quadrant: subduct it out of 270; the remaines will be the angle of longitude, acute. And the Angle of right ascension being found, must bee added to 90.
If the longitude be in the IIII quadrant: Subduct 270 out of it: the remaines wil be the angle of longitude, acute. And the Angle of right ascension being found, must bee subducted out of 90× 360.
Then say,
As the Radius, or totall Sine, is to the Sine of the complement, or excesse of the angle of longitude:
So is the tang. of the compl. of the latitude, to the tang. of the first base.
If the angle of longitude bee obtuse; vnto the first base found, adde the greatest declination deg. 23½: and the summe shall be the second base; and the angle of right ascension shall be acute.
But if the angle of longitude be acute; out of the first base subduct the greatest declination: and the remaines shall be the second base. And the angle of right ascension shall be obtuse.
Or else out of the greatest declination of the Sun, subduct the first base; and the remaines shall be the second base: and the angle of right ascension shall be acute.
Say againe,
As the Sine of the second base, is to the Sine of the first base:
So is the tang. of the angle of longitude, to the tang. of the angle of right asce [...]sion.
[Page 85] VVhence by adding or subducting as was before deliuered in the conditions of those angles, shall be giuen the Right ascension of that Starre sought for.
Lastly say
As the tang. of the second base, is to the Radius:
So is the Sine of the compl. or excesse of the angle of right ascension to the tang. of Declination.
VVhere note that if the second base exceede 90 degr: the declination found, shall not be of the same kinde, that the latitude is, but in the contrary Hemisphaere.
Names of Starres | Right Ascension | Declination | mag. | |||
The Polar Starre | 7° | 4′7 | 80° | 2′7 | N | 2 |
Andromedaes girdle | 12 | 32 | 33 | 48 | N | 2 |
the former horne of ♈ | 23 | 38 | 17 | 37 | N | 4 |
the bright starre in the head of ♈ | 26 | 56 | 21 | 48 | N | 3 |
the iawe of the Whale | 41 | 03 | 2 | 42 | N | 2 |
Medusaes head | 41 | 27 | 39 | 35 | N | 3 |
the eye of the Bull | 64 | 00 | 15 | 46 | N | 1 |
the Goat starre | 72 | 44 | 45 | 35 | N | 1 |
the former shoulder of Orion | 76 | 38 | 4 | 59 | N | 2 |
the latter shoulder of Orion | 84 | 07 | 7 | 18 | N | 2 |
the great dogge starre | 97 | 27 | 16 | 13 | S | 1 |
the higher head of ♊ | 108 | 01 | 32 | 35 | N | 2 |
the lesser Dogge starre | 110 | 17 | 6 | 06 | N | 2 |
the lower head of ♊ | 111 | 00 | 28 | 49 | N | 2 |
the Cribb, or Manger | 125 | 4 | 20 | 52 | N | Neb. |
the heart of Hydra | 137 | 39 | 7 | 10 | S | 2 |
the heart of the Lion | 147 | 27 | 13 | 39 | N | 1 |
In the loynes of the Lion | 163 | 54 | 22 | 26 | N | 2 |
In the tayle of the Lion | 172 | 49 | 16 | 32 | N | 1 |
In the girdle of Virgo | 189 | 32 | 5 | 20 | N | 3 |
Names of Starres | R. Ascen. | Declination | mag. | |||
Aliot | 189° | 36 | 57 | 53 | N | 2 |
Vindemiatrix | 191 | 15 | 15 | 51 | N | 3 |
Spica Virginis | 196 | 44 | 9 | 17 | S | 1 |
Arcturus | 209 | 56 | 21 | 34 | N | 1 |
the Southerne ballance | 217 | 56 | 14 | 32 | S | 2 |
the Northerne ballance | 224 | 31 | 8 | 2 | S | 2 |
the bright star in the serpents neck | 231 | 49 | 7 | 35 | N | 3 |
the heart of Scorpius | 242 | 4 | 25 | 34 | S | 1 |
the head of Hercules | 254 | 40 | 14 | 51 | N | 3 |
the head of Ophiucus | 259 | 41 | 12 | 52 | N | 3 |
bright starre in the Harp | 276 | 17 | 38 | 30 | N | 1 |
bright starre in the Vultur | 293 | 27 | 8 | 1 | N | 2 |
vpper horne of ♑ | 299 | 30 | 13 | 32 | S | 3 |
the left hand of ♒ | 307 | 10 | 10 | 43 | S | 4 |
the left shoulder of ♒ | 318 | 18 | 7 | 2 | S | 3 |
the mouth of Pegasus | 321 | 49 | 8 | 18 | N | 3 |
the right shoulder of ♒ | 326 | 59 | 1 | 58 | S | 3 |
Fomahant | 339 | 29 | 31 | 23 | S | 1 |
In the vpper wing of Pegasus | 341 | 53 | 13 | 21 | N | 2 |
In the tip of the wing of Pegasus | 358 | 52 | 13 | 15 | N | 2 |
[Page 88] 41. The longitude, and latitude of any two Starres being giuen, to finde their distances.
If the Starres haue both the same longitude, differing onely in latitude; the difference of latitude, is the distance of the starres.
And if they differ onely in longitude hauing the same latitude; Say
As the Radius, is to the Sine of halfe the difference of longitude:
So is the Sine of the compl. of the latitude giuen, to the Sine of halfe the distance of the Starres.
But if they differ both in longitude, and latitude, whether the latitudes be both of the same kinde, or one Northerne, and the other Southerne. Take the difference of both the starres, from the pole of the Ecliptick, toward which the starre hauing the greater latitude is. And say,
As the tang. of the compl. of the lesser distance from the pole, is to the Radius:
So is the Sine of the compl. or excesse of the difference of longitudes, to the tang. of the first base.
Take this first base out of the greater distance from the pole, and the remaines shal be the second base, Then say,
As the Sine of the compl. of the first base, is to the Sine of the compl. of the second base:
So is the Sine of the compl. of the lesser distance from the pole, to the Sine of the compl. of the distance of the two Starres.
[Page 89] If any man will take paines to calculate (by this last Rule) the distances of some noted starrs of the first, second, and third magnitudes, round about the heauens, which are not aboue 5, or 6 degrees, at the most, one from the other: and shall keepe them written in his booke: they may serue as a Rule, or Instrument, whereby he may reasonably estimate with his eye, the distance of any Planet, or Comet, or other apparition from a knowen fixed starre, not very farre remote: by comparing the distance which hee would know with some of those knowen distances which he shall find, either to be equall, or else to haue some proportion thereto.
42. The longitude, and latitude of any two Cities being giuen, to find their distance.
The manner of the operation is the very same with the former, vnto which therefore I referre the Reader: onely will note, that in the heauens, the longitude and latitude is taken in respect of the Ecliptic, which being the way of the Sunne, all the starrs in their proper motion, haue reference vnto it, as vnto their measure and rule. But in the Earth the principall Circle is the Equinoctiall, diuiding it into the Northerne, and Southerne he misphaeres. And therefore in the earth, the longitude, and latitude is reckoned by the Aequinoctiall.
The distance of two places vpon the Earth, being found in degrees, may bee conuerted into English miles, by taking 60 miles for euery degree, and one mile for every minute.
43. To find at what hower a fixed starre commeth into the Meridian any day.
Seeke the Right ascension of the Sunne, for that day, by Sect [...]; and subduct it out of the Right ascension [Page 90] of the Starre. And reduct the degrees remaining into howers, by Sect: 1. The same shall shew how long time from the Noone before, the same starre shall come into the Meridian.
Wherefore if at any time of the night, a Starr whose Right ascension is knowne, be in the Meridian, the hower of the night is easily found.
44. The height of any knowne Starre aboue the Horizon, being by any means given, to find the hower of the night.
First seeke out the hower of that starrs comming into the Meridian the same day, by Sect. 43. Againe seeke out the horary distance of that starr from the Meridian, according to Sect: 19. And then if the starr bee on the East side, not yet come to the Meridian, take the difference of those two numbers; but if the starre bee past the Meridian, take the Summe of them, for the houre of the night.
45. The height of the Pole being given to find the comming of any fixed Starre, in the due East, or West. Say
As the Radius is to the tang: of the starres declination: So is the tang: of the compl: of the Pole, to the Sine of the compl. of the Starres horary distance from the Meridian.
46. The height of the Pole being giuen, to find the Altitude of any fixed starr aboue the Horizon, being due East or West. Say,
[Page 91] As the Sine of the height of the Pole, is to the Radius: so is the Sine of the Starrs declination, to the Sine of the Altitude, at due East or West.
47. By the Altitudes of any two knowne fixed starrs taken when they are both in the same Azumith, to find the height of the Pole.
First say,
As the Sine of the difference of the starrs altitudes, is to the Sine of the difference of their Right ascensions: so is the sine of the neerer starrs distance from the apparent Pole, to the Sine of an angle to be kept.
Againe compare the furthest starrs distance from the Pole with the distance from the Zenith, and say
As the Radius is to the Sine of the compl. of the Angle kept: so is the tang: of the lesser of the compared arches, to the tang: of the first base.
Subduct the first base out of the greater of the two compared arches; and the remaines shall bee the second base.
Then lastly say,
As the Sine of the complement of the first base, is to the Sine of the compl. of the second base: so is the Sine of the compl. of the lesser of the two compared arches, to the Sine of the height of the Pole.
[Page 92] 48. To find out the horizontall Parallax of the Moone.
First the distance of the Moone from the Center of the earth must be knowne in Semidiameters of the earth: which vnto them that are acquainted with the Theorie of the Planets, is not very difficult. And whereof peraduenture, I may hereafter teach the practise, by most easie and exact instruments, which I haue long since framed.
Say,
As the distance of the Moone, from the center of the earth, is to the Semidiameter of the earth: So is the Radius, to the Sine of the Moones horizontall parallax in that distance.
49. The horizontall Parallax of the Moone being given, to find her Parallax in any apparent altitude.
As the Radius, is to the Sine of the altitude of the Moone: so is the Sine of the horizontall Parallax, to the Sine of the Parallax in that altitude.
50. The place of the Moone in the Ecliptic hauing little or no latitude (as in the Eclips of the Sunne) together with her Parallax of altitude being giuen, to find the Parallaxes of her longitude, and latitude.
If the Moone bee in the 90th degree of the Ecliptic: shee hath no Parallax of longitude, and the Parallax of latitude, is the very Parallax in that altitude.
[Page 93] But if the Moone be not in the 90th deg. say,
As the Radius is to the tang. of the angle of the Ecliptick with the horizon: So is the Sine of the compl. of the distance of the Moone, from the Ascendent, or descendent degree of the Ecliptick, to the tang. of the compl. of the angle of the Ecliptick with the Azumith of the Moone.
Againe say,
As the Radius is to the Sine of that angle: So is the Parallax of the Moones altitude, to the Parallax of her latitude.
Lastly say,
As the Radius is to the Sine of the compl. of that former angle: So is the Parallax of the Moones altitude, to the Parallax of her longitude. which is to bee added to the true motion of the Moone, if she be on the East part of the 90th degree of the Ecliptick: or to be subducted out of it, if she be on the West part.
Many other Astronomicall and Geographicall problemes might be added. But because it is impossible to set downe all, which may be of vse, at some time or other: I haue in the next Chapter deliuered briefly the doctrine of triangles fitted vnto practise: with all the seuerall cases belonging thereto.
CHAP. XIII. Of Trigonometria, or the manner of calculating both Plaine, and Sphaericall triangles. And first concerning certaine generall notions, and rules necessary thereto.
IN euery triangle both Plaine, and Sphaerical, the greater side subtendeth the greater angle. And the greater angle hath the greater side opposite vnto it. Also the greater angle lyeth to the lesser side, and the greater side hath the lesser angle lying vnto it.
In euery plaine triangle, any two angles being giuen, the third is also giuen: and one of the angles being giuen, the summe of both the other two is giuen. For all the three angles together, are equall to two right angles, that is to 180 degrees.
In a plaine rectangle triangle, one of the acure angles is the complement of the other. Where note that when the complement is named without any other addition, it is meant of the arch, which is wanting of a quadrant of that circle, or 90 degrees. In like manner the excesse is meant of the arch, which is aboue a quadrant. But when it is said the complement to a semicircle, it is vnderstood of so many degrees as will make vp 180.
But in a Sphaericall rectangle triangle, one of the oblique angles is alwayes greater then the compl: of the other.
If two arches together make vp a Semicircle, the excesse of the greater arch, is equall to the complement of the lesser.
[Page 95] The same Right Sine, and the same Tangent, and Secant, doth belong both to the arch it selfe, and also to the complement of it to a Semicircle. But their versed Sines differ: For the versed Sine of an arch lesse then a quadrant, is equall to the difference of the Radius, and the Sine of the complement of that arch: and the versed Sine of an arch greater then a quadrant, is equall to the summe of them. And the versed Sine is thus found out, As the Radius is to the Sine of halfe the arch; so is the Sine of that halfe arch, to halfe the versed Sine of the whole arch.
In a right angled triangle both Plaine, and Sphaericall, one of the sides containing the right angles, is called the Base, and the other the Cathetus: and the fide subtending the right angle is the Hypotenusa. And know that euery rectangled triangle, is most fitly noted with the letters ABC; so that BA may be the Base, and CA the Cathetus, and BC the Hypotenusa: and B the angle at the base, and C the angle at the Cathetus, and A the right angle. Likewise euery oblique-angled triangle with the letters BCD; so that out of the angle C a perpendicular CA, being let downe, it may in the base BD distinguish the two cases BA and DA, which are the bases of the two particular triangles into which it is cut. And in noting the triangles with letters, obserue diligently, that if any angle be giuen together with one of the sides including it, the same angle be noted with B; and the side with BC.
If both the angles at the Base BD be acute, the perpendicular CA shal fall within the triangle: And BD = BA + DA that is BD is equall to the summe of BA and DA. And if the angle B be obtuse, the perpendicular CA shall fall without the triangle, beyond the obtuse angle B: And BD = DA − BA, that is BD is equall to the excesse of DA aboue BA or if the angle B. be obtuse, the perpendicular CA: shall fall without the triangle beyond the obtuse [Page 96] angle D: And BD = BA − DA, that is BD is equall to the excesse of BA aboue DA. The lesser case being still taken from the greater angle.
And note that this signe +, or pl (that is plus) sheweth that the magnitude before which it is set, is affirmed and positiue in nature; and therefore to bee added. And that this signe—or mi (that is minus) sheweth the magnitude before which it is placed, is denied, and priuatiue in nature; and therefore to be substracted, as you may see in those former examples.
Againe, some magnitudes are taken seuerally and apart; as s BA, that is the Sine of the Base; s co BC, that is the Sine of the complement of the Hypotenusa; t B, that is the tangent of the angle ABC at the base; t co C, or t co ABC, the tangent of the complement of the angle at the Cathetus: So also VqZ, that is the quadrat side of the plaine Z. And some magnitudes are taken vniuersally, and then they are included in pricks: as [...]: that is the Sine of halfe the arch, which is composed of the summe of the two arches DC, and BD, abating thereout the arch BC. So also Vq ∶ Z × X ∶ that is the quadrat side of the two plaines Z and X put together: also Vq ∶ Q in R ∶ Or Vq ∶ Q × R ∶ that is the quadrat side of a rectangular plaine, the two sides whereof are the lines Q and R, or some fourth proportionall already found, and the Radius, or Semidiameter, which is the totall Sine. For by the signe in, or ×, I vse to expresse multiplication.
When any triangle is giuen to be resolued by Trigonometrie, note the parts thereof (either-sides or angles) which are giuen and knowne, with a little line drawne crosse each such part: and note the vnknowne part which is sought for with a little circle.
[Page 97] And if a triangle Sphaericall (bee it right angled or oblique-angled) proposed hath two sides each of them seuerally greater then a quadrant: you shall in resoluing thereof, keepe the least side with the least angle opposed to it: and for the two other both sides, and angles, take the complements of them to a semicircle.
Lastly, if a triangle with all the three angles giuen, be required to be conuerted into a triangle hauing the three sides giuen. You shall for the greatest angle of the triangle proposed, & for the greatest side subtending it, take the complements to a semicircle; keeping the other two lesser angles, with their subtendent sides as they are.
THE CALCVLATION OF PLAINE right-angled-triangles.
BC · BA ∷ R · [...] B ( [...]C) ·
BA · CA ∷ R · [...]B ( [...] [...] C) ∶ Of plaine Oblique-angled triangles.
[...]B · DC ∷ [...]D · BC ∷ [...]C · BD · and here it is necessary to be knowne, whether the angle sought for be greater, or less then a right angle, or 90 deg.
First seek the angle D, by the III; then both the angles Band D being subducted out of 180, you shall haue 180 − B − D = C ·
First seeke the angle D, by the III; then both the angles B and D being subducted out of 180, Say [...]B · DC ∷ s ∶ 180 − B − D · BD ·
Let the side BD be greater then the side BC: First, [...] then for the other two angles: [...]—the greater [...]—the lesser.
Let the side BD be greater then the side BC:
First, the angles C and D are to be sought, by the VI. and the side DC, by the III.
Take the greatest side BD for the base: and let the side BC, be greater then the side DC. First say, BD · BC + DC ∷ BC − DC · Q (viz BD − 2DA) · then [...]
Nextly seeke the angles B and D, by the III. Lastly 180 − B − D = C.
THE CALCVLATION OF Sphaericall right-angled, and quadrantall triangles.
R · [...]B ∷ sBC · sCA ·
R · sB ∷ [...] [...]BA ∶ s [...]CA ·
R · [...] [...]BA ∷ [...] [...]CA ∶ [...] [...]BC ∶
R · sBA ∷ tB · tBA ·
R · t coB ∷ tCA · sBA ·
R · sBA ∷ t coCA · t coB ·
R · s coB ∷ tBC · tBA ·
R · t coBC ∷ tBA · [...] coB ·
R · [...] coB ∷ t coBA · t coBC ·
R · [...] coBC ∷ [...]B · [...] [...]C ·
If a triangle BCD be quadrantall, hauing one side BC equall to a quadrant; vpon the pole D describe an arch of a great circle CA, cutting the side DB extended in A: and so making a right-angled triangle ABC without the other. This outward right-angled triangle shall be resolued in steed of the quadrantall proposed.
Of Sphaericall Oblique-angled triangles.
sB ∶ [...]DC ∷ [...]D · sBC ∷ [...]C · sBD · and in these it is necessary to bee knowne whether the terme sought for be greater then a quadrant, or not. The same also is to be knowne in the tenne rules next following, if the sides BC and DC are both giuen.
First, R · s coB ∷ tBC · [...]BA · then, s coBA · s coDA ∷ [...] coBC · s coDC ·
First, R · s coB ∷ tBC · tBA · then [...]DA · sBA ∷ [...]B tD ·
First, R · s coB ∷ [...]BC · [...]BA then, s coBC · [...] [...] DC ∷ [...] [...]BA · s [...]DA ·
First, R · s coB ∷ tBC · tBA · then, tD · tB ∷ [...]BA · sDA ·
First, R · [...] coBC ∷ [...]B · t coBCA · then, s coDCA · s coBCA ∷ tBC · tDC ·
First, R · s coBC ∷ tB · t coBCA · then, sBCA · sDCA ∷ s coB · s coD ·
First, R · s coBC ∷ tB · t coBCA · then, tDC · tBC ∷ s coBCA · s coDCA ·
First, R · s coBC ∷ tB · t coBCA · then, s coB · s coD ∷ [...]BCA · sDCA ·
First, R · sBD ∷ sBC · QI · then, [...]
See what QII cutteth in the fift circle, which is of equall diuisions: and thereto adde the Radius, by setting [Page 107] I before that number. Diuide the whole into two equall parts: and reckoning one halfe in that fift circle, set the Index to it, and it shall in the first circle cut the Sine of halfe the angle B.
If all the three angles be giuen: conuent the triangle into another hauing all the three sides giuen: and resolue the same for the triangle proposed.
CHAP. XIIII. Of the Nocturnall Dials.
THere are in the Instrument, two seuerall Nocturnall Dyals. The innermost of them is fitted to the starre in the rump of the great Beare, commonly called Aliot. The other is composed of 12 seuerall starres: whose names you shall finde written within, neere to the center.
The outermost circle of the Nocturnall Dyall is diuided into twise 12 houres: each houre being subdiuided into quarters, and are noted with figures belonging to the houres, as may be seene in the Instrument.
The middlemost circle of the Nocturnall is diuided into 12 moneths, hauing their names written: each moneth being distinguished into tenth dayes with longer lines; and into fift dayes with shorter lines. And if the Instrument be large enough, each day of the monethes throughout the yeare, may be noted with pricks.
In the innermost circle are the diuisions and names of 12 fixed starres: which are these.
- The bright star in the head of ♈.
- the Bulls eye
- the latter shoulder of Orion
- the little dogge
- the heart of the Lyon
- the tayle of the Lyon
- Spica Virginis
- the North ballance
- the head of Ophiuchus
- the heart of the Vultur
- the mouth of Pegasus
- the tip of the wing of Pegasus.
To finde out the houre of the night by Aliot.
Seeke the day of the moneth in the annuall circle of the Nocturnall: and apply the Index thereto: marke what houre it cutteth, in the houre circle. Remember this [Page 109] houre for all that day: then at night when you would finde out the houre, hold vp your Instrument by the handle, and moue it vp and downe, till you see the pole starre through the middle hole, and the starre called Aliot by the limbe: Set the Index or labell to Aliot, and marke what houre the labell cutteth, for if vnto this houre you adde the houre kept in minde for that day, the summe of both shall giue you the true houre of the night: so that you cast out 12 houres, from the said summe if it shall chance to be more.
Example. If on the 15th of Nouember you would find the houre of the night by the starre Aliot. Apply the Index to the day of the moneth, and it will cut in the houre circle 8 and an halfe: then suppose the Index being set to the starre Aliot, as aboue taught, doth cut in the houre circle 10. these two numbers being added together, the summe wil be 18½, out of which subduct 12; and the remaines 6½, will be the true houre of the night.
To finde out the houre of the night by the Inner Nocturnall Dyall.
To performe this it is necessary that you know the true Meridian of the place wherein you are, and can finde it out by night, which you may thus doe. Hauing a Meridian line drawne in some window, or other conuenient place (as is shewed in the Second part of this booke, Vse 19) stick vp therein a long needle perpendicularly, and watch till the Sunne casteth the shadow of the needle, vpon the Meridian line. Or else in a true Sunne Dyall obserue when the shadow falls iust on 12 a clock, for then is the Sunne in the Meridian. Wherefore goe instantly into some place about your house where you may see some marke, either a chimney, or the corner of an house, or else some tree, or such like, directly betweene you and the Sunne: then haue you the true Meridian.
[Page 110] Or otherwise you may in a cleare night goe into some plaine place neere your house, and setting vp a straight pole perpendicularly on the ground, goe a good distance from it Southwards; and then moue vp and downe, till you see the top of your pole, directly betweene your eye, and the North polar starre: then set vp another pole perpendicularly betweene your feet, so that both your poles, and the Polar starre, may be in one right line. And then going backe againe to your first pole, looke what knowne starre is directly ouer your last pole, for that starre is in the Meridian. You may therefore instantly goe to some conuenient place, and take a marke whereby you may at all times know the Meridian as is afore taught.
When therefore at any time of the night you would know what a clocke it is, goe to that place where you stood, and looking directly ouer your marke, see if any of the 12 fixed starres, bee in the Meridian; or if none of them be therein, obserue which two of them are on either side thereof, and what part of that space is in the Meridian. Then goe into the light, and take your instrument, and set the Index to that starre, or point which you saw in the Meridian: marke what houre it cutteth, for that same houre being added to the houre, which the day of the moneth sheweth, shall giue you the true houre of the night: so that you cast out 12 houres, from the said summe, if it shall chance to be more.
Example. Suppose the fifth of December, that the middle point of the space betweene the bright starre in the head of Aries, and the Bulls eye, bee in the Meridian. Set the Index to the middle point of the space betweene those two starres in the Instrument: and it will cut in the houre circle 2 and an halfe: then againe set the Index to the fifth of December, and in the houre circle it wil cut 7: [Page 111] which added vnto 2 and an halfe, giueth 9 and an halfe, for the true houre of the night.
Another example. Suppose the 19th of December, that one third part of the space betweene the Bulls eye, and the right shoulder of Orion, be in the Meridian. Set the Index to one third part of that space in the Instrument, and it will cut in the houre circle 4 and halfe a quarter almost: againe, set the Index to the 19th of December, and in the houre circle it will cut 6, which being added vnto 4, and halfe a quarter almost, giueth 10 and almost halfe a quarter for the houre of the night.
THE SECOND PART OF THIS BOOKE.
Shewing the vse of the Second side of the Instrument, for the working of most questions, which may be performed by the Globe: And the declination of Dyals, vpon any kinde of Plaine.
VPon the second side of the Instrument, is delineated the proiection of the vpper Hemisphaere vpon the plaine of the Horizon: The Horizon it selfe is vnderstood to bee the innermost circle of the limbe: and is diuided on both sides, from the points of East, and West into degrees, noted with 10, 20, 30, &c. vnto 90. And the center of the Instrument is the Zenith, or Ʋertical point.
Within the Horizon, the middle straight line, or Diameter pointing North and South, is the Meridian, or 12 a clock line: and the other shortarching lines, on both sides of it are the houre lines, distinguished accordingly by their [Page 114] figures. These houre lines should indeede bee drawne through the whole plaine, crossing one another in the Pole of the world: but that the Instrument may be more faire, they are onely drawne short.
And because diuers excellent vses, doe require the totall delineation of the houre circles, I haue in a seuerall paper, inscribed intirely, both the houre lines, and also two other circles betweene them, containing euery one fiue degrees. (But if the Instrument were large enough to receiue them, it were best if euery degree had his circle: and so euery 15 circle should bee an houre line.) And of the parallels, there needes no more, but the Aequinoctial, and both the Tropics.
For as much as there will be great vse of this paper Instrument; I haue in the 24 Vse shewed the manner of making it: so that any that 1 [...] ingenuous, and ready handed may himselfe delineate one sufficient enough to serue his turne, for any eleuation.
The two arches which crosse the houre lines meeting on both sides in the points of intersection of the sixe a clocke lines with the Horizon, are the two Semicircles of the Ecliptick, or Annuall circle of the Sunne: the vpper of which arches serueth for the Summer halfe yeare, and the lower for the Winter halfe yeare: and are therefore diuided in 365 dayes: which are also distinguished into 12 moneths with longer lines, hauing their names set downe: and into tenthes, and fifthes with shorter lines: and the rest of the dayes with pricks: as may plainly bee seene in the Instrument.
And this is for the ready finding out of the place of the Sunne euery day: and also for shewing of the Sunnes yearely motion: because by this motion the Sunne goeth round about the heauens in the compasse of a yeare, makeing [Page 115] the foure parts, or seasons thereof. Namely the Spring, in that quarter of the Ecliptick which beginneth at the intersection on the West side of the Instrument, and is therefore called the Vernall intersection. Then the Summer in that quarter of the Ecliptick which beginneth with the intersection of the Meridian in the highest point next the Zenith. And after that Autumne in that quarter of the Ecliptick, which beginneth at the intersection on the East side of the Instrument, and is therefore called the Autumnall intersection. And lastly, the Winter in that quarter of the Ecliptick, which beginneth at the intersection with the Meridian, in the lowest point next the Horizon.
But besides this yearely motion, the Sunne hath a Diurnall or dayly motion, whereby it maketh day and night with all the diuersities, and inequalities thereof: which is expressed by those other circles drawne crosse the houre lines: the middlemost whereof being grosser then the rest, meeting with the Ecliptick in the points of the Vernall, and Autumnall intersections, is the Aequinoctiall: and the rest on both sides of it, are called the Parallels, or Diurnall arches of the Sunne: the two outermost whereof are the Tropics, because in them the Sunne hath his furthest digression, or Declination from the Aequinoctiall, which is degrees 23½: and thence beginneth againe to returne to the Aequinoctiall. The vpper of the two Tropics next the center (in this our Northerne Hemisphaere) is the Tropick of Cancer: and the Sunne being in it, is highest into the North, making the longest day of Summer. And the lower next the Horizon, is called the Tropick of Capricorne; and the Sunne being in it, is lowest into the South, making the shortest day of Winter.
Betweene the two Tropics, and the Aequinoctiall infinite such parallel circles are vnderstoode to bee [Page 116] contained: for the Sunne is what point soeuer of the Ecliptick it is caried, describeth by his lation, a circle parallel to the Aequinoctial. Yet those parallels which are in the Instrument, though drawne but to euery second degree of Declination, may be sufficient to direct the eye, in imagining and tracing out, through euery day of the whole yeare in the Ecliptick, a proper circle, which may be the Diurnall arch of the Sunne for that day. For vpon the right estimation of that imaginary parallel, doth the manifold vse of this Instrument especially rely: because the true place of the Sunne, all that day, is in some part, or point of that circle. Wherefore for the better conceiuing, and bearing in minde thereof, euery fift parallel, is herein made a little grosser then the rest.
I Vse. And thus by the eye, and view only, to behold and comprehend the course of the Sunne, both for his Annuall and Diurnall motion, may be the first vse of this Instrument.
II Vse. To take the height of the Sun aboue the Horizon.
Set vp the pinne, (which is therefore made fit for the hole at the center) perpendicular in the center: and put the Indices on both sides, downe vpon the Meridian, that they with their waight, may not sway the Instrument any way as it hangeth: then with a threed put into the hole aboue in the handle, hang it perpendicularly, bearing the edge toward the Sunne, that the pinne may cast a shadow, vpon the degrees in the limbe: for that degree which the shadow of the pinne cutteth in the limbe, is the height of the Sunne aboue the Horizon, at that present.
[Page 117]III. Vse. To find the Declination of the Sunne euery day.
Looke the day of the moneth proposed in the Ecliptic, and marke how many degrees the prick shewing that day, is distant from the Equinoctiall, either on the Summer, or Winter side, viz North, or South.
Example. I. What will the Declination of the Sunne be, vpon the 11th day of August? Looke the 11th day of August: and you shall find it in the sixt Circle aboue the Aequinoctiall: now because each Parallel, standeth (as hath beene said before) for 2 degrees, the Sunne shall that day decline North-wards 12 degrees.
Example. II. What Declination hath the Sunne, vpon the 24th day of March? Looke the 24th day of March, and you shall find it, betweene the second, and third Northerne parallels, as it were an halfe and one fift part more of that distance from the second: reckon therefore 4 degrees for the two Circles, and one degree for the halfe space: so shall the Sunnes declination bee 5 degrees, and about one fift part of a degree Northward, that same day.
Example. III. What Declination hath the Sunne vpon the 13th day of Nouember? Looke the 13th day of Nouember, and you shall find it below the Equinoctiall, tenne parallels and about one quarter, which is 20 degrees, and an halfe South-wards. So much is the Declination. And according to these examples iudge of all the rest.
IIII. Vse. To find the Right ascension of the Sunne euery day.
Imagine an hower line through the day of the moneth giuen, and marke in what point it will cr [...]sse the [Page 118] Aequinoctiall: then lay a Ruler, or a streight Scroule of paper, to the Pole of the world (noted in the Instrument with P W) and that same point. For the Ruler shall in the innermost Circle of the limbe, of the South side, cut the Right ascension of the Sunne for that day, to be reckoned from the West, to the point of intersection, for the first, or vpper Semicircle of the Ecliptic: or from the East together with 180, for the second, or lower Semicircle of the Ecliptic.
V. Vse. To find the longitude of the Sunne, or in what degree of the Signe he is euery day.
The Pole of the first Semicircle of the Ecliptic is noted P I. and the Pole of the second Semicircle is noted P I I. Lay a Ruler, or a streight Scroule of paper, to the day of the moneth, and the proper Pole of the Semicircle of the Ecliptic, in which it is: for the Ruler shall in the innermost Circle of the limbe, on the South side, cut the degree of the Sunnes place in the Ecliptic, reckoning it in the same manner as you did in finding the Sunnes Right ascension: and the Arch thus found is called the longitude of the Sunne. which may bee expansed into signes, by reckoning on the limbe, from the West to South ♈, ♉, ♊, and from South to East ♋, ♌, ♍: then backe againe from East to South ♒, ♏, ♐; and lastly from South to West ♑ ♒, ♓, allowing 30 degrees, for each of those twelue signes.
VI. Vse. To find the Diurnall Arch, or Circle of the Sunnes course euery day.
The Sunne euery day by his motion (as hath beene said) describeth a Circle parallell to the Aequinoctiall, which is either one of the Circles in the Instrument, or [Page 119] some-where betweene two of them. First then seeke [...] of the moneth; and if it fall vpon one of those [...], that is the Circle of the Sunnes course that same day: But if it fall betweene any two of those Parallel [...], imagine in your minde, and estimate with your eye, another Parallel through that point, betweene those two Parallels, keeping still the same distance from each of them.
As in the first of the three former Examples, The circle of the Sunnes course, vpon the 11th day of August, shall be the very sixt Parallel aboue the Aequinoctiall towards the Center.
In Example II. The Circle of the Sunnes course vpon the 24th day of March, shall bee an imaginary Circle betweene the second, and third Parallels, still keeping an halfe of that space, and one fift part more of the rest from the second.
In Example III. The Circle of the Sunnes course vpon the 13th day of Nouember, shall be an imaginary Circle, betweene the tenth, and eleauenth Parallels, below the Aequinoctiall, still keeping one quarter of that space from the tenth.
VII. Vse. To find the Rising and Setting of the Sunne euery day.
Seeke out (as was last shewed) the imaginary Circle or Parallel of the Sunnes course, for that day, and marke the point where it meeteth with the Horizon, both on the East and West sides thereof, for that is the very point of the Sunnes rising, and setting that same day, and the hower lines which are on both sides of it, by proportioning the distance reasonably, according to 15 minuts, for the quarter of the hower, will shew the hower of the Sunnes rising, on the East side, and the Sunnes setting on the West side.
[Page 120]VIII. Vse. To know the reason, and manner, of the Increasing, and Decreasing of the dayes and nights throughout the whole yeare.
When the Sunne is in the Aequinoctiall, it riseth, and setteth at 6 a Clock, for in the instrument, the intersection of the Aequinoctiall, and the Ecliptic with the Horizon, is in the 6 a clock Circle on both sides. But if the Sunne bee out of the Aequinoctiall, declining toward the North, the intersections of the Parallel of the Sunne with the Horizon, is before 6 in the Morning, and after 6 in the Euening: and the diurnall Arch of the Sunne, greater then 12 howers; and so much more great, the greater the Northerne Declination is. Againe if the Sun be declining toward the South, the intersections of the Parallel of the Sunne with the Horizon, is after 6 in the Morning, and before 6 in the Euening; and the diurnall Arch lesser then 12 howers; and by so much lesser, the greater the Southerne Declination is.
And in those places of the Ecliptic in which the Sun most speedily changeth his Declination, the length also of the day is most altered, and where the Ecliptic goeth most parallel to the Aequinoctiall changing the Declination but little, the length of the day also is but little altered.
As for example, when the Sunne is neere vnto the Aequinoctiall, on both sides, the dayes increase, and also decrease suddenly and apace: because in those places, the Ecliptic inclineth to the Aequinoctiall in a manner like a streight line, making sensible declination. Againe when the Sunne is neere his greatest Declination, as in the height of the Summer, and the depth of Winter, the [Page 121] dayes keepe for a good time, as it were at one stay, because in those places the Ecliptic is in a manner parallel to the Aequinoctiall, scarce altering the declination: and because in those two times of the yeare, the Sunne standeth as it were still, at one declination; they are called the Summer Solstice, and the Winter Solstice. And in the meane spaces, the neerer every place is to the Aequinoctiall, the greater is the diversitie of dayes.
Wherefore we may hereby plainely see, that the common receiued opinion, that in every moneth, the dayes doe equally increase, is erroneous.
Also wee may see that in Parallels equally distant from the Aequinoctiall, the day on the one side, is equall to the night on the other side.
IX. Vse. To find the Ascensionall difference of the Sunne every day.
Seeke out the time of the Suns Rising, or Setting that same day (by the VII Vse) and see how much it differeth from sixe a clocke, then conuert the same difference into degrees (as was taught in 1 Part. Chap. 12. Sect. 1.) by multiplying the howers with their decimall parts, by 15. And so haue you the Ascensionall difference for that day.
X. Vse. To find out the Oblique ascension of the Sunne every day.
Seeke out the Sunnes Right ascension (by the IIII Vse) and the Ascensionall difference (by the IX Vse:) And if the Sunne be in the first Semicircle of the Ecliptic, Subduct the Ascensionall difference, out of the Right ascension: But if the Sunne be in the second Semicircle of the Ecliptic, adde the Ascensionall difference to the Right ascension: and you shall haue the oblique ascension.
[Page 122]XI. Vse. To find how farre the Sunne riseth, and setteth, from the true East and West points, which is called the Sunnes Amplitude ortiue, and occasiue.
Seeke out (as was shewed in the VI. Vse) the imaginary Circle, or Parallel of the Sunnes course, and the points of that Circle in the Horizon, on the East, and West sides, cutteth the degree of the Amplitude Ortiue, and occasiue.
XII. Vse. To find the length of every day and night.
Double the hower of the Sunnes setting, and you shall haue the length of the day; and double the hower of the Sunnes rising, and you shall haue the length of the night.
XIII. Vse To find the true place of the Sunne, vpon the Instrument, which answereth to the point, wherein the Sunne is in the heauens: and is the ground of all the questions following.
Take with your Instrument the height of the Sunne, and reckon it on the moueable Index, or Labell: and then moue the said Labell, till you find the height of the Sunne, exactly to fall vpon the Parallel of the Sunne for that day, on the East side if it bee in the Fore-noone, and on the West side, if it bee in the After-noone; the point of intersection, where the Index, or Labell crosseth the Parallel, [Page 123] in that point of the Sunnes altitude, shall bee the true place of the Sunne on the Instrument.
XIIII. Vse. To find the Hower of the day.
The true place of the Sunne on the Instrument (found out as was last shewed) sheweth among the hower lines the true hower of the day.
XV. Vse. To find out the Azumith or verticall Circle in which the Sunne is, or the Horizontall distance of the Sunne from the Meridian.
The Index or Labell fastned at the Center, is a moueable Azumith: apply therefore the edge thereof, vnto the true place of the Sunne on the instrument (found out as was shewed by XIII. Vse.) And marke what point of the Horizon, or Limbe, the same edge of the Labell cutteth; reckon how many degrees of the H [...]rizon, are intercepted betweene that point, and the Meridian line, or South point, either on the East, or West side: and that Arch shall be the Horizontall distance sought for, whereby is shewed the Azumith of the Sunne at that instant: and consequently the Angle which the verticall Circle, or Azumith of the Sunne maketh with the Meridian.
XVI. Vse. The Azumith of the Sunne being knowne, to find out the Altitude of the Sunne, and the Hower of the day.
Set the edge of the Labell to the Azumith given, and marke in what point the same edge crosseth the Parallel of the Sunne for that day: that point of intersection [Page 124] sheweth the height of the Sunne aboue the Horizon, vpon the Labell: and also it sheweth the hower of the day among the hower lines.
XVII. Vse. To find at what hower the Sunne commeth to be full East, or West every day in Summer.
Apply the edge of the Labell, vnto the East, or West points of the Limbe, and marke in what point, the said edge cutteth the Parallel of the Sunne for that day, for that same point among the hower lines, shall shew the time of the Sunnes comming to be full East, or West in that day, and likewise of what altitude the Sunne will be aboue the Horizon, at that time of his being full East, or West.
XVIII. Vse. To find the height of the Sunne at high Noone every day, and likewise at every other hower.
Marke in what point the Parallel of the Sunne for that day, cutteth the line of that hower, for which you would know the Sunnes altitude: And vnto that point of intersection, apply the edge of the moueable Labell, or Index: and thereon shall you find, the very degree of the Sunnes altitude, at that hower.
By this XVIII Vse, and by the XVI, are made the Quadrants, described by Gemma Frizius, Munster, Clauins, Mr. Gunter, and others: and also all manner of Rings, Cylinders, & inuumerable other topicall Instruments, for the finding out of the hower, and other like conclusions. And likewise the reason, of finding the hower of the day, by a mans shadow, or by the shadow of any Gnomon, set vp perpendicular to the Horizon, or else parallel to it.
[Page 125]XIX. Vse. To find out the Meridian line, and the points of the compasse without a Magneticall needle, yea more exactly then with a needle.
Take the height of the Sunne, by the shadow of the pinne: and apply the same height, reckoned on the Index, or Labell to the parallel of the Sunne for that day, whereby you haue the true place of the Sunne, in the instrument, as hath beene shewed in the XIII. Vse. Then keeping both the Labell at that point, and the pinne vpright in the Center, hold, or set your instrument parallel to the plaine of the Horizon, with the pinne toward the Sunne, and moue it gently, till the shadow of the pinne shall fall, exactly vpon, the fiduciall edge of the Labell. For then the Meridian line of the instrument, shall be in the true Meridian of the place: and the foure quarters of the instrument, shall looke into the foure cardinall points, of East, West, North, and South. Wherefore if with a bodkin, you make a prick at each end of the Meridian of your instrument where it standeth: and with a Ruler draw a line through them: the same shall bee the Meridian of that place.
This is a most excellent practise, for finding out the Meridian in any place, and is in an instant performed, and that easily. And hereby you may examine the Variation of the Compasse. And also exactly place any Sunne Dyall.
XX. Vse. Consid [...]rations for the vse of the instrument in the night.
In such questions as concerne the night, or the time before Sun rising, and after Sunne setting, the instrument representeth the lower Hemisphaere, wherin the Southerne [Page 126] Pole is eleuated. And therefore the Parallels, which are aboue the Aequinoctiall, shall bee for the Southerne, or Winter Parallels, and those beneath the Aequinoctiall, for the Northerne, or Summer parallels. And the East shall be accounted for West, and the West for East: and the North shall bee accounted for South, and the South for North: contrary to that which was before, when the Instrument represented the vpper Hemisphaere.
XXI. Vse. To find how many degrees the Sunne is vnder the Horizon, at any time of the night.
Seeke the declination of the Sunne for the day proposed: and at the same declination, on the contrary side, imagine a Parallel for the Sunne that night: and marke what point of it is in the very hower and minute proposed: then set the Index, or Labell to that point of the Parallel, and it will shew you thereon the degree of the Sunnes depression vnder the Horizon.
XXII. Vse. To find out the length of the Crepusculum, or Twilight euery day.
Because the question concerneth the night time, you must seeke out the Sunnes Parallel, for the night, on the other side of the Aequinoctiall, hauing the same declination with that which the day of the moneth sheweth: then moue about the Labell, vntill the said Parallel cutteth the edge thereof in the 18th deg: on the West side for the Morning Twilight, and on the East side for the Evening Twilight, of the same day.
And note that in the height of Summer, the Twilight in our Horizon, continueth all night long: because [Page 127] the same goeth not vnder the Horizon, full 18 degrees
XXIII. Vse. To find the Declination of any Wall, or Plaine.
Take a board hauing one streight edge, and a line drawne perpendicular vnto that edge: apply the streight edge vnto the Wall, at what time the Sunne shineth theron, holding the board parallel to the plaine of the Horizon: and hang vp a thread with a plummet, so that the shadow of the thread may fall on the board, crossing that perpendicular line. Then take with your Instrument the height of the Sunne, and instantly make two pricks, in the shadow of the thread on the board, a good way distant one from the other: and laying a Ruler to those two pricks, draw a line, which line shall be the Azumith of the Sunne, on the board: againe with the height of the Sunne lastly taken, find out on your instrument, the Azumith of the Sunne; or the Angle which the Sunnes Azumith maketh with the Meridian, (by the XV. Vse.) And on the board taking the intersection of the shadow line with the perpendicular for the Center, describe a Circle equall to the innermost Circle of the Limbe: (which you may easily doe, if you set one foot of your compasses vpon the East, or West point, and extend the other foot vnto 60 degrees, on the same innermost Circle, for this distance is equall to the Radius thereof.) Againe with your compasses, take of the Arch betweene the Azumith of your Instrument, and the Meridian, and set that on the Circle of the board, that way that the true South is: and through the end of that Arch measured on the board, draw a streight line for the Meridian. Lastly take with your compasses, the Arch intercepted between the Meridian on the board, and the perpendicular line, and by applying it to the in most Circle of the limbe, from the East, or West points see how many degrees it [Page 128] containeth: for that is the declination of the Wall. Or else you may find the Meridian vpon the board, by XIX Vse.
If the Angle of the Meridian with the perpendicular, on the board, be a right Angle, the Wall is direct East, or West.
But if the Meridian fall vpon the perpendicular, or be parallel there to making no Angle with it, the Wall is direct North, or South.
XXIIII. Vse. The Art of Dyalling. And first how to make the Instrument in paper, promised in the beginning of this second part.
For the Delincation of this instrument in paper, it will bee necessary first to shew the manner how the Semidiameter is to bee graduated, or diuided into degrees: and how the Centers, and Semidiameters, of the seuerall kinds of Arches are to be found.
Vpon halfe a sheet of strong large Dutch paper, (the larger, the better) draw two streight lines, making a right Angle neere one of the corners, the one through the length, and the other through the breadth of the paper; which two lines I therefore call the longer, and the shorter perpendicular.
Vpon the right Angle point, being the Center, with a Semidiameter equall to that by which you intend to delineate your instrument, describe a quadrant of a Circle: and on the point where it meeteth with the shorter perpendicular, draw a long tangent line parallel to the longer pependicular.
Divide the Quadrant into 90 degrees, among which from the beginning at the shorter perpendicular, reckon the eleuation of the Pole, for which you will make your [Page 129] instrument, and applying a Ruler to the end thereof, and to the Center, where the Ruler cutteth the tangent line make a prick. And taking with your compasses the distance from the Center to that prick, measure it vpon the shorter perpendicular: this shall be the Semidiameter of the sixt hower Circle. At the end thereof draw another long line parallel also to the longer perpendicular.
Then out of the Center vnto the second parallel through every degree of the quadrant, draw fine streight lines, cutting also the first Parallel. The intersection of those lines with the first Parallel, shall be The scale of centers of Arches. And their intersection with the second Parallel shall be The scale of centers of hower Circles. And the segments of those lines, intercepted betweene the Center, and the first Parallel, shall be the Semidiameters of Arches: and the whole lines betweene the Center and the second Parallel, shall bee The Semidiameters of hower Circles. And that you may know for what Circle, every Center, and Semidiameter serueth, you shall note every fift line from the beginning, with the figures 5, 10, 15, 20, &c. Set vnder the second Parallel, vnto 90 which will fall vpon the longer perpendicular: that so you may readily find the Center, and Semidiameter of any Circle required.
Againe divide the first 45 degrees of the Quadrant in the middest: and applying your Ruler to the Center, and to every one of those halfe divisions, where in each place the Ruler cutteth the first Parallel, or tangent line, make a prick. So shall you haue vpon the tangent line betweene the shorter perpendicular and the midlemost line 45, a third scale, which is, The scale of 90 degrees, for the graduating of the Semidiameter of your instrument on the paper: In which you shall also distinguish every fift degree, with figures set vnder the tangent line.
Having thus prepared your paper of scales with lines [Page 130] neatly and exactly drawne, keepe it by you to haue it still in a readinesse for the making, and vsing of the Instrument in paper. The making whereof is thus.
Take with your compasses the Semidiameter of the Quadrant in your paper of scales: and therewith vpon a peice of strong Dutch paper, Describe the Horizontall Circle: which you shall cut into two Semicircles with a Meri [...]ian line drawne through the Center: divide them into Quadrants in the points of East, and West: and each Q [...]adr [...]nt into 90 degrees to be marked with figures iust as is done in the Instrument.
Then with your compasses take the eleuation of the pole vpon the scale of degrees in your paper: & set it vpon the Meridian line from the Center which way you please: that shall bee the intersection of the Aequinoctiall with the Meridian. Also reckon the complement of the height of the Pole, vpon the scale of Centers of Arches, and with your compasses take the distance from the end therof to the Center: the same shall bee the Semidiameter of the Aequinoctiall, to bee drawne from the East point of the Horizon through the point of intersection with the Meridian vnto the West point.
Againe take with your compasses vpon the scale of degrees in your paper the complement of the height of the Pole: and set it vpon the Meridian on the other side of the Center from the Aequinoctiall: there shall bee the Pole of the Aequinoctiall, or of the World, in which all the houre lines shall crosse one another.
Nextly vnto the height of the Pole both adde, and also subduct 23½ degrees: and with your compasses take both those Arches in the scale of degrees: and set them in the Meridian from the Center, one falling beyond the Aequinoctiall, and the other short of it: those shall be the intersections of the two Tropics with the Meridian. Seek [Page] [Page]
[Page 131] also by Sect: 8, Chapt: 12 of the first part, the Amplitude ortiue of the Sun, having 23½ degrees declination: and reckon it being found, in the Horizontall Circle from the East and West points both wayes: those are the points of intersection of the Tropics with the Horizon on both sides: and so having three points in each Tropic, you may easily through them drawe the Circles.
Moreover with your compasses, take the distance betweene the Center and the second Parallel in your paper, which is the Semidiameter of the sixt houre Circle: and set it on the Meridian from the Pole beyond the Aequinoctiall: that shall be the Center of the sixt houre Circle: vpon which you may draw the same Circle, from the East point of the Horizon through the Pole to the West point. Then through the center of the sixt houre Circle erect a line perpendicular to the Meridian, extending it infinit [...]y on both sides of the Meridian: and in that line both wayes, pricke downe the Centers of the horary Circles, out of the scale in paper: And lastly opening your compasses from every one of those Centers vnto the Pole severally, describe all the horary Circles, or at least every fift of them, and so is your paper instrument perfectly finished.
The vse of this instrument on paper is, that lines, and arches may bee designed vpon it with a fine pennicell of blacke lead, and afterward be wiped out againe. Wherefore it will bee needfull for him that will vse this instrument, to all the purposes thereof, to get a good paire of large compasses with three points, [...]ne sharpe, another for inke, a third for blacke Lead. And I suppose it would doe well to fast [...]n over your instrument a peice of thinne oyled paper, through which the lineaments may be conspicuous: and vpon it to trace such lines, and arches as you haue occasion to vse: that so your instrument may be kept cleane, and last longer.
[Page 132] For as much as in delineating the horary Circles, which are within 30 degrees of the Meridian, the Semidiameters will be too long for your compasses: you may in that streight thus helpe your selfe. First say, As the Radius, is to the Sine of the Eleuation of the Pole; So is the tang: of the distance of any Horary Circle from the Meridian, suppose 25, or 20, or 15, or 10, or 5 degrees, to the arch of the Horizon betweene the Meridian, and that horary Circle.
Reckon this distance on the limbe of your Instrument from both ends of the Meridian, and marke it. Thus doe for the 25th, 20th, 15th, 10th, and 5th horary Circle on both sides of each end of the Meridian.
Then in any peice of cleane paper, through the middest of the longer way, draw aline: and toward one end which (I call the upper ende) crosse the same with a perpendicular line exactly equall to the Diameter of your Instrument, the point of Intersection being the center.
Take with your Compasses out of the paper of scales, the semidiameter of 60. degr: (which you may well doe for an ordinary instrument): and setting one foot on either end of the Diameter, that point wherein the other foot shall cutt the first long line, make your Center, and thereon draw an Arch through both ends of the Diameter, and cutting the vpper part of the first long line: this Arch is equall to that horary Circle, which is distant from the Meridian 30 degrees the complement of 60.
[Page 134] Divide each halfe of the Diameter into 3 equall parts, with 4 points, and from every of those points vnto the Arch draw lines parallel to the first long line. And having divided euery one of those fiue parallel lines intercepted betweene the Diameter and the Arch into 6 equall parts, for the 6 times 5 degrees which remaine to the Meridian, draw through those divisions from the ends of the Diameter (with a smooth and even hand) the Arches 25 20, 15, 10 and 5.
Those Arches you may transferre from the paper to your instrument in this manner. Rubb the backe side of the paper against the Arches, with fine powder of blacke lead: then applying the paper with Arches to your instrument, that the ends of the Diameter may exactly fall vpon the two opposite markes, in the limbe of your instrument, which serue for the horary Circle that you would draw, either 25, 20, 15, 10, or 5, trace over that Arch with the point of any hard peice of wood sharpened: and the blacke lead on the backe side will vpon the instrument leaue the print of that Arch.
XXV. Vse. To set an vpright Wall or plaine vpon the instrument: and to find how many houres the Sunne shall shine thereon at some time of the yeare.
The situation of Wals, or Plaines is considered either in respect of the Meridian, or of the Horizon. And vnto both it is either perpendicular, or oblique, or parallel.
The plaine perpendicular to the Meridian, is that which standeth directly North, or South: which if it be also perpendicular to the Horizon, is called North, or South direct vpright. But if it stoope from the Zenith forward, it is called North, or South inclining: if backeward, [Page 135] it is called North or South reclining. And note that in a stooping Plaine that side which is toward the Horizon, is inclining, and that which is toward the Zenith is reclining.
The Plaine oblique to the Meridian is that which standeth not directly North, or South, but declineth one side into the East, and the other into the West: and is therefore called Declining Eastward, or Westward, according as either side of the Plaine looketh: As if an vpright Wall being Southerne, declineth from the South into the East, it is called South declining Eastwards vpright. But if it be not vpright, it is called South declining Eastward, and inclining, or reclining.
The Plaine parallel to the Meridian, is that which looketh directly East, or West; and accordingly, hath his denomination, whether it bee Vpright, Inclining, or Reclining.
The Plaine Parallel to the Horizon, is called Horizontall: and is represented by the instrument it selfe, or at least by the inner most Circle of the limbe thereof.
And note that the Arch of Declination, is reckoned from the next East, or West point. And that the Arch of Inclination, or Reclination is reckoned from the Zenith, or the complement of it from the Horizon. So that euery vpright Plaine is vnderstood to passe through the Zenith, which in the instrument is the Center.
And thus having shewed the seuerall affections of Plaines, wee will now proceed to shew the manner how to set them vpon the Instrument.
A Direct North, or South vpright Plaine, is represented in the instrument by a line drawne through the Center from the East point to the West, which is also the Horizontall intersection of the Pla [...]ne. And by it you [Page 136] shall see that the Southerne side or face of the plaine is open to all the houres betweene sixe in the morning and sixe in the evening. And that about London, the Northerne side, onely in the Summer enioyeth the Sunne from his rising till after seven in the morning: and from before 5 a clocke in the afternoone, till his setting.
A direct East, or West upright plaine, is represented in the Instrument by the Meridian, which is also the Horizontall intersection of the plaine. And in it you shall see that all the forenoone houres are open to the East side: and all the afternoone houres to the West side.
A Declining Plaine is thus set upon the Instrument, reckon on the Horizon the arch of Declination, from the East, or West point: and at the end draw a line through the Center vnto the opposite point of the Horizon: So that each side thereof may be open to that point, either East, or West, into which the Declination is supposed. That line so drawne throught the center is the Horizontall intersection of the plaine, and representeth the plaine it selfe, if it bee vpright. For example, there is about London an vpright Wall declining Eastwards 35 degrees: which I would set vpon the Instrument. Hold the Southerne part of the Instrument to you, and reckon from the East backward into the North vpon the Horizon 35 degrees: there draw a line through the Center: this line shall not onely vpon the South side represent a Southerne Plaine declining Eastward 35 degrees. But also vpon the North side shall represent a Northerne Plaine declining Westward 35 deg. And moreover it will appeare that on the Southerne side shall bee drawne the houres from almost 4 a clocke in the morning, till 3 in the afternoone. And that in the Northerne side shall bee drawne vpon one side 4 a clocke in the morning onely: and vpon the other side all the houres from 3 in the afternoone till Sunne set.
[Page 137] And [...]o consequently the declination of an vpright wall, or Window being given, it may be found at what houre the Sunne vpon any day in the yeare will come to that Wall, or Window, and when it will goe from it. As in the former example, There is about London a Northerne wall declining Westward 35 deg. I would know at what time of the day the Sunne will begin to shine vpon it on the 24th day of March. Set the Index at 35 deg: from West toward South: and because that day the Sunnes Declination is 6 degrees Northward; Looke at what houre the sixt Parallel aboue the Aequinoctiall toward the Center meeteth with the Index so placed: and you shall find it at 3 [...] clock in the Afternoone. Wherefore at that time the Sunne will begin to shine vpon the Wall that same day.
The Poles of every vpright Wall are in the Horizon 90 deg: that is a quarter of a Circle, distant from the line representing the Plaine. Wherefore if vpon that line in the Center you erect a perpendicular, the ends therof in the Horizon shall be the poles of that Plaine: and are so farre distant from the North and South points, as the Plaine it selfe is from the East, and West.
XXVI. Vse. To set an Inclining, and Reclining Wall, or Plaine vpon the Instrument: and to find how many houres the Sunne shall shine thereon, at some time of the yeare.
When you haue an Inclining, or Reclining Plaine to be described on the Instrument. First the Horizontall intersection is to be set thereon, as if it were vpright; together with the line perpendicular thereto, in which are the Poles of the Plaine: according as was taught in the XXV Vse.
[Page 138] Then vpon the scale of degrees in your paper, reckon the arch of Inclination, or Reclination; and with your compasses take, & set it in your Instrument vpon the line perpendicular to the Horizontall intersection of your Plaine, from the Center that way into which the Inclination, or Reclination tendeth: the same shall bee the vppermost point of your Plaine.
Againe, with your Compasses take the Complement of inclination, or reclination, both upon the scale of degrees, and also upon the scale of centers of arches in your paper: and set both spaces upon the same perpendicular line, but on the other side of the center (extended if need be): At the shorter of those spaces shal be the pole of your plaine: and at the longer of them shal be the Center of it.
Lastly, setting one foot of your Compasses in the center of your Plaine, and extending the other foot to the vppermost point, describe in your Instrument an Arch of a Circle: which if you haue done well, will exactly fall vpon the ends of the Horizontal intersection of your Plaine. That Arch shall represent your Plaine, inclining vpon the lower side, which is toward the Horizon, or Limbe: but reclining vpon the vpper-side, which is toward the Zenith, or Center. And so either side shall shew in what hower lines the Sunne, at some time of the yeare, will shine vpon it: that in delineating a Dyall thereon, it may not be combered with vnnecessary houre lines. For Example, suppose that the former Plaine, which with the South declined Eastward 35 deg: doe also incline 41 deg: 30 min. Wherefore also with the North side it shall decline Westward 35 deg: and Recline 41 deg: 30 min. Describe this plaine vpon your Instrument with an Arch of a Circle, found out as was taught last before. And it will appeare that vpon the Inclining side shall be drawne all the houre lines from almost 4 in the morning, to 4 in the afternoone: And vpon the Reclining side shall bee drawne first 4 and 5 in the morning: and then beginning at 0 a clocke, all houres to Sunne set.
[Page 139] And note that in all Northerne plaines, the North Pole is eleuated: and in all Southerne plaines the South Pole is eleuated. Except such North inclining, and South reclining Plaines, that in the Instrument fall below the North Pole, betweene it and the Horizon: For in them the contrary Pole is eleuated. And also that a direct East and West plaine, if it Recline, hath the North Pole eleuated: and if it Incline, the South Pole.
XXVII. Vse. The Plaine being set vpon the Instrument, to find the distances of the houre lines, and Substile from the Horizontall Intersection. And also the height of the Stile aboue the Substile.
Euery Dyall either hath a Center in which all the houre lines, together with the Substile, and Stile doe meet: or else it hath no center, & so they are al parallel one to another.
If the Plaine being set vpon the Instrument, cutteth the Pole of the Aequinoctiall (that is the point in which all the horary Circles crosse the Meridian) the Dyal to be drawne vpon that Plaine shall haue no Center. But if it cutteth not the Pole, the Dyal shall haue a Center. And of these Dyals with Centers wee will first intreate: as being most proper for the vse of the Instrument.
Behold therefore the Pole of your plaine heedily what horary Circle it falleth vpon: Or if it fall betweene any two, the distance of each being reasonably apportioned, imagine a horary Circle passing through it. Marke in what point that horary Circle, either real, or imagined, doth cut the Plaine, that same point shall bee the place of the Substile in your Plaine: and the height of the Stile aboue it, is the Arch of that horary Circle intercepted betwixt the Pole of the Aequinoctial, and the point of the Substile noted in the Plaine.
[Page 140] Therefore applying a Ruler to the Pole of your Plaine, carry it about vnto all the intersections of the Plaine with the houre Circles, and the substile seuerally: and where in euery place the Ruler shall cut the innermost Circle of the Limbe, there make a visible marke: For the arches of the Limbe intercepted betweene the Horizontall points of your Plaine, and euery one of those marks, shall be the distance intended to be sought.
But for the Horizontall plaine, the ends of the houre Circles in the Limbe of your instrument, doe giue the distance without any more adoe.
Concerning the height of the Stile aboue the Substile: It is apparent by the instrument, that in a Horizontal dyal, the 6 a clocke line lyeth directly East and West: and the Meridian perpendicular to it, directly North and South. And that the Meridian is the Substile. And that the height of the Stile aboue the Substile, is equall to the height of the Pole in that place.
It is also apparent, that in all direct North and South Dyals, the 6 a clocke Line is drawne parallel to the Horizon, and the Meridian perpendicular to it: And that the Meridian is the substile. And that the height of the Stile aboue the substile, if the Plaine bee vpright, is equall to the complement of the height of the Pole. But if it be North inclining, or South Reclining, it is equall to the difference, of the height of the Pole, and the Arch of Inclination, or Reclination. And if the Plaine bee North Reclining, or South Inclining, it is equall to the Summe of the complement of the height of the Pole and of the Arch of Inclination, or Reclination. And if the Plaine fall vpon the Aequinoctiall, the stile shall stand vp perpendicular vpon it in the Center: and the hower lines shall be drawne all at equall Angles, viz. 15 degrees one from another.
[Page 141] In such Dyals as haue not the Meridian for the substile, the height of the Stile aboue the Substile is thus sound by the Instrument. It was shewed before that the height of the stile aboue the substile is the Arch of the horary Circle through the Pole of the Plaine, intercepted betweene the pole of the Aequinoctiall, and the point noted in the Plaine for the substile. Therefore from the Horizontall points, or intersections of that horary Circle reckon 90 degrees both wayes: and thereto through the Center draw an obscure line: in which line shall be both the Inclination of that horary Circle, which is the distance of the intersection, or vppermost point thereof from the Center: and also the Pole. Then with your compasses take that distance, or Inclination: and setting it vpon the scale of degrees in your paper, see how many degrees it containeth vpon that scal [...]. Againe vpon the same scale take with your compasses the complement of that inclination or distance, which being set vpon the obscure line on the other side of the Center, shall shew the Pole of that horary Circle. Lastly applying a Ruler to the Pole of that horary Circle, and both to the Pole of the Aequinoctiall, and to the point of the substile in the Plaine seuerally: marke where in both places the Ruler cutteth the innermost limbe of your instrument: For the degrees of the limbe intercepted betwixt those markes, shall be the height of the stile, aboue the substile, which was sought for.
And by this which hath beene taught you shall find that in an vpright Dyall declining, as before 35 deg: from the South into the East, or from the North into the West, the substile shall fall vpon that horary Circle, which is about 3 deg: after 9 a clock in the morning: and the stile eleuated aboue the substile about 31 deg: And also that in a South Dyall declining Eastward 35 deg: and inclining 41 deg: 30 min: Or in a North declining Westward 35 deg: and reclining 41 deg: 30 min: the [Page 42] substile shall fall vpon that horary Circle which is about 8 degrees after 6 a clock: and the stile eleuated aboue the substile about 63 deg. 30 minutes.
XXVIII. Vse. The making of all manner of plaine Dyals with Centers.
I haue already shewed how to find out in our Instrument the distances of all the houre lines, and the substile, from the Horizontal intersection. Now the delineating of a Dyal is nothing else but to transferre those distances out of your Instrument into the Dyal plaine, euery one in his due situation: and then through them, out of the Center, to draw such houre lines as shall be of vse, together with the substile.
The due situation of those distances vpon the Dyal plaine, dependeth on the true placing of the Meridian, or 12 a clocke line: for that being truely described, all the rest will be easie enough.
First therefore I will shew the manner how the Meridian, or 12 a clocke line, is to be described.
Take in your Dyal some point for the Center, where you shall thinke fit: and through it draw a line parallel to the plaine of the Horizon. Crosse it in the Center with a perpendicular line. And hauing opened your compasses to the length of the Semidiameter of your paper Instrument, describe on the Center a Circle equall to the innermost Limbe thereof. In which Circle the line parallel to the Horizon is for the Horizontal intersection: and the other for the line perpendicular to it: and the Circle it selfe representeth the plaine: Marke therein the East and West sides of the Plaine with E and W.
In the Horizontal, and in al North and South direct Plaines, both vpright, and stooping; and in all vpright [Page 143] declining plaines, the Meridian is perpendicular to the Line parallel to the Horizon.
In North [...]clining, and South reclining plaines, the Meridian is to bee drawne on that side of the Dyal plaine either East, or West, into which the declination is: But in North inclining and South reclining, on the contrary side. And if the plaine bee Northerne, the Meridian shall be aboue the Line parallel to the Horizon: and if the plaine be Southerne, it shal be vnder it. And if the contrary Pole be eleuated, it shall be drawne through the Center into the opposite Quadrant of the Circle in your Dyal plaine.
Lastly in a direct East and West plaine, both inclining and reclining, the Meridian is the same with the line parallel to the Horizon.
Wherefore with your compasses take the distance in the limbe of your Instrument, from the next Horizontall point, vnto the marke of the Meridian; and measure it vpon the Circle of the Dyal plaine, in that part, and on that side, according as in consideration of the eleuated Pole, and of the qualitie of the Plaine, was shewed to be agreeable. And at the end of that arch, through the Center, draw a line for the Meridian.
Againe with your compasses take the distances in the limbe of your Instrument, betweene the marke of the Meridian, and the markes of all the houre Lines seuerally: and setting them vpon the Circle of the Dyal plaine orderly from the Meridian, the Forenoone houres on the West side of it, and the Afternoone houres on the East side: at the end of euery one of those arches draw the houre Lines: and distinguish them with their proper figures accordingly.
Lastly fasten the stile in the Center, so that it may hang perpendicular vnto the plaine in the Substile, at the iust height. And because the stile in every Dyal is vnderstood to be a segment of the Axis of the world [Page 144] which is a line imagined to passe from the North to the South Pole through the Center of the earth; the stile being rightly placed shal still with the end point towards the eleuated Pole, that is vpward from the Center, if the North Pole be eleuated; or downeward from the Center if the South Pole be eleuated.
XXIX. Vse. The making of all manner of plaine Dyals not hauing Centers.
If the plaine represented on the Instrument (as was taught before in the XXV and XXVI Vses) cut the Pole of the Aequinoctiall, it is an horary Circle, either one of them which are drawne in the Instrument, or falling betweene some two of them: and the Dyall plaine it selfe shall not crosse the axis of the world, but lye parallel to it, without any Angle of eleuation. And therefore such a Dyal can haue no Center: But the stile, the substile, and all the houre lines shall be parallel one to another.
Every such Plaine represented on the Instrument,
Either, First it is the Meridian of the place, the Horizontall intersection whereof is the 12 a clocke Line drawne from North to South: and the Dyall made thereon, is a direct East, or West vpright Dyal: In which the substile is distant from the Line, in the Circle of the Dyall plaine parallel to the Horizon, with an Arch equall to the eleuation of the Pole, and vpward toward the Pole. And is also the 6 a clocke line in your Dyal.
The rest of the houre lines are thus described. Draw through the substile, in any point, a long Line at right Angles: that line shall bee the Aequinoctial intersection vsually called the Contingent line: And taking a conuenient distance for the stile to hang parallel over the substile (according to the greatnesse of your Dyall plaine) [Page 145] measure it vpon the substile from the Aequinoctiall intersection: and vpon the end of that measure, describe halfe a Circle for the Aequinoctiall it selfe. Diuide each Quadrant thereof from the substile, into 6 equall parts, or houres. Then applying a Ruler to the Center, and to euery one of those diuisions seuerally, where in euery place the Ruler shall cut the long line of Aequinoctiall intersection, make pricks: and through those pricks draw the houre lines, parallel to the Substile, or 6 a clocke line: distinguishing so many of them as bee needfull, with their figures: that is all the Forenoone houres on the East plaine, and all the Afternoone houres on the West plaine. But in these Dyals there is no 12 a clock line, it being infinitly distant from the Substile. Lastly hang the stile directly over the Substile, and parallel to it, at the distance formerly taken. And thus are your East, and West Dyals finished.
Or Secondly, it is the sixt houre Circle, the Horizontal intersection whereof is the line of East, and West: and the Dyal made thereon is direct North inclining, or South reclining, with an Arch equal to the complement of the height of the Pole. And the parallel to the Horizon is the Aequinoctial intersection: and the line perpendicular to it is the 12 a clocke line, and also the Substile.
The rest of the houre Lines, from 7 a clocke in the morning, to 5 in the euening, are thus described. Take a conuenient distance for the Stile from the Substile, measuring it vpon the Substile from the Aequinoctial intersection: and on the end of that space describe the Semicircle of the Aequinoctial, to bee diuided on both sides of the Substile into 6 houres: through euery one of which out of the Center, a Ruler being applyed; at the points of the seuerall intersections of the Ruler with the Aequinoctial intersection, draw the houre Lines parallel to the Substile, or 12 a clocke Line: distinguishing them with their figures, namely 11, 10, 9, 8, 7, on the West side: [Page 146] and 1, 2, 3, 4, 5, on the East side: but in these Dyals there is no sixe a clocke Line, it being infinitly distant from the Substile. Lastly hang the Stile directly over the Substile, and parallel to it, at the distance formerly taken.
Or Thirdly, it is North inclining, or South reclining, and also declining: in which.
As the tangent of the Eleuation of the Pole, is to the Radius; So is the Sine of the compl: of Declination, to the tang: of the compl: of Inclination or Reclination.
The Plaine being set vpon the Instrument by the Arches of Declination and stooping thereof (as hath beene taught in XXV [...] Vse) shall cut the pole of the Aequinoctiall. Apply therefore a Ruler to the Pole of the plaine, and to the Pole of the Aequinoctial; and the point in which it cutteth the Limbe, marke for the substile: which is to bee transferred vnto the Circle of the Dyal plaine, by taking the distance betweene that point, and the next Horizontal intersection, and setting it on that Circle from the line parallel to the Horizon, vpward if the plaine be North: or downe-ward if the plaine bee South: and on that side which is contrary to the Declination. The substile being thus sound, draw a long line perpendicular to it, for the Aequinoctial intersection. And taking a conuenient distance for the stile from the substile, measure it vpon the substile from the Aequinoctiall intersection: and on the end of that space describe the Semicircle of the Aequinoctial. Then looke in your Instrument how many degrees of the Aequinoctial are intercepted betweene the Meridian, and the Arch representing your Plaine: and reckoning the same number of degrees vpon the Aequinoctial of the Dyal plaine, from the substile towards the side of Declination, there make a marke for the Meridian point thereof: in which [Page 147] you must begin to diuide the Aequinoctial semicircle into houres both wayes: And that being diuided, apply a ruler to the center, and to euery one of the diuisions: and at the points of the seuerall intersections of the ruler with the Aequinoctial intersection, draw the houre lines parallel to the substile. Set 12 at that houre line which was drawne at the intersection through the Meridian point of the Equinoctial: and 11, 10, 9, 8, &c. on the West side: and 1, 2, 3, 4, &c, on the East side. Lastly, hang the stile directly ouer the substile, and parallel to it, at the distance formerly taken.
XXX Vse. How by Sines and tangents to calculate the places of the Meridian, and Substile, and the height of the Stile aboue it: and the distance of the Meridian of the Aequinoctiall from the Substile; together with the places of houre lines, both by calculation, and also Geometrically.
I haue already taught the making of all manner of plaine Dyals most easily by the Instrument, for the same height of the Pole. But if any man either want an Instrument, or else desireth greater exactnesse, I will also here shew how to performe the same by calculation, on the other side of the Instrument.
In a plaine erect Dyall declining.
As the Radius is to the Sine of doclination; So is the tang. of the compl. of the Poles height. to the tang. of the distance of the substile from the Meridian.
[Page 149] In plaine Dyalls both declining and also inclining, and reclining. As the Radius is to the Sine of inclination reclination So is the tang: of Declination, to the tang. of the compl. of the distance of the Meridian, from the line parallel to the horizon.
Againe As the Radius is to the Sine of the compl. of Declination; So is the tang. of the compl. of the Poles height, to the tang. of Base I.
If the Dyall be South reclining, or North inclining, the summe of Base I, and of the complement of Inclination or reclination shall be Base II. But if the Plaine be South inclining, or North reclining, the difference of Base I, and of the complement of inclination, or reclination shall bee Base II.
Then say thirdly, As the Sine of the compl. of Base I, is to the Sine of the compl. or excesse of Base II; So is the Sine of the height of the Poles to the Sine of the height of the stile aboue the substile.
Fourthly, As the Sine of the compl. of the height of the stile aboue the substile, is to the Sine of Declination; So is the Sine of the compl. of the height of the Pole, to the Sine of the compl. of the distance of the substile from the line parallel to the horizon.
[Page 148] Againe As the Radius is to the Sine of the compl. of Declination; So is the Sine of the compl. of the Poles height, to the Sine of the height of the stile aboue the substile.
Thirdly As the Sine of the Poles height is to the Radius; So is the tang. of Declination, to the tang. of the Distance of the Meridian of the Aequinoctiall from the substile. And this distance is euer lesse then 90 degrees.
In a plaine East and West Inclining and Reclining Dyall. As the Radius is to the Sine of the compl. of inclination reclination So is the tang. of the height of the Pole, to the tang. of the distance of the substile from the Meridian.
Againe As the Radius is to the Sine of inclination reclination So is the Sine of the height of the Pole, to the Sine of the height of the stile aboue the substile.
Thirdly, As the Sine of the compl. of the Poles height; is to the Radius; So is the tang. of the compl. of inclination reclination to the tang. of the distance of the Meridian of the Aequinoctiall from the substile. And this distance is euer greater then 90 degrees.
[Page 150] Fiftly As the Sine of the compl. of the height of the stile aboue the substile, is to the Sine of Declination; So is the Sine of the compl. of inclination reclination to the Sine of the distance of the Meridian of the Aequinoctiall from the substile.
And note that in South reclining, and North inclining Plaines, if Base II be lesse then a quadrant, the contrary pole is eleuated aboue the Plaine: And if Base II be equall to a quadrant, the Plaine doth cut the Pole of the Aequinoctiall.
Now concerning the placing of the substile vpon the Dyall plaine (as I haue already in the XXVIII Vse shewed for the Meridian) Wee are to know, First that the substile is to be drawne vpward from the line parallel to the horizon, if the Plaine be Northerne; or downeward from it, if it bee Southerne. Except in North reclining, and South inclining Dyalls, in which the Base I exceedeth the complement of inclination, and reclination: for in them it is quite contrary. And secondly that the substile is to be drawne in the contrary side from the Declination. But in North inclining, and South reclining Dyalls, in which the contrary Pole is eleuated, the substile must be drawne through the center into the opposite quadrant of your Dyall circle.
Lastly, the houre lines in all manner of plaine Dyalls, are thus to be found.
If the substile and houre bee both on the same side of the Meridian: the arch of the Aequinoctiall betweene the substile, and the houre line, shall bee equall to the difference of the two distances, namely of the houre line from noone, and of the Meridian of the Aequinoctiall from the substile. But if the substile bee vpon one side of the Meridian, [Page 151] and the houre on the other side: it shall be equall to the summe thereof. Then say As the Radius is to the Sine of the height of the stile aboue the substile; So is the tang. of the arch of the aequinoctiall, betweene the substile and the houre line, to the tang. of the arch of the circle of your Dyall plaine, betweene the substile and that lower line.
Or else you may without calculation Geometrically inscribe the houre lines in Dyals hauing centers (for how to doe it in Dyals not hauing centers, I haue already shewed in the XIX Vse) thus.
Describe in your Dyall plaine a line for the stile, at the same height or distance from the substile, that the true stile ought to haue. Take also in the substile (as in reason you shall see fit) a point, and through it draw at right angles a long line, for the contingent, or Aequinoctiall intersection. Againe from the same point let fall a perpendicular vnto the stile: the length of this perpendicular is the nearest distance betweene that point and the stile: and it is also the distance of the center of the Aequinoctiall from that point: measure it therefore vpon the substile, the contrary way from the center of the Dyall: and hauing thus the center of the Aequinoctiall, describe therevpon toward the contingent line one halfe of the Aequinoctiall circle: which if the substile be the Meridian, or 12 a clock line of your Dyall, you must begin to diuide into houres at the substile: But if the substile and Meridian of your Dyall be seuerall lines, apply a ruler to the center of the Aequinoctial, and to the intersection of the 12 a clock line with the contingent, and there draw a line: this line shal bee the Meridian of the Aequinoctial: at which you must begin to diuide the Aequinoctiall circle into houres, both wayes. Then applying a ruler vnto the center of the Aequinoctial & euery one of those diuisions, where [Page 152] the ruler in euery place shal cut the contingent line, there make a marke: and lastly, through euery one of those marks from the center of the Dyall, draw the houre lines themselues.
And if in any houre line it shall happen, that the ruler so applied will not reach to intersecat the contingent line: you may thus help your selfe. Which rule also may serue you to find the Meridian of the Aequinoctiall, as often as the intersection of the Meridian of the Dyall with the contingent, falleth without your paper or plaine.
Draw the houre line as farre as it will goe. And take with your Compasses the distance of the intersection point of the contingent with the substile, both from the center of the Dyal, & frō the center of the Aequinoctial. And taking at all aduenture a point in the contingent line, on that side in which the houre line is, measure from that point on the contingent, both those distances: and at the ends of them both draw two lines parallel to the substile, crossing the contingent. Then applying a ruler to the point, which you tooke at all aduenture, and to the intersection of the parallel, which hath the distance of that center, whence the houre line giuen proceedeth, with that houre line: where the ruler shall cut the other parallel, make a prick: and measure the distance betweene that prick and the contingent, vpon the former parallel, on the other side of the contingent. Lastly, out of the proper center through the end of that measure, draw a line: which shall be that you desire.
An example of this Geometricall way of delineating th [...] houre lines you shall finde in the description of a South vpright Dyall declining 35 degr. and reclining degr. 41 min. 30. by considering whereof these rules will be found exceeding plainely set downe: As also all the other rules and obseruations here deliuered, to one that is any whit pregnant and ingenious, will neede no other exemplification, then the inspection of the instrument it selfe, and of these seuerall Dyalls following
The Translator to the Reader.
Gentle Reader, by reason of my absence, whilest this Booke was in the Presse, it is no meruaile though some faults haue escaped, which you will be pleased to amend thus.
Pag. 14 lin. 14, 2.0413927. Pag. 15. lin. 1, the first terme of a progression Pag. 17, lin 17, the Antecedent arme Pag. 18 lin. 19, terme giuen from Pag. 19 lin. 11, in the fift circle Pag. 20 lin. 19, lye hid. As in this lin. 20 D. Rat. multa—1 in R. lin. 28, and Rat multa in R in α—R in α,
Also in the aequations pag. 21, 24, 26 which haue a magnitude equall to a fraction: the same magnitude together with the note of equality, ought to be set right against the line that is betweene the Numerator and Denominator of the fraction, as in these, [...]. And [...]. And so of the rest.
Pag. 25 lin. 20, arme at 71⌊382: Pag. 26 lin. 16, Ratiocination. Pag. 29 lin. 29. number of figures Pag. 35 lin. 5, 61 49/144 Pag. 36 lin. 11, 17⌊48 lin. 14, 17⌊48 · 3⌊26 +. Pag. 44 lin. 8, is a roofe line 26, therof Pag. 94 lin. 21, a circle, or 90 degrees. Pag. 100 lin. 3, and then the side DC Pag. 113 lin. 7, delineation Pag. 127 lin. 1, the Sunne goeth not Pag. 131 lin. 19, in the paper Pag. 132 lin. 10, to the tangent of the arch of Pag. 143 lin. 3, in North reclining, and South inclining Pag. 152 lin. 30 North Dyall declining Eastward 35 deg.