Astronomia Britannica exhibiting the doctrine of the sphere, and theory of the planets decimally by trigonometry, and by tables : fitted for the meridian of London ... / by John Newton ...

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Title
Astronomia Britannica exhibiting the doctrine of the sphere, and theory of the planets decimally by trigonometry, and by tables : fitted for the meridian of London ... / by John Newton ...
Author
Newton, John, 1622-1678.
Publication
London :: Printed for the author by R. and W. Leybourn, and are to be sold by Thomas Piercepoint ...,
1657.
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Subject terms
Astronomy -- Early works to 1800.
Planetary theory -- Early works to 1800.
Astronomy -- Mathematics -- Early works to 1800.
Cite this Item
"Astronomia Britannica exhibiting the doctrine of the sphere, and theory of the planets decimally by trigonometry, and by tables : fitted for the meridian of London ... / by John Newton ..." In the digital collection Early English Books Online. https://name.umdl.umich.edu/A52255.0001.001. University of Michigan Library Digital Collections. Accessed May 16, 2024.

Pages

Page 133

CHAP. 17. Of the Motion of Mercury.

THe forme of calculating the place of this Planet is the same with Venus, the Dimensions of whose orbs we shall give you, as the learned Bullialdus hath computed them, but first we will set down the middle motions thereof to the former time.

The middle motions of Mercury.

An. Christ.Longit. ☿Aphel. ☿Node ☿
1500352. 53750248. 73556039. 85639
8059. 534722. 316112. 12417
6326. 41889. 17361. 15917
Iuly147. 58583. 01694. 01528
D 165. 47806. 00126. 00117
H 183. 06917  
P 4564. 07781  
Meane Mot.234. 70198251. 2434842. 15618
Aphel. Snbt.251. 24348Rest Anom.343. 45850

The proportion between the Earths orb, and the orbe of Mercury is as 100. 000 to 38585 Semicentricity in the same parts is, 8105. The parts or greatest inclination 4635. And the angle it selfe 6. 90. In the trian∣gle therefore M E H, of the first Diagram of the former Chapter we have known. 1. The halfe sum of the opposite angles M E H and M H E, 8. 27075 the halfe of 16. 54150 which is the complement of the meane A∣nomaly, 343. 4585 to a circle.

2. The side M E77170 
3. The side M H16210 
Summe93380 co. ar.5. 0297462
Differ.609604. 7850449
So tang. halfe sum.8. 270759. 1628126
To tang. halfe differ.5. 425328. 9776037
Difference2. 84543 Angle M E H 
Difference doubled5. 69086 Angle M B H or the E∣quation to be added to the meane longitude, because the Anomaly is more then a semicircle. 

Example.
The meane Longitude of Mercury
234. 70198
Equation adde
5. 69086
Eccentrick place
240. 39284
Node subtract
42. 15618
Argument of Latitude K L
198. 23666

Page 134

To finde the distance of Mercury from the Sun.

As the sine of MBH5. 69086 co. ar.1. 0036592
To the side MH162104. 209780
So sine of EMH16. 541509. 4544022
To the side BH465414. 6678444

To finde the Reduction.

As Radius, to cosine of XKL6. 909. 9968431
So tangent of KL18. 236669. 5178453
To tangent of XK11. 113229. 5146884
Reduction12344 

And because the argument of Latitude is more then 180, it must be sub∣tracted from the eccentrick place 240. 39284

And then the eccentrick reduced will be. 240. 26940

To finde the present inclination.

As Radius  
To the greatest inclination EB46353. 6660497
So sine of KL.18. 236669. 4954646
To the inclinat. XL14503. 1615143

Which are the parts of inclination agreeing to the common Radius 38585. But the distance of Mercury from the Sun being put for Radius, the inclination will be. 1749

For as Radius DL38585 co. ar.5. 413585
To Mercury dist. BH or AL465414. 6678444
So is XL14503. 1615143
To XL17493. 2429402

To finde the distance corrected by Curtation.

As AL46541 co. ar.5. 3321556
To Radius 10. 0000000
So is XL17493. 2429402
To the sine of LAX2. 154378. 5750958
As Radius 10. 0000000
To AL465414. 6678444
So cosine of LAX2. 154379. 9996929
To AX465094. 6675373

To finde the second inequality of Mercury.

We must have given, 1. The Angle NAS which is to be found by sub∣ductiug the Suns place, from the eccentrick place of Mercury reduced, or this from it, so that less then 6 signes may remain, this remainer is the

Page 135

Anomaly of the orbe, and the complement thereof is the Angle NAS, or the halfe, is the halfe sum of the opposite angles.

Example.
The eccentrick of Mercury reduced
220. 26940
The Suns true place
154. 07347
Anomaly of the orbe
96. 19593
Complement is NAS
83. 80407
Halfe Anomaly
48. 09796

These given with the sides NA and SA. the Analogies are

As the greater side SA100895 co. ar.4. 9961293
Is to Radius 10. 0000000
So is the lesser side NA465094. 6675373
To the tangent of24. 747999. 6636666
Adde45. 
As Radius  
To the cotang. of69. 747999. 5669785
So tang. halfe summe48. 0979610. 0470559
To tang. halfe difference22. 351609. 6140344
Summe70. 44956 Angle ANS 
Difference25. 74636 Angle ASN 

Because the Suns place was subtracted from the eccentrick of Mercury reduced, therefore the angle of Elongation ASN must be added to the

Suns place.
154. 07347
Elongation ASN adde
25. 74636
True place of Mercury
179. 81983
To finde the distance of Mercury from the Earth.

As the sine of ANS70. 44956 co. ar.0. 0257891
To the side AS1008955. 0038707
So the sine of NAS83. 804079. 9974556
To the side SN1064425. 0271154

To finde the Latitude of Mercury from the Earth.

As the side SX106442 co. ar.4. 9728846
Is to Radius 10. 0000000
So is XL17493. 2429402
To the tang. of XSL0. 941698. 2158248
Which is the south Latitude of Mercury.  

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