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.
Link to this Item
http://name.umdl.umich.edu/A52255.0001.001
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 June 24, 2025.

Pages

The meane motions of Jupiter.

Anno Christi.Longitude ♃Aphelion ♃Node ♃
Years 1500004. 50000185. 54833097. 93889
80269. 044441. 98000. 54722
6182. 13667. 14833. 04111
Iuly17. 62333. 01444. 00389
Dayes 161. 33000. 00104. 00030
Houres 18. 06222  
Parts 4564. 00154  
Mean motion.474. 69820187. 6841498. 53141
Aphelion subt.187. 68414Rests Anomaly287. 01406

The halfe of Jupiter first inequality, or his eccentricity, supposing his Semidiameter to be 100. 000 by the computation of Bullialdus is 4856, and the Semidiameter of the Earths Orbe 19138▪ and therefore to find ♃ Semidiameter, when the Semidiameter of the Earths Orb is 100. 000 the proportion is, As 19138. Is to 100. 000 so is 100. 000 to 522520, the Semidiameter required, which being doubled is the Diameter of the El∣lipsis,

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or the side M E 1045040. And to find the eccentricity in the same parts, say, as 100. 000. is to 522520, so is 4856, to 2537. the excentri∣city, and the double thereof. 50746 is M H the distance of the foces.

The complement of the Anomaly 72. 98594 is the angle A M E, and the halfe compl: 36. 49297, is the halfe sum of the opposite angles M E H and M H E.

The side M E1045040 
The side M H50746 
Sum1095786 co. ar.3. 9602744
Differ9942945. 9975147
Tang. ½ sum36. 492979. 8690974
Tang. ½ differ33. 871629. 8268865
Differ.2. 62135 Angle M E H 

Double differ. 5. 24270 Angle M B H or the Equatiō sought, and to be added to Jupiters mean longitude, the Anomaly being above a Semi-circle.

Jupiters mean longitude
114. 69820
Equation add
5. 24270
Jupiters eccentrick place
119. 94090
The Node subt.
98. 53141
Argument of Latitude.
21. 40949

By help whereof, and the angle of his greatest inclination 1. 36333, or E B 2379, we may find the reduction: but to find the parts of inclination in proportion to the given Radius 522520. say, As 100. 000. is to 2379, so is 522520 to 13619. the parts required.

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