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 ...

About this Item

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.
Rights/Permissions

To the extent possible under law, the Text Creation Partnership has waived all copyright and related or neighboring rights to this keyboarded and encoded edition of the work described above, according to the terms of the CC0 1.0 Public Domain Dedication (http://creativecommons.org/publicdomain/zero/1.0/). This waiver does not extend to any page images or other supplementary files associated with this work, which may be protected by copyright or other license restrictions. Please go to http://www.textcreationpartnership.org/ for more information.

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 23, 2024.

Pages

CHAP. 9. Having the Declination and Right ascension of a star given, to finde the longitude and latitude thereof.

IN the Diagram of the 3 Chapter, having the Right ascension of the little Star in the breast of Pegasus A C. 337. 49239. And the decli∣nation C M. 22. 43333. with the greatest obliquity of the Ecliptique

B A C. 23. 5250. we are to enquire its Longitude A N. and Lati∣tude M N. wherefore in the Triangle A B C. we have the angle B A C. 23. 5250. and the side A C 22. 50761 the complement of the Right ascen∣sion: then I say.

As Radius.  
To Tangent of B A C23. 52509▪63••••198
So sine of A C.22. 507619. 8••••787
To Tangent of B C.6. 461259. 2217985
Adde C M.22. 43333 The Declination 
Sum is M B.31. 89458 
when the Declination is South the arch found must be subtracted from it, and their difference shall be M B.

2. To finde the angle A B C.
As the sine of B C9. 46125 co. ar.0. 7841497
To the sine B A C23. 52509. 6011352
So the sine of A C22. 507619. 5829787
To the sine of A B C68. 368439. 9682836
3. To finde the side A B.
As the sine of B A C.23. 52520. co. ar.0. 3988648
To the sine of B C.9. 46125.9. 2158503
So is Radius. 10. 0000000
To the sine of A B.24. 319679. 6147151
4. The angle A B C is equall to the angle M B N, therefore to finde the latitude M N.

Page 20

As the sine M N B90. 
To the sine of M B31. 89458.9. 722928
So the sine of M B N.68. 36843.9. 9682836
To the sine of M N.29. 41602.9. 6912118
Lastly, to finde the arch B N.
As Radins.  
To Cotangent of. M B N.68. 36843.9. 5983151
So Tangent of M N.29. 41602.9. 7511554
To the sine of B N.12. 92052.9. 3494705

Which is to be added to A B if the Right ascension be lesse then a semi∣circle, but if the Right ascension exceed 180, as in our example, the Com∣plement of B N. 357▪07948, is the longitude desired.

Do you have questions about this content? Need to report a problem? Please contact us.