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 4, 2024.

Pages

Precept 1.

The Declination of the Sun or other Planet is found by the signe in the head or foot, and the degree on the right side, if the signe be in the foot, or on the left side if it be in the head: for the common angle gives the Decli∣nation sought, if you have respect, to your Planets proper latitude, and the proper part proportional.

For Example: Suppose the Moon were in 19 degrees 56 parts of Leo, and her declination were required, having North latitude 3 degrees. Her Declination in that latitude, in 19 degrees of Leo will be found 18. 02

In 20 degrees it is 17. 70
There difference is 0. 32
Now then if one degree give0. 321. 5051499▪
What shall0. 561. 7481880
They give 18 ferè 1. 2533379

Which being subtracted from 18. 02 because the Declination doth de∣crease, the Moons Declination will be found to be 17. 84

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