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
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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 May 19, 2025.
Pages
Example.
Let the time given be May the 12th. houre 11 parts 15 before noon at London in the Bissextile yeare 1656, and the Suns place to be soughts The numbers are thus,
Suns Longitude
Suns Apogeon
Deg.
parts
Deg.
parts
The Epocha
1640
291.
24777
96.
22265
Years comp.
15
359.
37294
23686
April
118.
27760
519
Dayes
12
011.
82776
52
Houres
23
94458
Scruples
15
616
Suns Mean Longitude
421.
87681
96.
46522
2 Subtract the Apogaeum from the Mean Longitude, there rests the mean Anomaly.
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