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 5, 2024.

Pages

Probleme 1.

Three points in the circumference of a circle being given, to find a dia∣meter▪ upon which there being perpendiculars let fall from the points given; the segments of the diameter intercepted by these perpendiculars shall be proportional to another proportion given.

In the circle B C D whose center is A, let the points given be B, C, D, and let it be required to find the diameter of that circle upon which per∣pendiculars

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being let fall fall from the points B, C, D, the segments of the Diameter shall be proportional to another proportion given: let the pro∣portion of the segments intercepted by the perpendiculars let fall from B and C be required to be as S to R.

Let the line C B be cut in E, so as C B may be to E B, as S to R, and let D E, cut the Diameter F G at right angles in H. Then is F G the Diameter sought, upon which seeing the lines B I, C K, D H doe fall perpendicularly, K I shall be to H I as S to R.

For the right lines C B are parallel, or not parallel, if they be parallel, C B shall be equal to K I, and E B to H I, and then by construction K I shall be H I, that is C B to E B, in the given proportion as S to R. But if they can meet, let the point of their meeting be at L. Then it shall be as L C to L K, so L E to L H, and so is L B to L I. And then dividing and changing the termes, it shall be as K I to H I, so is C B to E B, or so is S to R as was required.

And thus likewise K H and H I, with the arches B C, C D, and B D, being given, we may find the arch B G, and the Diameter F G in the same parts with K H and H I, for the arches C D and D B being given, the subtenses of those arches and angles opposite to them in the triangle B C D shall be given also in the parts of the Diameter F G, and there∣fore the sides E B and D B with the angle E B D being given, the angle E D B or D B M shall be given also, which being deducted from the arch B M D shall leave B M or the double of B G.

[illustration]

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