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History of physical astronomy, from the earliest ages to the middle of the 19th century. Comprehending a detailed account of the establishment of the theory of gravitation by Newton, and its development by his successors; with an exposition of the progress of research on all the other subjects of celestial physics (1852)

Grant, Robert, 1814-1892 · London, R. Baldwin · leaf 613

An illustration from History of physical astronomy, from the earliest ages to the middle of the 19th century. Comprehending a detailed account of the establishment of the theory of gravitation by Newton, and its development by his successors; with an exposition of the progress of research on all the other subjects of celestial physics, 1852, leaf 613
tangential angle vanishes. Now, it has been remarked (7) thatthe fulfilment of this condition is in-dependent of the actual magnitudeof the tangential angle; it will there-fore still hold good in the presentcase, notwithstanding the diminutionof the tangential angle occasioned bythe action of the… … APPENDIX. 589 of mean distance. Hence it follows that in tbe new, as well as in theundisturbed ellipse, the planet is at the mean distance. Let p denote theplace of the planet, p t the tangent of the undisturbed orbit, and p t thetangent of the new^ orbit. Now, since in an ellipse the tangent at…

Astronomy

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