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LECTURES ON HILL'S LUNAR THEORY

Published online by Cambridge University Press:  05 June 2011

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Summary

Introduction.

An account of Hill's Lunar Theory can best be prefaced by a few quotations from Hill's original papers. These will indicate the peculiarities which mark off his treatment from that of earlier writers and also, to some extent, the reasons for the changes he introduced. Referring to the well-known expressions which give, for undisturbed elliptic motion, the rectangular coordinates as explicit functions of the time—expressions involving nothing more complicated than Bessel's functions of integral order—Hill writes:

“Here the law of series is manifest, and the approximation can easily be carried as far as we wish. But the longitude and latitude, variables employed by nearly all lunar theorists, are far from having such simple expressions; in fact their coefficients cannot be finitely expressed in terms of Besselian functions. And if this is true in the elliptic theory how much more likely is a similar thing to be true when the complexity of the problem is increased by the consideration of disturbing forces?…There is also another advantage in employing coordinates of the former kind (rectangular): the differential equations are expressed in purely algebraic functions, while with the latter (polar) circular functions immediately present themselves.”

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Chapter
Information
The Scientific Papers of Sir George Darwin
Supplementary Volume
, pp. 16 - 58
Publisher: Cambridge University Press
Print publication year: 2009
First published in: 1916

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