Titlebook: Measure of the Moon; Proceedings of the S Zdeněk Kopal,Constantine L. Goudas Conference proceedings 1967 D. Reidel Publishing Company 1967

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Investigating the Moon’s Motion by Laser Rangingterminations have been especially interesting because radar measures distance (albeit in light-seconds rather than in meters) more directly than and independently of the classical astronomical triangulation methods. In addition to yielding precise distances, detailed examination of the reflected ene

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Astrophysics and Space Science Libraryhttp://image.papertrans.cn/m/image/628063.jpg

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Cassini’s Second and Third LawsIn 1693 G. D. Cassini published the three following empirical laws on the Moon’s rotational motion:

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The Moon’s Mechanical EllipticityIn a discussion of problems connected with the Moon’s physical libration one cannot fail to pay particular attention to the quantity ., the so-called Moon’s mechanical ellipticity.

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Lunar Physical Libration Theorye Moon, is a very onerous task. The differential equations are complicated, mutually coupled and non-linear. The elaborate numerical treatment of . (1902) furnished solutions which remain authoritative to this day except for the modifications of . (1948) who replaced Hansen’s lunar theory with Brown’s theory.

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Laser Measurement of Earth-Moon Distance and Selenographye then, there has been practically no interruption in observation of the Moon by radar, which has brought us a great deal of important information, including, in particular, a new lunar parallax value (cf. .., 1965).

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