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Titlebook: An Introduction to the Study of the Moon; Zdeněk Kopal Book 1966 Springer Science+Business Media Dordrecht 1966 moon

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发表于 2025-3-21 19:34:28 | 显示全部楼层 |阅读模式
期刊全称An Introduction to the Study of the Moon
影响因子2023Zdeněk Kopal
视频video
学科分类Astrophysics and Space Science Library
图书封面Titlebook: An Introduction to the Study of the Moon;  Zdeněk Kopal Book 1966 Springer Science+Business Media Dordrecht 1966 moon
影响因子After several decades spent in astronomical semi-obscurity, the Moon has of late suddenly emerged as an object of considerable interest to students of astronomy as well as of other branches of natural science and technology; and the reasons for this are indeed of historical significance. For the Moon has now been destined to be the first celestial body outside the confines of our own planet to be reconnoitered at a close range by means of spacecraft built and sent out by human hand for this purpose. At the time of writing, not less than ten such spacecraft of American as well as Rus­ sian origin landed already on different parts of the lunar surface; and some of these provided remarkable records of its detail structure to a spatial resolution increased thousandfold over that attained so far from our ground-based facilities. A renewed interest in our satellite, stemming from this source, on the part of the students of many branches of science and technology has also underlined the need for presenting the gist of our present knowledge in this field in the form that could serve as an introduction to the study of the Moon not only for astronomers, but also for serious students from oth
Pindex Book 1966
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发表于 2025-3-22 00:06:37 | 显示全部楼层
Rotation of the Moon; Optical Librationsized in the earliest days of lunar observations from the fact that the Moon exhibit to us on Earth (almost) always the same face, it must also rotate with a uniform angular velocity about an axis fixed in space and inclined but little to its orbital plane.
发表于 2025-3-22 03:13:54 | 显示全部楼层
Photometric Consequences of the Moon’s Motion: Phases and Eclipsesy. This motion affects, of course, vitally most observational manifestations of our satellite; and the most elementary aspect of these are the conditions of illumination of the Moon by the Sun and the Earth — i.e., the . of the Moon — which we shall now proceed to describe.
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Stress History of the Moontude as that of the Moon; and of the way in which this heat is likely to be distributed in the course of time. The time-dependence of the sources of radiogenic heat, together with the gradual cooling of lunar globe by escape of its thermal radiation into space, is bound to render the distribution of
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Possible Convection in Lunar Interiorastic solid. The physical reason why the Moon should behave so at least in the outer parts of its interior are indeed overwhelming; but is this necessarily the case also in the deep interior of our satellite? The relatively high temperatures which we have reasons to expect there as a result of radio
发表于 2025-3-23 03:45:26 | 显示全部楼层
Chemical Composition of the Moonmical composition of the lunar globe — a difficult subject to approach with any confidence at a distance, when most of its discussion has to rest on indirect arguments. Yet such arguments should enable us already at this stage to draw certain probable conclusions which should facilitate our discussi
发表于 2025-3-23 06:21:04 | 显示全部楼层
Exosphere of the Moonition of its globe as discussed in the preceding chapter, entail several further important consequences; and perhaps the most important one for an understanding of lunar surface features is the well-nigh complete ., which would protect this surface from a direct contact with the outer space.
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