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Titlebook: Mathematical Theory of Stellar Eclipses; Zdeněk Kopal Book 1990 Kluwer Academic Publishers 1990 celestial bodies.earth.moon.photometry.pla

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發(fā)表于 2025-3-21 19:37:39 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Mathematical Theory of Stellar Eclipses
編輯Zdeněk Kopal
視頻videohttp://file.papertrans.cn/627/626655/626655.mp4
圖書封面Titlebook: Mathematical Theory of Stellar Eclipses;  Zdeněk Kopal Book 1990 Kluwer Academic Publishers 1990 celestial bodies.earth.moon.photometry.pla
描述ASTRONOMICAL ECLIPSE PHENOMENA In looking over the long history of human science from time immemorial to our own times, it is impossible to overestimate the role played in it by the phenomena of eclipses of the celestial bodies-both within our solar system as well as in the stellar universe at large. Not later than in the 4th century B. C. , the observed features of the shadow cast on the Moon by the Earth during eclipses led Aristotle (384-322 B. C. ) to formulate the first scientific proof worthy of that name of the spherical shape of the Earth; and only somewhat later, the eclipses of the Sun provided Aristarchos (in the early part of the 3rd century B. C. ) or Hipparchos (2nd half ofthe same century) with the geometric means to ascertain the distance which separates the Earth from the Sun. In the 17th century A. D. (in 1676, to be exact) the timings of the eclipses of the satellites of Jupiter by their central planet enabled Olaf Romer to discover that the velocity with which light propagates through space is finite.
出版日期Book 1990
關(guān)鍵詞celestial bodies; earth; moon; photometry; planet; solar system; star; stellar; sun; universe
版次1
doihttps://doi.org/10.1007/978-94-009-0539-9
isbn_softcover978-94-010-6729-4
isbn_ebook978-94-009-0539-9
copyrightKluwer Academic Publishers 1990
The information of publication is updating

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Light Changes Due to Eclipses of Spherical Stars,uct theoretical models of such phenomena which should serve as a “code” to the language we shall try to decipher; while in Chapters V and VI we shall expose the details of the decoding procedures which can be based upon it.
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Theoretical Photometry of Distorted Eclipsing Systems,ponents, and of their mutual .. A theory of the effects produced by such forces has recently been summarized by the present writer in another volume (cf. Kopal, 1989), to which the reader is referred for fuller details that need not be repeated in this place.
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Inverse Problem for Distorted Eclipsing Systems,r observations accurate to about one part in 1000; this should in general be true as long as their fractional radii . of the components constituting such systems do not exceed (approximately) 0.15 in numerical value.
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Introduction, phenomena of eclipses of the celestial bodies—both within our solar system as well as in the stellar universe at large. Not later than in the 4th century B.C., the observed features of the shadow cast on the Moon by the Earth during eclipses led Aristotle (384–322 B.C.) to formulate the first scien
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