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Titlebook: Cosmochemistry; Proceedings of the S A. G. W. Cameron Conference proceedings 1973 D. Reidel Publishing Company, Dordrecht, Holland 1973 cos

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發(fā)表于 2025-3-21 18:53:39 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Cosmochemistry
副標題Proceedings of the S
編輯A. G. W. Cameron
視頻videohttp://file.papertrans.cn/239/238910/238910.mp4
叢書名稱Astrophysics and Space Science Library
圖書封面Titlebook: Cosmochemistry; Proceedings of the S A. G. W. Cameron Conference proceedings 1973 D. Reidel Publishing Company, Dordrecht, Holland 1973 cos
描述The International Association of Geochemistry and Cosmochemistry was organized in 1967, and held its first meeting at UNESCO Headquartels that year in association with its symposium on The Origin and Distribution of the Elements‘. The Association is a member of the International Union uf Geological Sciences, and holds regular meetings at the time of the I nternatlOnal Geological Congresses, the last of which was held in Montreal, in August. 1972. The IAGC was organized to coordinate activities on an international scale in a wide variety of branches of geochemistry. Its activities are carried on through Commissions and Working Groups, and by means of symposia and other international activities. It has national, corporate, and individual members. One of the first actions taken by the Council of the [AGC when it met in 1967 was to establish an initial set of Working Groups to commence the activity of the organization. Among these Working Groups was one on Extraterrestrial Chemistry, established under the chairmanship of the writer. This Working Group recognized that its basic concern with the chemical composition of cosmic systems was a problem with ramifications in many fields in add
出版日期Conference proceedings 1973
關鍵詞cosmic ray; moon; observatory; planet; stellar
版次1
doihttps://doi.org/10.1007/978-94-010-2658-1
isbn_softcover978-94-010-2660-4
isbn_ebook978-94-010-2658-1Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1973
The information of publication is updating

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發(fā)表于 2025-3-21 21:36:32 | 只看該作者
https://doi.org/10.1007/978-94-010-2658-1cosmic ray; moon; observatory; planet; stellar
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,Introduction: ‘Trans-Scripts’,rs, (3) non-violent (quasi-static) stellar evolution, (4) supernova explosions, (5) cosmic ray interactions with the interstellar medium and (6) nova explosions to the observed solar system abundances are summarized. Recent studies of ‘explosive nucleosynthesis’ in supernovae and of the production o
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,Introduction: ‘Trans-Scripts’,d solar matter. The composition of solar particles changes with energy and from flare to flare. A strong excess of heavy elements at energies below a few MeV/nuc decreases with energy, and at energies above ~15 MeV/nuc the composition of solar particles resembles that of galactic cosmic rays somewha
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,Introduction: ‘Trans-Scripts’,sses which took place in the primitive solar nebula. Chondrites thus are thought to contain a unique record of the physico-chemical conditions which prevailed at the time and place (asteroid belt) of their origin. Elemental abundance patterns are an important clue to the events and processes. Most e
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發(fā)表于 2025-3-23 06:57:44 | 只看該作者
Simone de Beauvoir on Sexual Differenceof the terrestrial planets and the Moon. An important factor is the variation of pressure and temperature with distance from the Sun, and in the case of the Moon and captured satellites of other planets, with distance from the median plane. Current estimates of the temperature and pressure in the so
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