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Titlebook: Composition and Origin of Cometary Materials; Proceedings of an IS K. Altwegg,P. Ehrenfreund,W. F. Huebner Conference proceedings 1999 Spri

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书目名称Composition and Origin of Cometary Materials
副标题Proceedings of an IS
编辑K. Altwegg,P. Ehrenfreund,W. F. Huebner
视频video
丛书名称Space Sciences Series of ISSI
图书封面Titlebook: Composition and Origin of Cometary Materials; Proceedings of an IS K. Altwegg,P. Ehrenfreund,W. F. Huebner Conference proceedings 1999 Spri
描述Comet nuclei are the most primitive bodies in the solar system.They have been created far away from the early Sun and their materialproperties have been altered the least since their formation. Thus,the composition and structure of comet nuclei provide the bestinformation about the chemical and thermodynamic conditions in thenebula from which our solar system formed. .In this volume, cometary experts review a broad spectrum of ideas andconclusions based on .in situ. measurement of Comet Halley andremote sensing observations of the recent bright Comets Hale-Bopp andHyakutake. The chemical character of comet nuclei suggests many closesimilarities with the composition of interstellar clouds. It alsosuggests material mixing from the inner solar nebula and challengesthe importance of the accretion shock in the outer nebula. The book isintended to serve as a guide for researchers and graduate studentsworking in the field of planetology and solar system exploration.Several special indexes focus the reader‘s attention to detailedresults and discussions. It concludes with recommendations forlaboratory investigations and for advanced modeling of comets, thesolar nebula, and the collapse of i
出版日期Conference proceedings 1999
关键词Accretion; planet; planetary science; solar system; sun
版次1
doihttps://doi.org/10.1007/978-94-011-4211-3
isbn_softcover978-94-010-5830-8
isbn_ebook978-94-011-4211-3Series ISSN 1385-7525
issn_series 1385-7525
copyrightSpringer Science+Business Media Dordrecht 1999
The information of publication is updating

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Conference proceedings 1999studentsworking in the field of planetology and solar system exploration.Several special indexes focus the reader‘s attention to detailedresults and discussions. It concludes with recommendations forlaboratory investigations and for advanced modeling of comets, thesolar nebula, and the collapse of i
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https://doi.org/10.1007/978-3-663-05582-2it difficult to defend an early influx of icy planetesimals from the Jupiter zone to the early Earth. D/H measurements of OH groups in phyllosilicate rich meteorites suggest a mixture of cometary water and water adsorbed from the nebula by the rocky grains that formed the bulk of the Earth may be re
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