| 書(shū)目名稱(chēng) | Composition and Origin of Cometary Materials |
| 副標(biāo)題 | Proceedings of an IS |
| 編輯 | K. Altwegg,P. Ehrenfreund,W. F. Huebner |
| 視頻video | http://file.papertrans.cn/232/231845/231845.mp4 |
| 叢書(shū)名稱(chēng) | Space Sciences Series of ISSI |
| 圖書(shū)封面 |  |
| 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 |
| 關(guān)鍵詞 | Accretion; planet; planetary science; solar system; sun |
| 版次 | 1 |
| doi | https://doi.org/10.1007/978-94-011-4211-3 |
| isbn_softcover | 978-94-010-5830-8 |
| isbn_ebook | 978-94-011-4211-3Series ISSN 1385-7525 |
| issn_series | 1385-7525 |
| copyright | Springer Science+Business Media Dordrecht 1999 |
|Archiver|手機(jī)版|小黑屋|
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