| 書目名稱 | Chronology and Evolution of Mars | | 副標題 | Proceedings of an IS | | 編輯 | Reinald Kallenbach,Johannes Geiss,William K. Hartm | | 視頻video | http://file.papertrans.cn/227/226480/226480.mp4 | | 叢書名稱 | Space Sciences Series of ISSI | | 圖書封面 |  | | 描述 | Mars is about one-eighth the mass of the Earth and it may provide an analogue of what the Earth was like when it was at such an early stage of accretion. The fur- ther growth of the Earth was sustained by major collisions with planetesimals and planets such as that which resulted in the formation ofthe Earth‘s moon (Hartmann and Davis, 1975; Cameron and Ward, 1976; Wetherill, 1986; Cameron and Benz, 1991). This late accretionary history, which lasted more than 50 Myr in the case of the Earth (Halliday, 2000a, b), appears to have been shorter and less catastrophic in the case of Mars (Harper et ai. , 1995; Lee and Halliday, 1997). In this article we review the basic differences between the bulk composition of Mars and the Earth and the manner in which this plays into our understanding of the timing and mechanisms of accretion and core formation. We highlight some of the evidence for early cessation of major collisional growth on Mars. Finally, we reevaluate the isotopic evidence that Mars differentiated quickly. Fundamental differences between the composition of Mars and that of other terrestrial planets are apparent from the planet‘s slightly lower density and from the compositions | | 出版日期 | Conference proceedings 2001 | | 關(guān)鍵詞 | Accretion; Solar System; atmosphere; solar; space science | | 版次 | 1 | | doi | https://doi.org/10.1007/978-94-017-1035-0 | | isbn_softcover | 978-90-481-5725-9 | | isbn_ebook | 978-94-017-1035-0Series ISSN 1385-7525 | | issn_series | 1385-7525 | | copyright | Springer Science+Business Media Dordrecht 2001 |
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