中大學術數位典藏-NCU Institutional Repository:Item 987654321/101756
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    题名: Boulders on asteroid toutatis as observed by chang e-2
    作者: 葉永烜;Jiang, Yun;Ji, Jianghui;Huang, Jiangchuan;Marchi, Simone;Li, Yuan;Ip, Wing-Huen
    贡献者: 理學院天文研究所
    关键词: 639/33/445;704/445/848;Asteroids;Frequency distribution;Geology;Humanities and Social Sciences;Morphology;multidisciplinary;Preservation;Science;Spacecraft;Spatial distribution
    日期: 2015-11-02
    上传时间: 2026-04-21 14:43:11 (UTC+8)
    出版者: Nature Publishing Group;London: Springer Science and Business Media LLC
    摘要: 摘要: AbstractBoulders are ubiquitously found on the surfaces of small rocky bodies in the inner solar system and their spatial and size distributions give insight into the geological evolution and collisional history of the parent bodies. Using images acquired by the Chang’e-2 spacecraft, more than 200 boulders have been identified over the imaged area of the near-Earth asteroid Toutatis. The cumulative boulder size frequency distribution (SFD) shows a steep slope of −4.4 ± 0.1, which is indicative of a high degree of fragmentation. Similar to Itokawa, Toutatis probably has a rubble-pile structure, as most boulders on its surface cannot solely be explained by impact cratering. The significantly steeper slope for Toutatis’ boulder SFD compared to Itokawa may imply a different preservation state or diverse formation scenarios. In addition, the cumulative crater SFD has been used to estimate a surface crater retention age of approximately 1.6 ± 0.3 Gyr.
    其他題名: Sci Rep
    出版者: London: Springer Science and Business Media LLC
    出版日期: 2015-11-02
    出處: Scientific Reports, 2015-11, Vol.5 (1), p.16029-16029, Article 16029
    資源來源: Publicly available content database
    版權: The Author(s) 2015
    版權: Copyright Nature Publishing Group Nov 2015
    版權: Copyright © 2015, Macmillan Publishers Limited 2015 Macmillan Publishers Limited
    識別號: ISSN: 2045-2322
    識別號: EISSN: 2045-2322
    識別號: DOI: 10.1038/srep16029
    識別號: PMID: 26522880
    显示于类别:[天文研究所] 期刊論文

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