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    請使用永久網址來引用或連結此文件: https://ir.lib.ncu.edu.tw/handle/987654321/101819


    題名: The distribution and source of boulders on asteroid 4179 Toutatis
    作者: 葉永烜;Jiang, Yun;Ji, Jianghui;Huang, Jiangchuan;Marchi, Simone;Li, Yuan;Ip, Wing-Huen
    貢獻者: 理學院天文研究所
    關鍵詞: Asteroids;Astronomical bodies;Boulders;Contributed Papers;Craters;Fragments;Information dissemination;Parents;Planetology
    日期: 2016-01-01
    上傳時間: 2026-04-21 14:46:35 (UTC+8)
    出版者: Cambridge University Press;Cambridge, UK: Cambridge University Press
    摘要: 摘要: Boulders are ubiquitous on the surfaces of asteroids and their spatial and size distributions provide information for the geological evolution and collisional history of parent bodies. We identify more than 200 boulders on near-Earth asteroid 4179 Toutatis based on images obtained by Chang'e-2 flyby. The cumulative boulder size frequency distribution (SFD) gives a power-index of −4.4 ± 0.1, which is clearly steeper than those of boulders on Itokawa and Eros, indicating much high degree of fragmentation. Correlation analyses with craters suggest that most boulders cannot solely be produced as products of cratering, but are probably survived fragments from the parent body of Toutatis, accreted after its breakup. Similar to Itokawa, Toutatis probably has a rubble-pile structure, but owns a different preservation state of boulders.
    其他題名: Proc. IAU
    出版者: Cambridge, UK: Cambridge University Press
    出版日期: 2015-08-01
    出處: Proceedings of the International Astronomical Union, 2015-08, Vol.10 (S318), p.153-155
    資源來源: Alma/SFX Local Collection
    版權: Copyright © International Astronomical Union 2016
    識別號: ISSN: 1743-9213
    識別號: ISSN: 1743-9221
    識別號: EISSN: 1743-9221
    識別號: DOI: 10.1017/S1743921315007280
    顯示於類別:[天文研究所] 期刊論文

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