Regolith migration and sorting on asteroid Itokawa

被引:255
|
作者
Miyamoto, Hideaki
Yano, Hajime
Scheeres, Daniel J.
Abe, Shinsuke
Barnouin-Jha, Olivier
Cheng, Andrew F.
Demura, Hirohide
Gaskell, Robert W.
Hirata, Naru
Ishiguro, Masateru
Michikami, Tatsuhiro
Nakamura, Akiko M.
Nakamura, Ryosuke
Saito, Jun
Sasaki, Sho
机构
[1] Univ Tokyo, Univ Museum, Dept Museum Collect Utilizat Studies, Bunkyo Ku, Tokyo 1130033, Japan
[2] Univ Tokyo, Dept Earth & Planetary Sci, Bunkyo Ku, Tokyo 1130033, Japan
[3] Univ Tokyo, Dept Geosyst Engn, Bunkyo Ku, Tokyo 1138656, Japan
[4] Planetary Sci Inst, Tucson, AZ 85719 USA
[5] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Kanagawa 2298510, Japan
[6] Univ Michigan, Dept Aerosp Engn, Ann Arbor, MI 48109 USA
[7] Kobe Univ, Grad Sch Sci & Technol, Nada Ku, Kobe, Hyogo 6578501, Japan
[8] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
[9] Univ Aizu, Dept Comp Software, Aizu Wakamatsu, Fukushima 9658580, Japan
[10] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[11] Seoul Natl Univ, Dept Astron, Seoul 151747, South Korea
[12] Fukushima Natl Coll Technol, Iwaki, Fukushima 9708034, Japan
[13] Natl Inst Adv Ind Sci & Technol, Tsukuba, Ibaraki 3068568, Japan
[14] Tokai Univ, Sch Engn, Kanagawa 2591292, Japan
[15] Natl Astron Observ Japan, Res Selenodesy Project Off, Mizusawa, Oshu 0230861, Japan
关键词
D O I
10.1126/science.1134390
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
High-resolution images of the surface of asteroid Itokawa from the Hayabusa mission reveal it to be covered with unconsolidated millimeter-sized and larger gravels. Locations and morphologic characteristics of this gravel indicate that Itokawa has experienced considerable vibrations, which have triggered global-scale granular processes in its dry, vacuum, microgravity environment. These processes likely include granular convection, landslide-like granular migrations, and particle sorting, resulting in the segregation of the fine gravels into areas of potential lows. Granular processes become major resurfacing processes because of Itokawa's small size, implying that they can occur on other small asteroids should those have regolith.
引用
收藏
页码:1011 / 1014
页数:4
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