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
Department of Museum Collection Utilization Studies, University Museum, University of Tokyo, Hongo 7-3-1, Bunkyoku, Tokyo 113-0033, Japan.
Science. 2007 May 18;316(5827):1011-4. doi: 10.1126/science.1134390. Epub 2007 Apr 19.
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.
隼鸟号任务获取的糸川小行星表面的高分辨率图像显示,其表面覆盖着未固结的毫米级及更大尺寸的砾石。这些砾石的位置和形态特征表明,糸川小行星经历了相当大的震动,这些震动在其干燥、真空、微重力环境中引发了全球规模的颗粒过程。这些过程可能包括颗粒对流、类似滑坡的颗粒迁移和颗粒分选,导致细砾石分离到潜在的低洼区域。由于糸川小行星体积小,颗粒过程成为主要的表面重塑过程,这意味着如果其他小行星有风化层,这些过程也可能发生在它们身上。