Regolith Migration and Sorting on Asteroid Itokawa

Author:

Miyamoto Hideaki12345,Yano Hajime12345,Scheeres Daniel J.12345,Abe Shinsuke12345,Barnouin-Jha Olivier12345,Cheng Andrew F.12345,Demura Hirohide12345,Gaskell Robert W.12345,Hirata Naru12345,Ishiguro Masateru12345,Michikami Tatsuhiro12345,Nakamura Akiko M.12345,Nakamura Ryosuke12345,Saito Jun12345,Sasaki Sho12345

Affiliation:

1. Department of Museum Collection Utilization Studies, The University Museum, University of Tokyo, Hongo 7-3-1, Bunkyoku, Tokyo 113-0033, Japan.

2. Department of Earth and Planetary Science, University of Tokyo, Hongo 7-3-1, Bunkyoku, Tokyo 113-0033, Japan.

3. Department of Geosystem Engineering, University of Tokyo, Hongo 7-3-1, Bunkyo-ku, Tokyo 113-8656, Japan.

4. Planetary Science Institute, 1700 East Fort Lowell Road, Suite 106, Tucson, AZ 85719, USA.

5. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan.

Abstract

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.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference28 articles.

1. Regolith is loosely defined as any particulate covering an asteroid. We use the terminology of sedimentary deposits (pebble cobble and boulder represent objects whose sizes range from 4 mm to 6.4 cm 6.4 cm to 2.6 m and >2.6 m respectively with “gravel” including all of them) ( 6 ).

2. C. R. Chapman, in Asteroids III, W. F. Bottke Jr., A. Cellino, P. Paolicchi, R. P. Binzel, Eds. (Univ. Arizona Press, Tucson, 2002) pp. 315–330.

3. The Rubble-Pile Asteroid Itokawa as Observed by Hayabusa

4. Touchdown of the Hayabusa Spacecraft at the Muses Sea on Itokawa

5. Grain-size and textural classification of coarse sedimentary particles

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