Space environment of an asteroid preserved on micrograins returned by the Hayabusa spacecraft

Eizo Nakamura, Akio Makishima, Takuya Moriguti, Katsura Kobayashi, Ryoji Tanaka, Tak Kunihiro, Tatsuki Tsujimori, Chie Sakaguchi, Hiroshi Kitagawa, Tsutomu Ota, Yusuke Yachi, Toru Yada, Masanao Abe, Akio Fujimura, Munetaka Ueno, Toshifumi Mukai, Makoto Yoshikawa, Jun'ichiro Kawaguchi

    Research output: Contribution to journalArticlepeer-review

    68 Citations (Scopus)

    Abstract

    Records of micrometeorite collisions at down to submicron scales were discovered on dust grains recovered from near-Earth asteroid 25143 (Itokawa). Because the grains were sampled from very near the surface of the asteroid, by the Hayabusa spacecraft, their surfaces reflect the low-gravity space environment influencing the physical nature of the asteroid exterior. The space environment was examined by description of grain surfaces and asteroidal scenes were reconstructed. Chemical and O isotope compositions of five lithic grains, with diameters near 50 μm, indicate that the uppermost layer of the rubble-pile-textured Itokawa is largely composed of equilibrated LL-ordinary-chondrite-like material with superimposed effects of collisions. The surfaces of the grains are dominated by fractures, and the fracture planes contain not only sub-μm-sized craters but also a large number of sub-μm- to several- μm-sized adhered particles, some of the latter composed of glass. The size distribution and chemical compositions of the adhered particles, together with the occurrences of the sub-μm-sized craters, suggest formation by hypervelocity collisions of micrometeorites at down to nm scales, a process expected in the physically hostile environment at an asteroid's surface. We describe impact-related phenomena, ranging in scale from 10 -9 to 10 4 meters, demonstrating the central role played by impact processes in the long-term evolution of planetary bodies. Impact appears to be an important process shaping the exteriors of not only large planetary bodies, such as the moon, but also low-gravity bodies such as asteroids.

    Original languageEnglish
    Pages (from-to)E624-E629
    JournalProceedings of the National Academy of Sciences of the United States of America
    Volume109
    Issue number11
    DOIs
    Publication statusPublished - Mar 13 2012

    Keywords

    • Comprehensive analysis
    • Impacts
    • Interplanetary dust
    • Sample-return mission
    • Space weathering

    ASJC Scopus subject areas

    • General

    Fingerprint

    Dive into the research topics of 'Space environment of an asteroid preserved on micrograins returned by the Hayabusa spacecraft'. Together they form a unique fingerprint.

    Cite this