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Adhering grains and surface features on two Itokawa particles

Journal Article · · Earth, Planets and Space (Online)
 [1];  [2]
  1. Univ. of New Mexico, Albuquerque, NM (United States)
  2. Washington Univ., St. Louis, MO (United States)
We investigated the surface texture and chemical compositions of two ~40-μm particles returned from the surface regolith of asteroid Itokawa (RB-DQ04-0062 and RB-DQ04-0091) by the Japan Aerospace Exploration Agency’s Hayabusa mission. We identified splash melts, surface blistering, and many small adhering particles. Seven focused ion beam sections were extracted from both Itokawa particles, targeting one splash melt and ten adhering particles to investigate their composition and provenance and the role of micrometeoroid impacts on Itokawa’s surface. Based on the particle’s structure, mineralogy, and interface between the adhering particle and host grain, we identified lithic fragments and particles deposited by impact. These have morphologies and compositions consistent with impact-generated deposits: two have morphologies and compositions that are consistent with impact-generated silica glass, and one was a Ni-free, metallic Fe, and S-rich assemblage that was likely generated by vapor recondensation during a micrometeoroid impact. Here this study shows that, even though its regolith is young, micrometeoroid impacts have altered the regolith of asteroid Itokawa.
Research Organization:
Nevada Field Office, Las Vegas, NV (United States)
Sponsoring Organization:
USDOE Office of Science (SC), Biological and Environmental Research (BER) (SC-23)
OSTI ID:
1376693
Journal Information:
Earth, Planets and Space (Online), Journal Name: Earth, Planets and Space (Online) Journal Issue: 1 Vol. 68; ISSN 1880-5981
Publisher:
SpringerCopyright Statement
Country of Publication:
United States
Language:
English

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Cited By (1)

Special issue “Science of solar system materials examined from Hayabusa and future missions (II)” journal February 2017

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