Thermal modeling for a parent body of Itokawa

S. Wakita, T. Nakamura, Takeshi Ikeda, H. Yurimoto

Research output: Contribution to journalArticle

14 Citations (Scopus)

Abstract

We modeled the possible parent bodies of Itokawa, which was heated within by the decay energy of 26 Al. Based on mineralogic studies of dust particles derived from Itokawa by the Hayabusa spacecraft, it appeared that they were thermally metamorphosed at a peak temperature of 800 °C, and kept at 700 °C or higher at 7.6 Myr after CAI formation. Our numerical results show that the parent bodies of Itokawa would have been larger than 20 km in radius and accreted at a period between 1.9 and 2.2 Myr after CAI formation, to satisfy mineralogic and isotopic evidence from dust particles.

Original languageEnglish
Pages (from-to)228-236
Number of pages9
JournalMeteoritics and Planetary Science
Volume49
Issue number2
DOIs
Publication statusPublished - Jan 1 2014

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computer assisted instruction
parent body
dust
modeling
spacecraft
radii
decay
energy
temperature
particle

All Science Journal Classification (ASJC) codes

  • Geophysics
  • Space and Planetary Science

Cite this

Thermal modeling for a parent body of Itokawa. / Wakita, S.; Nakamura, T.; Ikeda, Takeshi; Yurimoto, H.

In: Meteoritics and Planetary Science, Vol. 49, No. 2, 01.01.2014, p. 228-236.

Research output: Contribution to journalArticle

Wakita, S. ; Nakamura, T. ; Ikeda, Takeshi ; Yurimoto, H. / Thermal modeling for a parent body of Itokawa. In: Meteoritics and Planetary Science. 2014 ; Vol. 49, No. 2. pp. 228-236.
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