Interaction of energetic particles and dust grains with asteroidal surfaces
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- Goswami J. N.
- Physical Research Laboratory
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Low energy solar wind (SW) and solar energetic particles (SEP) interact with material exposed on the surface of planetary objects devoid of an atmosphere and a global magnetic field such as the Moon and the asteroids. Micrometeoroid impacts will produce microcraters on samples exposed on the surfaces of these bodies and also cause microscale erosion and at times catastrophic rupture of the target rocks and soil grains. The impacting flux of meteoroids thus controls the effective SW and SEP exposure durations of samples on the lunar and asteroidal surfaces. The lunar samples contain abundant records of energetic particle interactions and micrometeoroid impacts while such records found in gas-rich meteorites can be considered to be representative of asteroidal samples. These records allow us to infer the composition and intensity of SW and SEP in the past as well as surface dynamical processes operating on the Moon and asteroids at different epochs. However, unlike the lunar records that span the time interval from the present to several billion years in the past, the asteroidal (gas-rich meteorite) records provide information only for some distant epochs in the past. We do not have much information about the contemporary energetic particle and dust grain environment in the asteroidal region. The Muses-C mission, that will bring back near surface samples from an asteroid, will be extremely important in this regard.
収録刊行物
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- Earth, Planets and Space
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Earth, Planets and Space 53 (11), 1029-1037, 2001
地球電磁気・地球惑星圏学会 、公益社団法人 日本地震学会、特定非営利活動法人 日本火山学会、日本測地学会、日本惑星科学会
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詳細情報 詳細情報について
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- CRID
- 1390001206512460160
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- NII論文ID
- 10007641219
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- NII書誌ID
- AA11211921
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- COI
- 1:CAS:528:DC%2BD38XisFGjsg%3D%3D
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- ISSN
- 18805981
- 13438832
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- NDL書誌ID
- 5995268
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- 本文言語コード
- en
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- データソース種別
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- JaLC
- NDL
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