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熱疲労が小惑星のレゴリスの起源である
Marco Delbo1, Guy Libourel2, Justin Wilkerson3
1Laboratoire Lagrange, UNS-CNRS, Observatoire de la Côte d'Azur, Boulevard de l'Observatoire-CS 34229, 06304 Nice Cedex 4, France.
Nature
|April 4, 2014
まとめ
衝突ではなく,熱的疲労が小惑星のレゴリットの主な源である. 温度変化によって引き起こされるこのプロセスは岩石を分解し,近地小惑星の表面を説明する可能性がある.
科学分野:
- 惑星科学 惑星科学
- 小惑星の表面プロセス
- レゴリトのダイナミクス
背景:
- 小型小惑星は,より小さな粒子の層であるレゴリスで覆われています.
- レゴリット生成は,以前は,インパクトエジェクタとマイクロメテオロイドインパクトに起因していた.
研究 の 目的:
- 小惑星のレゴリット生成の主なプロセスを特定するために.
- 小惑星の表面進化における熱疲労の役割を調査する.
主な方法:
- 宇宙ミッションのデータと熱赤外線観測の分析.
- クレーター噴出物に関する実験室の実験と衝撃モデルのレビュー.
- 断片化メカニズムとしての熱疲労の理論モデル化.
主要な成果:
- 衝突噴射速度は小さな小惑星の脱出速度を超えており,小惑星はレゴリットの主な源である可能性は低い.
- 熱的疲労は,日中の温度変動によって引き起こされ,微小隕石の衝突よりも,断片の岩が速くなります.
- 熱的断片化はサイズに関係なく,あらゆるサイズの小惑星のレゴリットに寄与します.
結論:
- 熱疲労は,小惑星のレゴリット生成の主なプロセスです.
- このメカニズムは,近地小惑星の表面を若返らせます.
- 熱的疲労は,地球に近い炭酸性小惑星の稀有性を説明する可能性がある.
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