ヒット・アンド・ラン惑星衝突
Erik Asphaug1, Craig B Agnor, Quentin Williams
1Earth Sciences Department, Institute for Geophysics and Planetary Physics, 1156 High St, University of California, Santa Cruz, California 95064, USA.
Nature
|January 13, 2006
まとめ
陸上の惑星形成の際に発生する巨大衝突は,地球に惑星が形成されるのを引き起こす可能性があります.
科学分野:
- 惑星科学は惑星科学である.
- 天体物理学 天体物理学
- 地質学 地質学 地質学
背景:
- 地球上の惑星の形成は,巨大な衝突で終わったと考えられています.
- 何百もの惑星の胚が衝突し,惑星,月,小惑星が形成されました.
研究 の 目的:
- 単なる合併以上の惑星の衝突の結果を調査する.
- 惑星形成における新しい衝突ダイナミクスの影響を理解する.
主な方法:
- 惑星の胚衝突のシミュレーション.
- 変形と断片化を含む衝突結果の分析.
主要な成果:
- 衝突する惑星は必ずしも合体することはなく,より小さな惑星は逃れることができる.
- 衝突の結果には,変形,スピンアップ,減圧,そして断片化が含まれます.
- ヒット・アンド・ランの衝突は,様々な残骸を生成します.
結論:
- ヒット・アンド・ランの衝突は,惑星形成の重要な要因である.
- これらの衝突残骸は小惑星の形成と隕石の起源に関連しています.
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