S Sugita1, T Ootsubo, T Kadono

  • 1Department of Complexity Science and Engineering, University of Tokyo, Kashiwa, Chiba, Japan. sugita@k.u-tokyo.ac.jp

Science (New York, N.Y.)
|September 17, 2005
PubMed
まとめ

彗星の衝突クレーター形成は複雑です. スバルー望遠鏡のデータは,重力が大きな塵の羽根を制御していることを明らかにしますが,揮発性の膨張はまた,内部の塵の羽根を加速しました.

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