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Updated: Jul 11, 2026

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
09:44

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System

Published on: June 5, 2014

隕石の回転速度の起源は,大災害の影響によるものです

S G Love1, T J Ahrens

  • 1Seismological Laboratory, California Institute of Technology, Pasadena 91125, USA. sglove@gps.caltech.edu

Nature
|March 13, 1997
PubMed
まとめ

小惑星の自転は衝突によって制御され,重力がより大きな小惑星の材料の強さに優勢である. 壊滅的な衝撃は,観測された小惑星の回転パターンと整合して,スピン速度を大幅に変化させます.

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