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Updated: May 9, 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

メインベルトの小惑星の崩壊によるミオセンの終わりの塵のシャワー

Kenneth A Farley1, David Vokrouhlický, William F Bottke

  • 1Division of Geological and Planetary Sciences, California Institute of Technology, MS 170-25, Pasadena, California 91125, USA. farley@gps.caltech.edu

Nature
|January 20, 2006
PubMed
まとめ

8300万年前の大きな小惑星の衝突により,地球に到達する惑星間塵粒子が著しく増加しました. 海底ヘリウム-3 (3He) の記録は,この出来事を明らかにし,ベリタス族の断片からのIDP流の4倍の増加を示しています.

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