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Updated: Jul 20, 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

小惑星の断片の半大軸の移動性

Farinella1, Vokrouhlick

  • 1Dipartimento di Astronomia, Universita di Trieste, Via Tiepolo 11, I-34131 Trieste, Italy. Institute of Astronomy, Charles University, V Holesovickach 2, CZ-18000 Prague 8, Czech Republic.

Science (New York, N.Y.)
|March 5, 1999
PubMed
まとめ

ヤーコフスキー効果は小惑星の軌道を漂流させ,それらを共鳴経路に移動させます. この微妙な放射線圧力メカニズムは,小惑星を地球に近い宇宙に運ぶために極めて重要です.

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