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Updated: Jul 20, 2026

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
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小行星碎片的半大轴移动性

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
概括

亚科夫斯基效应导致小行星轨道漂移,将它们移动到共振轨道中. 这种微妙的辐射压力机制对于将小行星送入近地空间至关重要.

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