P Vernazza1, R P Binzel, C A Thomas

  • 1Research and Scientific Support Department, European Space Agency, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands. pierre.vernazza@esa.int

Nature
|August 16, 2008
PubMed
概括

大多数近地小行星与罕见的LL石石具有相同的光谱特性,这表明它们有着令人惊的起源. 佛罗拉小行星家族可能是主要来源,可能受到Yarkovsky效应对运输的影响.

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