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小行星 (54509) 2000 PH5的旋转速度因YORP效应而增加

Patrick A Taylor1, Jean-Luc Margot, David Vokrouhlicky

  • 1Department of Astronomy, Cornell University, Ithaca, NY 14853-6801, USA. ptaylor@astro.cornell.edu

Science (New York, N.Y.)
|March 10, 2007
PubMed
概括

由阳光引起的Yarkovsky-O'Keefe-Radzievskii-Paddack (YORP) 效应,是导致近地小行星2000 PH5.5的旋转速度增加的原因. 这一发现支持YORP效应.

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