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在upsilon Andromedae系统中的行星-行星分散.

Eric B Ford1, Verene Lystad, Frederic A Rasio

  • 1Department of Astronomy, University of California, Berkeley, California 94720, USA.

Nature
|April 15, 2005
PubMed
概括

巨型系外行星可以由于与其他行星的混乱相互作用而发展出高度偏心的轨道. 乌普西隆的安德罗米达星系显示出一个失落的行星造成这些轨道变化的证据,其中一个行星定期返回圆形轨道.

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