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ケプラー36:近隣の軌道と異なった密度を持つ惑星のペア

Joshua A Carter1, Eric Agol, William J Chaplin

  • 1Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA. jacarter@cfa.harvard.edu

Science (New York, N.Y.)
|June 23, 2012
PubMed
まとめ

天文学者は,非常に異なる密度を持つ2つの系外惑星を発見し,密接に一緒に軌道を回し,私たちの太陽系で観察された典型的な惑星の形成と軌道パターンを挑戦しました. この発見は,惑星系がこれまで理解していたよりも大きな多様性を表す可能性があることを示唆しています.

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