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Updated: May 13, 2026

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在系外行星大气层中检测一氧化碳和水吸收线

Quinn M Konopacky1, Travis S Barman, Bruce A Macintosh

  • 1Dunlap Institute for Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, ON M5S 3H4, Canada. konopacky@di.utoronto.ca

Science (New York, N.Y.)
|March 16, 2013
PubMed
概括

对HR 8799系外行星的直接成像揭示了其大气组成和结构. 对水和一氧化碳线的分析表明,这个年轻而巨大的行星有一个独特的形成路径.

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