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Updated: May 13, 2026

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外惑星の大気中の一酸化炭素と水の吸収線を検出する

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
まとめ

HR 8799系外惑星の直接画像は,その大気の組成と構造を明らかにします. 水と一酸化炭素の線を分析した結果,この若くて巨大な惑星の形成経路が独特であることが示唆されています.

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