エクソプラネットの大気. 外惑星の大気の熱構造は,相解像度放出スペクトロスコーピーによるものです

Kevin B Stevenson1, Jean-Michel Désert2, Michael R Line3

  • 1Department of Astronomy and Astrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USA. NASA Sagan Fellow. kbs@uchicago.edu.

Science (New York, N.Y.)
|October 11, 2014
PubMed
まとめ

WASP-43bのような高放射系系外惑星は,昼夜間の極端な温度差を示しています. ハッブル宇宙望遠鏡の観測により,詳細な大気熱構造と,圧力と経度による変動が明らかになりました.

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