土星の質量を持つ系外惑星WASP-69bに広がったヘリウム大気の地上探知
Lisa Nortmann1,2, Enric Pallé3,2, Michael Salz4
1Instituto de Astrofísica de Canarias, Vía Láctea s/n, 38205 La Laguna, Tenerife, Spain. nortmann.astro@gmail.com.
まとめ
熱いガスの巨大系外惑星は 恒星の放射線によって大気を失います 地上でのヘリウム観測は WASP-69bの外惑星からの大気の脱出を明らかにし,彗星のような尾を示しています.
科学分野:
- 外惑星科学
- 大気物理学
- スペクトロスコーピー
背景:
- 熱いガスの巨大系外惑星は 恒星の放射線の影響で 大気の進化を遂げます
- エクソプラネットの大気逃逸に関する以前の研究は,主に星間吸収によって制限された宇宙ベースの紫外線観測を用いた.
研究 の 目的:
- 地上での高解像度スペクトロスコーピーを用いて エクソプラネットの大気逃亡を調査する.
- 土星質量系外惑星WASP-69bからの大気損失を検知し特徴づけること.
主な方法:
- 外惑星の通過時に1083ナノメートルでヘリウム三重体を観測するために,地上の高解像度スペクトロスコーピーを使った.
- 過剰吸収とラインのブルーシフトを分析した
主要な成果:
- WASP-69bの通過中にヘリウムトリプレート (信号対ノイズ比18) で有意な過剰吸収が検出されました.
- 毎秒数キロの 青い線を測った.
- 通過後の吸収が観測され,大気流出を示す.
結論:
- 観測された現象はWASP-69bからの大気の脱出として解釈された.
- 脱出する大気は 彗星のような尾状の惑星を形成します
- この研究は,外惑星の大気脱出研究における地上ヘリウムスペクトロスコーピーの有効性を示しています.
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