通過する太陽系外惑星の大気中の水蒸気
Giovanna Tinetti1, Alfred Vidal-Madjar, Mao-Chang Liang
1European Space Agency, Frascati 00044, Italy. gio@gps.caltech.edu
Nature
|July 13, 2007
まとめ
科学者たちは,熱い木星HD 189733b.の大気中に水蒸気を検出しました. 惑星の通過時に観測されたこの発見は,水の存在を確認しています.
科学分野:
- エクソプラネット科学 エクソプラネット科学
- 大気物理学 大気物理学
- 赤外線天文学の天文学
背景:
- 水は,熱い木星の大気の重要な分子です.
- これらの惑星で水を検出する以前の試みは,不確実な結果をもたらしました.
研究 の 目的:
- 熱い木星HD 189733bの通過中の最近の観測を分析するために.
- 惑星の有効半径の波長依存の変動の原因を調査する.
主な方法:
- 惑星通過中の赤外線 (3.6,5.8,および8μm) と可視光観測の分析.
- 効果半径の変動を吸収シグネチャーとして解釈する.
主要な成果:
- 水蒸気吸収は,赤外線波長で観測された有効半径の変動の最も可能性の高い説明です.
- 可視波長におけるより大きな有効半径は,恒星の変動性や雲/霧によるものかもしれません.
- これまでの水分検出の欠如は,惑星のほぼ同熱の気象プロファイルによって説明される.
結論:
- この研究は,HD 189733b.の大気中に水蒸気が存在するという説得力のある証拠を提供します.
- 大気組成を理解することは,系外惑星の特徴づけに極めて重要です.
- 大気プロフィールは,分子種の検出能力に大きな影響を与えます.
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