まとめ
金星の大気中の水は,珍しいプロフィールを呈しています. 調和したデータは,水が二酸化炭素と三酸化硫黄と結合し,大気の下層で炭素酸と硫黄酸を形成することを示唆しています.
科学分野:
- 惑星科学は惑星科学である.
- 大気化学 大気化学
- スペクトロスコーピーは,スペクトロスコーピーを用います.
背景:
- 金星の大気中の垂直の水量プロファイルは,表面の近くで急激に減少する異常な分布を示しています.
- 異なる赤外線帯の間には不一致があり,2.5から10の因数で変動する水の豊富さを示唆しています.
研究 の 目的:
- 金星の大気中の水の豊富性プロファイルに関する矛盾するデータを調和させるため.
- 観測された水蒸気分布を説明する化学モデルを提案する.
主な方法:
- 様々な赤外線帯からの既存の大気データの分析.
- 下層大気中の分子関連を調査するための化学モデリング.
- 水蒸気と硫酸の吸収特性を比較するための光譜分析.
主要な成果:
- データ調整は,水分子が二酸化炭素と三酸化硫黄と結合することを提案することによって達成されます.
- 下層大気中のガス状の炭素酸と硫酸の形成が,異常なプロフィールを説明している.
- 硫酸は,0.94マイクロメートルで水蒸気よりも強い吸収物質として識別され,測定の不一致を解決します.
結論:
- 金星の大気の平均総水量50 +/- 20 ppmは,金星の大気のために導出されています.
- 表面近くの自由水蒸気濃度が10 +/- 4 parts per millionと決定される.
- 提案された化学的関連は,垂直の水の豊富性プロフィールの一貫した説明を提供します.
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