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Updated: Jul 12, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
まとめ
マリナー10号は,客観的な格子スペクトロメーターを使用して,金星の上層大気中の水素,ヘリウム,炭素,酸素を検出しました. 予備的な分析によると,金星は400Kのエクソスフィアの温度を示している.
科学分野:
- 惑星科学 惑星科学
- 大気科学 大気科学
- スペクトル顕微鏡検査です.
背景:
- 惑星の大気の組成を理解することは,惑星の進化を理解するために不可欠です.
- 金星の上層大気に関する以前の研究は,範囲と波長の範囲が限られていた.
研究 の 目的:
- 紫外線の範囲で金星の空気の輝きを測定するために.
- 金星の上層大気の組成を決定する.
- 金星のエクソスフィアの温度を調査する.
主な方法:
- マリナー10号の宇宙船に搭載されたオブジェクト格子スペクトロメーターを利用した.
- アングストーム200〜1700の波長範囲でエアグローデータを収集しました.
主要な成果:
- 金星の上層大気中の水素,ヘリウム,炭素,酸素原子の大量の濃度が検出されました.
- 予備的な水素データは,外気圏の温度が400Kであることを示した.
- 1350アングストームの長方に向かって観測された強烈な空気光放射は,空間的に広範囲で,昼と夜の両面に存在しています.
結論:
- 金星の上層大気には,かなりの量の主要な元素が含まれています.
- 金星のエクソスフィアの気温は約400Kと推定されています.
- 強烈な空気光放射の性質については,さらなる調査が必要である.
関連する概念動画
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The UV–Vis spectrum of a molecule is the plot of its absorbance versus wavelength. The plot is drawn by taking molar absorptivity (ε) or log ε on the y-axis (ordinate)...
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