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Updated: Jul 11, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
バイキング着陸機のカメラによる恐怖症の多色観測:炭酸性コンドリート組成の証拠
まとめ
フォボス (Phobos) とは
科学分野:
- 惑星科学は惑星科学である.
- アストロジオロジー アストロジオロジー
- スペクトル顕微鏡検査です.
背景:
- 火星の衛星であるフォボスには,完全に理解されていない表面組成があります.
- 以前の研究では,フォボスのスペクトルデータが限られている.
研究 の 目的:
- フォボスの反射率を0.4〜1.1マイクロメートルのスペクトル領域で測定する.
- フォボスのスペクトル特性を実験室で採取したサンプルと比較して,その起源を推測する.
主な方法:
- バイキング着陸機のカメラ画像からの反射率データの分析.
- 観測されたスペクトルデータを,炭酸性コンドライトとベースアルトの実験室スペクトルと比較.
主要な成果:
- フォボスは0.4~1.1μmの平らな反射率曲線を示している.
- フォボスの幾何学的なアルベドは0.05 +/- 0.01.01と決定されました.
- 観測されたスペクトルは,塩基岩ではなく,炭酸塩状のコンドライトと一致しています.
結論:
- フォボスのスペクトル特性は,炭酸性コンドライト物質と一致しています.
- この発見により,フォボスは火星の天然衛星ではなく,捕獲された小惑星である可能性が示唆されています.
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