メルキュアの表面反射のスペクトル観測は,メッセンジャーの第1回メルキュア・フライバイの際に行われました
William E McClintock1, Noam R Izenberg, Gregory M Holsclaw
1Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO 80303, USA. william.mcclintock@lasp.colorado.edu
まとめ
メルキュール メルキュール メルキュール メルキュール メルキュール
科学分野:
- 惑星科学は惑星科学である.
- スペクトル顕微鏡検査です.
- 地質化学 地質化学
背景:
- MESSENGERミッションは,水星に関する前例のないデータを提供した.
- 表面組成の分析は,惑星の進化を理解するための鍵です.
研究 の 目的:
- 水銀の表面の鉄 (Fe2+) 含有量を測定する.
- 表面の組成とレゴリット成熟の変動を調査する.
主な方法:
- 同時に中紫外線から近赤外線まで反射スペクトル (200-1300 nm) を用いる.
- 吸収特性の分析,特に<280nmと1μm帯.
- 多様な表面材料の高空間解像度スペクトル分析.
主要な成果:
- 平均表面シリケートにおける低鉄酸化物 (Fe2+) 含有量 (<2-3重量%)
- 様々な表面材料に検出可能な1マイクロメートルのFe2+吸収帯がない.
- スペクトルの変動は,組成の違いとレゴライトの成熟度を示しています.
結論:
- 水銀の表面は,全体的に鉄素鉄の含有量が低い.
- 鉄の含有量は,地表と地深の両方において低い可能性が高い.
- 表面の組成と成熟は水星全体で異なっています.
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