火星のゲールクレーターにおける塩水による粘土鉱物の破壊
T F Bristow1, J P Grotzinger2, E B Rampe3
1Eobiology Branch, NASA Ames Research Center, Moffett Field, CA 94035, USA. thomas.f.bristow@nasa.gov.
まとめ
キュリオシティ・ローバーのデータは 古代の火星の湖床岩に 局所的な塩塩の浸透を示しています この発見は,初期の火星で広範囲にわたるシリケート鉱物不安定化が地質学的および天体生物学的なプロセスに影響を与えたことを示唆している.
科学分野:
- 地質学
- 天体生物学
- 惑星科学
背景:
- 火星の堆積岩は 古代の地質学的・天体生物学的な過程に 洞察力を与えてくれます
- キュリオシティローバーは ゲールクレーターにあるシャープ山を調査し 35億年前の湖床層を調べています
研究 の 目的:
- 時間同等の堆積岩の鉱物学における空間的変化を分析する.
- 古代の火星の岩層の変化における 塩塩の役割を理解するために
主な方法:
- キュリオシティローバーは ベラ・ルービン山脈から グレン・トーリドンまで移動しました
- 400メートル未満の沈殿岩層の鉱物学的分析
主要な成果:
- 鉱物学の重要な空間的差異は,時間相当の岩層で観察されました.
- これらの変異は,シリカが少ない塩塩の局所的浸透に起因する.
結論:
- マグネシウム硫酸の堆積と関連した 局所的に変化した沈殿岩の浸透
- 硫酸塩堆積物の広範囲の分布は,この塩水によるシリケート不安定化は,初期の火星で一般的なプロセスであったことを示唆しています.
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