地球の水っぽい始まりの 深いマントルのヒント
1Earth and Planets Laboratory, Carnegie Science, Washington, DC, USA.
まとめ
地下マントルの鉱物には 以前考えられていたよりも 水分がかなり多く含まれているかもしれません この発見は惑星の水貯蔵庫と 地質学的過程の理解に影響を与えます
科学分野:
- 地化学
- 鉱物物理学
- 地震学
背景:
- 地球の深い内部,特に下層マントルは,かなりの量の水の潜在的貯蔵庫です.
- 下層マントルの水貯蔵量に関する以前の推定は,鉱物学的および地質学的データによって制限されています.
研究 の 目的:
- 地下マントルの水分貯蔵能力を再評価する
- 新しい鉱物物理学データと地質学的観測を統合する.
主な方法:
- マントルの鉱物に対する高圧・高温実験
- 鉱物中の水分を測定するスペクトル分析
- 地震波分析で鉱物成分と水分状態を推測する
主要な成果:
- 下層マントルに安定した特定の鉱物は,以前よりも水素の組み込みに対するより高い親和性を示す.
- 改訂されたモデルでは 下層マントルの水分含有量が 表面の海よりも 大きくなることが示唆されています
結論:
- 下層マントルは,マントルのダイナミクスと揮発性サイクルに影響を与える主要な地球規模の水貯蔵庫である可能性があります.
- この発見は,地球の水循環と地球深層のプロセスの役割を再評価することを必要としています.
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