アステノスフィアのマントルの浸透性と,海洋中部の山脊における溶融抽出率
James A D Connolly1, Max W Schmidt, Giulio Solferino
1Institute for Mineralogy and Petrology, ETH Zurich, 8092 Zurich, Switzerland.
Nature
|November 13, 2009
まとめ
地球 地球 地球 地球 地球 地球
科学分野:
- 地質物理学 地質物理学とは地質物理学です.
- 地質化学 地質化学
- ペトロロジー・ペトロロジーとは
背景:
- 地球の地殻形成に不可欠なマグマの生成は,アステノスフィアの溶融に依存しています.
- 融解輸送は,アステノスフィアのマントルの浸透性に依存しており,現在のモデルではあまり制限されていません.
研究 の 目的:
- オリヴィン集積物の玄武岩溶融の浸透性を実験的に決定する.
- 地球のアステノスフィアの融解輸送時間スケールのモデルを精製する.
主な方法:
- 高圧,高温離心体実験 (400g-700g) で,玄武岩の溶融の流れを測定した.
- 5~12%の多孔性を有するオリヴィン集積物の溶融流の分析.
主要な成果:
- 測定された浸透性は,既存のモデルによって予測されるよりも1〜2倍の大きさです.
- 浸透性は,オリヴィン集積体内の完全に接続された溶融ネットワークを示しています.
結論:
- より高い融解の浸透性は,アステノスフィアの融解の輸送がより速いことを示唆しています.
- 推定された溶融輸送時間 (1-2.5 kyr) は,海中の玄武岩における同位体シグネチャーを説明する.
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