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Updated: May 21, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
06:04

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Published on: November 16, 2013

オリヴィンを含まないマントルの源はハワイのシールド玄武岩である

Alexander V Sobolev1, Albrecht W Hofmann, Stephan V Sobolev

  • 1Max-Planck-Institut für Chemie, Postfach 3060, 55020 Mainz, Germany. asobolev@mpch-mainz.mpg.de

Nature
|April 1, 2005
PubMed
まとめ

ハワイのマグマは驚くべき起源を示唆している. オリビンに富んだマントルの代わりに,高いニッケルとシリコンの含有量は,リサイクルされた海洋殻から形成されたピロキセニット源を指しています. この改訂された理解は,マントルの融解のモデルに影響を与えます.

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