David C Rubie1, Christine K Gessmann, Daniel J Frost

  • 1Bayerisches Geoinstitut, University of Bayreuth, D-95444 Bayreuth, Germany. dave.rubie@uni-bayreuth.de

Nature
|May 7, 2004
PubMed
まとめ

地球と火星の核形成は,液体鉄の温度に依存する酸素溶解性により異なっていた. 地球の温度が高くなると,より多くの酸化鉄 (FeO) が抽出され,火星はより豊かなマントルを残した.

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