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Hf-W-Thは,火星の急速な成長と惑星の胚としての地位の証拠です

N Dauphas1, A Pourmand

  • 1Origins Laboratory, Department of the Geophysical Sciences and Enrico Fermi Institute, The University of Chicago, 5734 South Ellis Avenue, Chicago, Illinois 60637, USA. dauphas@uchicago.edu

Nature
|May 27, 2011
PubMed
まとめ

火星は急速な増殖を経験し,180万年以内に半分のサイズに達しました. これは,太陽系形成の初期に衝突を回避した惑星の胚として火星の理論を支持する.

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