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Updated: May 13, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
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Published on: November 16, 2013

原惑星円盤の地上の領域にある砂粒からの反射光

William Herbst1, Catrina M Hamilton, Katherine LeDuc

  • 1Astronomy Department, Wesleyan University, Middletown, Connecticut 06459, USA. wherbst@wesleyan.edu

Nature
|March 14, 2008
PubMed
まとめ

恒星間塵粒は,若い恒星系の地上の領域で,ミリメートルの大きさまで急速に成長します. KH 15D二重星系を観測した結果,惑星形成に不可欠なこれらの大きな粒子が明らかになりました.

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