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Updated: May 3, 2026

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

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乱暴な環恒星円盤における急速な小惑星形成

Anders Johansen1, Jeffrey S Oishi, Mordecai-Mark Mac Low

  • 1Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany. johansen@mpia.de

Nature
|August 31, 2007
PubMed
まとめ

惑星の形成は,星周円盤の中で重力的に効率的に崩壊する岩石によって説明されます. このプロセスは,岩石の接着やガスの引きずりといった課題を克服し,プラネテシマルを急速に形成します.

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