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Updated: Apr 29, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
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Published on: November 15, 2013

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宿主星の金属性から推論された,太陽系外惑星半径の3つの体制

Lars A Buchhave1, Martin Bizzarro2, David W Latham3

  • 11] Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138, USA [2] Centre for Star and Planet Formation, Natural History Museum of Denmark, University of Copenhagen, DK-1350 Copenhagen, Denmark.

Nature
|May 30, 2014
PubMed
まとめ

この研究は,宿主星の金属性に基づいて600以上の系外惑星を3つの集団に分類し,岩石,ガス矮星,巨大惑星の形成の異なる経路を明らかにした.

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