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Updated: Jun 20, 2025

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

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超中心の逆行軌道にある 熱い木星の祖先

Arvind F Gupta1,2,3, Sarah C Millholland4,5, Haedam Im4,5

  • 1U.S. National Science Foundation National Optical-Infrared Astronomy Research Laboratory (NSF NOIRLab), Tucson, AZ, USA. arvind.gupta@noirlab.edu.

Nature
|July 17, 2024
PubMed
まとめ

巨大な系外惑星や ホット・ジュピターは 内側へ移動するようです この研究では,高質量で偏心的な系外惑星が発見され,熱い木星の形成のための高偏心性の潮移動経路を支えている.

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