Enhanced collisional growth to a protoplanet that has an atmosphere

S. Inaba, M. Ikoma

研究成果: Article査読

102 被引用数 (Scopus)

抄録

Once a protoplanet becomes larger than about lunar size, it accumulates a significant atmosphere that surrounds the solid core. When a planetesimal approaches the protoplanet, it interacts with the atmosphere. If enough energy of the planetesimal is lost by gas drag of the atmosphere, it is captured in the atmosphere even if its original trajectory would not lead to a direct collision with the solid core of the protoplanet. This increases the collision rate, resulting in faster growth of the protoplanet. We have derived the analytical calculations for the collision rate, and calculated the structure of the atmosphere and the trajectories of the planetesimals in the atmosphere. As a result of their large gas drag, small planetesimals are easily captured, resulting in a large rate of collision with the protoplanet. A collision rate of a protoplanet of Earth size with a planetesimal of 100 m radius is, for example, enhanced by a factor of ∼10. These effects play an essential role in the study of formation of solid cores of gas giant planets by the core accretion model.

本文言語English
ページ(範囲)711-723
ページ数13
ジャーナルAstronomy and Astrophysics
410
2
DOI
出版ステータスPublished - 2003 11
外部発表はい

ASJC Scopus subject areas

  • 天文学と天体物理学
  • 宇宙惑星科学

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