Chapter 23 Gas Capture by Proto-Jupiter and Proto-Saturn : Part VI Growth of the Planets : Origin of the Solar System

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概要

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• The interaction of proto-giant-planets and the solar nebula in the stage after the occurrence of Mizuno's instability of the proto-giant-planets is reviewed. When the mass of proto-Jupiter reaches the present Jovian value by accreting the gases of the solar nebula, proto-Jupiter begins to push the gases away from its orbit and form a gap around the orbit. It is considered that this process determined the present Jovian mass. On the other hand, Saturn would have stopped growing owing to the dissipation of the nebular gas.

• 理論物理学刊行会の論文
• 1989-03-10

著者

• SEKIYA Minoru

  Department of Applied Physics, Tokyo Institute of Technology

• Miyama Shoken

  Department Of Physics Kyoto Unvi

• Miyama Shoken

  Department Of Physics Kyoto Univeristy

• Hayashi Chushiro

  Kyoto University

• Sekiya Minoru

  Department Of Earth And Planetary Sciences Faculty Of Sciences 33 Kyushu University

• Sekiya Minoru

  Department Of Applied Physics Tokyo Institute Of Technology

• Shoken M.

  National Astronomical Observatory

• SEKIYA Makoto

  Department of Physics, Kyoto University

• SEKIYA Minoru

  Department of Physics, Kyoto University

• SEKIYA Minoru

  Department of Earth and Planetary Sciences, Faculty of Sciences 33, Kyushu University

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