The Gas Drag Effect on the Elliptic Motion of a Solid Body in the Primordial Solar Nebula
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概要
- 論文の詳細を見る
The gas drag effect in the primordial solar nebula on the motion of a solid body, ranging from a large planetesimal to a small dust grain, is investigated. For a planetesimal, expressions for the short-term variation of the semi-major axis, the eccentricity and inclination are obtained using a perturbation method and a realistic formula for the gas drag force. For a small body, an orbit spiralling towards the sun in the equatorial plane of the nebula is investigated and the decay time of the orbital radius is obtained. It is found that the decay time at 1 a.u. is as short as 10^2 or 10^3 years for a solid body with mass in the range between 10^3 g and 10^8 g.
- 理論物理学刊行会の論文
- 1976-12-25
著者
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HAYASHI Chushiro
Department of Physics, Kyoto University
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ADACHI Isao
Department of Hospital Pharmacy, Toyama Medical and Pharmaceutical University
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Hayashi Chushiro
Department Of Nuclear Science Kyoto University
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Nakazawa Masami
Department Of Physics Kyoto University
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Adachi Isao
Department Of Hospital Pharmacy Toyama Medical And Pharmaceutical University
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Adachi Isao
Department Of Physics Kyoto University
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Nakazawa Kiyoshi
Department Of Applied Physics Tokyo Institute Of Technology
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NAKAZAWA Masami
Department of Physics, Kyoto University
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ADACHI Isao
Department of Physics, Kyoto University
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ADACHI Isao
Department of Applied Mathematics Osaka University
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HAYASHI Chushiro
Department of Nuclear Science : Research Institute for Fundamental Physics Kyoto University : National Aeronautics and Space Administration
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