Chapter 15 Hill's Approximation in the Three-Body Problem : Part V Physical Processes Relevant to the Planetary Growth : Origin of the Solar System
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概要
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Hill's equation which describes approximately motions of interacting two bodies orbiting around the Sun is summarized, together with its properties. Hill's equation can be separated into equations of the relative and center of mass motions, and the center of mass motion can be integrated analytically. Further, it can be rewritten in a non-dimensional form scaled by the Hill radius and the heliocentric distance. These characteristics of Hill's equation reduce the degrees of freedom of particle motion and, hence, it is advantageous to use it in studies of gravitational scattering and collision between Keplerian particles, which will be described in later chapters.
- 理論物理学刊行会の論文
- 1989-03-10
著者
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Nakazawa Kiyoshi
Department of Cardiology, St. Marianna University School of Medicine
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Ida S
Geophysical Institute University Of Tokyo
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Ida Shigeru
Geophysical Institute University Of Tokyo
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Nakazawa K
Physics Department Gifu University
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井田 茂
東京工業大学・地球惑星科学科
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井田 茂
東京工業大学・理・地球惑星科学
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Nakazawa Kiyoshi
Department Of Applied Physics Tokyo Institute Of Technology
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NAKAZAWA Kiyoshi
Department of Applied Physics, Tokyo Institute of Technology
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Nakazawa Kiyoshi
Gifu University
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