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New Trends in Numerical Simulation of the Motion of Small Bodies of the Solar System

โœ Scribed by Tatyana Bordovitsyna; Victor Avdyushev; Alexandr Chernitsov

Book ID
110309794
Publisher
Springer Netherlands
Year
2001
Tongue
English
Weight
310 KB
Volume
80
Category
Article
ISSN
1572-9478

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๐Ÿ“œ SIMILAR VOLUMES

Small bodies of the Solar System
Small bodies of the Solar System
โœ Yeomans, Don ๐Ÿ“‚ Article ๐Ÿ“… 2000 ๐Ÿ› Nature Publishing Group ๐ŸŒ English โš– 548 KB
Migration of small bodies in the solar s
Migration of small bodies in the solar system
โœ S. I. Ipatov ๐Ÿ“‚ Article ๐Ÿ“… 1996 ๐Ÿ› Springer Netherlands ๐ŸŒ English โš– 307 KB

We investigate several parts of the process of migration of small bodies to the Earth from the asteroid and transneptunian belts. The obtained characteristic times up lo collisions of near-Earth objects with the Earth are less than those obtained by other scientists.

Symplectic methods and their application
Symplectic methods and their application to the motion of small bodies in the Solar System
โœ T. -Y. Huang; K. A. Innanen; C. -B. Wang; Z. -Y. Zhao ๐Ÿ“‚ Article ๐Ÿ“… 1996 ๐Ÿ› Springer Netherlands ๐ŸŒ English โš– 324 KB

Symplectic methods have been widely used in Solar System dynamics. This paper discusses both single step and multistep symplectic methods. For single step methods we point out that the modified algorithm (Wisdom et al., 1991et al., , Kinoshita et. al., 1991) ) can be executed in the mass center coor