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- Shida Koichiro
- Department of Computer Science, Keio University
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- Suzuki Kiyohiro
- Department of Physics, Keio University
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- Kawai Toshio
- Department of Physics, Keio University
書誌事項
- タイトル別名
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- Formation of Sharp Ringlets by Inelasti
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説明
We investigate the possibility that the sharp ringlets observed around giant planets of the solar system are generated through inelastic collisions. First, a model is defined, and then ringlet formation is shown to occur under certain conditions on the rebound coefficients. A three-dimensional case with 2000-body was then simulated. If the condition is satisfied, particles under the gravitational influence of a planet are shown to evolve from a three-dimensional torus to a two-dimensional disc, and finally to one-dimensional ringlets. The form is thus simplified through inelastic collisions. This result is contrary to the common notion that collisions among the constituents of planetary rings would cause the rings to lose their sharp features.
収録刊行物
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- Journal of the Physical Society of Japan
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Journal of the Physical Society of Japan 60 (11), 3953-3966, 1991
一般社団法人 日本物理学会
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詳細情報 詳細情報について
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- CRID
- 1390282679153210624
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- NII論文ID
- 210000096426
- 110001969101
- 130003900991
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- NII書誌ID
- AA00704814
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- BIBCODE
- 1991JPSJ...60.3953S
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- ISSN
- 13474073
- 00319015
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- NDL書誌ID
- 3739756
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- 本文言語コード
- en
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- データソース種別
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- JaLC
- NDL
- Crossref
- CiNii Articles
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- 抄録ライセンスフラグ
- 使用不可