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E-belt asteroids : ウィキペディア英語版 | E-belt asteroids The E-belt asteroids were the population of a hypothetical extension of the primordial asteroid belt proposed as the source of most of the basin-forming lunar impacts during the Late Heavy Bombardment. == The E-Belt Model ==
The E-belt model was developed by William F. Bottke, David Vokrouhlicky, David Minton, David Nesvorny, Alessandro Morbidelli, Ramon Brasser, Bruce Simonson and Harold F. Levison.〔 It describes the dynamics of an inner band of the early asteroid belt within the framework of the Nice model.
抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)』 ■ウィキペディアで「E-belt asteroids」の詳細全文を読む
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