Yoko Funato1, Junichiro Makino, Piet Hut

  • 1General Systems Studies, University of Tokyo, Komaba, Meguro-ku, Tokyo 153, Japan. funato@chianti.c.u-tokyo.ac.jp

Nature
|February 7, 2004
PubMed
まとめ

新しいメカニズムは,広大でエキセントリックなバイナリ・トランス・ネプチューン天体 (TNOs) を説明する. この形成プロセスは,初期のTNO成長の間に交換反応を伴い,惑星科学の重要なパズルを解く.

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