AMD-stability and the classification of planetary systems
作者： J. Laskar , A. C. Petit
DOI: 10.1051/0004-6361/201630022
关键词:
摘要: We present here in full detail the evolution of angular momentum deficit (AMD) during collisions as it was described (Laskar, PRL,2000). Since then, AMD has been revealed to be a key parameter for understanding outcome planetary formation models. define AMD-stability criterion that can easily verified on newly discovered system. show how used establish classification multiplanet systems order exhibit are long-term stable because they AMD-stable, and those AMD-unstable which then require some additional dynamical studies conclude their stability. The is applied 131 from Extrasolar Planet Encyclopaedia database (this http URL) orbital elements sufficiently well known.
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