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pro vyhledávání: '"Hayashi, Nanae"'
Can the orbital distribution of Neptune's 3:2 mean motion resonance result from stability sculpting?
Autor:
Balaji, Sricharan, Zaveri, Nihaal, Hayashi, Nanae, Ruiz, Arcelia Hermosillo, Barnes, Jackson, Murray-Clay, Ruth, Volk, Kathryn, Gerhardt, Jake, Syed, Zain
We explore a simplified model of the outcome of an early outer Solar System gravitational upheaval during which objects were captured into Neptune's 3:2 mean motion resonance via scattering rather than smooth planetary migration. We use N-body simula
Externí odkaz:
http://arxiv.org/abs/2307.06280
