Origin of scattered disk resonant TNOs: Evidence for an ancient excited Kuiper belt of 50 AU radius |
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| Authors: | Patryk Sofia Lykawka Tadashi Mukai |
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| Institution: | Graduate School of Science and Technology, Department of Earth and Planetary System Sciences, Kobe University, 1-1 Rokkodai, Nada-ku, Kobe, 657-8501, Japan |
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| Abstract: | Resonance occupation of trans-neptunian objects (TNOs) in the scattered disk (>48 AU) was investigated by integrating the orbits of 85 observed members for 4 Gyr. Twenty seven TNOs were locked in the 9:4, 16:7, 7:3, 12:5, 5:2, 8:3, 3:1, 4:1, 11:2, and 27:4 resonances. We then explored mechanisms for the origin of the resonant structure in the scattered disk, in particular the long-term 9:4, 5:2, and 8:3 resonant TNOs (median 4 Gyr), by performing large scale simulations involving Neptune scattering and planetary migration over an initially excited planetesimals disk (wide range of eccentricities and inclinations). To explain the formation of Gyr-resident populations in such distant resonances, our results suggest the existence of a primordial planetesimal disk of at least 45-50 AU radius that suffered a dynamical perturbation leading to 0.1-0.3 or greater eccentricities and a range of inclinations up to ∼20° during early stages of the Solar System history, before planetary migration. |
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| Keywords: | Kuiper belt Trans-neptunian objects Resonances orbital Neptune Origin Solar System |
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