On the Early In Situ Formation of Pluto's Small Satellites
Man Yin Woo, Man Hoi Lee (HKU)

TL;DR
This study uses N-body simulations to test if Pluto's small satellites could have formed from debris ejected during Charon's formation, finding that the current orbital eccentricities are unlikely to result from this scenario.
Contribution
The paper provides a detailed simulation-based analysis of the debris disk formation scenario for Pluto's small satellites, challenging its validity based on orbital eccentricity matching.
Findings
Test particles matching current eccentricities are not in resonances.
Resonance effects do not favor formation near specific mean-motion resonances.
Alternative formation scenarios may be necessary.
Abstract
The formation of Pluto's small satellites - Styx, Nix, Keberos and Hydra - remains a mystery. Their orbits are nearly circular and are near mean-motion resonances and nearly coplanar with Charon's orbit. One scenario suggests that they all formed close to their current locations from a disk of debris that was ejected from the Charon-forming impact before the tidal evolution of Charon. The validity of this scenario is tested by performing -body simulations with the small satellites treated as test particles and Pluto-Charon evolving tidally from an initial orbit at a few Pluto radii with initial eccentricity or 0.2. After tidal evolution, the free eccentricities of the test particles are extracted by applying fast Fourier transformation to the distance between the test particles and the center of mass of the system and compared with the current…
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Taxonomy
TopicsAstro and Planetary Science · Planetary Science and Exploration · Geology and Paleoclimatology Research
