Could Jupiter or Saturn Have Ejected a Fifth Giant Planet?
Ryan Cloutier, Daniel Tamayo, and Diana Valencia

TL;DR
This study assesses the likelihood that Jupiter or Saturn ejected a fifth ice giant planet by analyzing the orbital perturbations on their satellites, finding a plausible ejection scenario for Jupiter but not for Saturn.
Contribution
It introduces a method to constrain giant planet ejection events based on the current orbits of their regular satellites, providing quantitative likelihood estimates.
Findings
Approximately 42% likelihood for Jupiter's ejection scenario to match Callisto's orbit.
Only about 1% likelihood for Saturn's ejection scenario to match Iapetus's orbit.
Uncertainties in Iapetus's formation complicate the interpretation of Saturn's ejection likelihood.
Abstract
Models of the dynamical evolution of the early solar system following the dispersal of the gaseous protoplanetary disk have been widely successful in reconstructing the current orbital configuration of the giant planets. Statistically, some of the most successful dynamical evolution simulations have initially included a hypothetical fifth giant planet, of ice giant mass, which gets ejected by a gas giant during the early solar system's proposed instability phase. We investigate the likelihood of an ice giant ejection event by either Jupiter or Saturn through constraints imposed by the current orbits of their wide-separation regular satellites Callisto and Iapetus respectively. We show that planetary encounters that are sufficient to eject an ice giant, often provide excessive perturbations to the orbits of Callisto and Iapetus making it difficult to reconcile a planet ejection event…
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