Interstellar object 'Oumuamua as an extinct fragment of an ejected cometary planetesimal
Sean N. Raymond, Philip J. Armitage, and Dimitri Veras

TL;DR
This paper proposes that 'Oumuamua is an extinct fragment of a comet-like planetesimal ejected from its planetary system, explaining its unusual properties through dynamical simulations of tidal disruption and volatile loss.
Contribution
It introduces a new model where 'Oumuamua is a tidally disrupted fragment from a planetesimal, supported by dynamical simulations of ejection and disruption processes.
Findings
0.1-1% of cometary planetesimals undergo disruptive encounters before ejection
Fragments lose surface volatiles and become extinct after multiple close passages
Planetesimal fragments dominate interstellar objects by number, not mass
Abstract
'Oumuamua was discovered passing through our Solar System on a hyperbolic orbit. It presents an apparent contradiction, with colors similar to those of volatile-rich Solar System bodies but with no visible outgassing or activity during its close approach to the Sun. Here we show that this contradiction can be explained by the dynamics of planetesimal ejection by giant planets. We propose that 'Oumuamua is an extinct fragment of a comet-like planetesimal born in a planet-forming disk that also formed Neptune- to Jupiter-mass giant planets. On its pathway to ejection 'Oumuamua's parent body underwent a close encounter with a giant planet and was tidally disrupted into small pieces, similar to comet Shoemaker-Levy 9's disruption after passing close to Jupiter. We use dynamical simulations to show that 0.1-1% of cometary planetesimals undergo disruptive encounters prior to ejection. Rocky…
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