The Neptune Trojans - a new source for the Centaurs?
J. Horner, P. S. Lykawka

TL;DR
This paper proposes that Neptune Trojans could be a significant, previously underappreciated source of Centaurs, based on dynamical simulations showing their instability and potential to evolve onto Centaur-like orbits.
Contribution
It introduces the idea that Neptune Trojans are a major source of Centaurs, supported by dynamical simulations and flux estimates, expanding understanding of Centaur origins.
Findings
Neptune Trojans are dynamically unstable on Myr and Gyr timescales.
Objects leaving Neptune Trojans can evolve into Centaur-like orbits.
Trojans may contribute a significant, possibly dominant, proportion of the Centaur population.
Abstract
The fact that the Centaurs are the primary source of the Short Period Comets is well established. However, the origin of the Centaurs themselves is still under some debate, with a variety of different source reservoirs being proposed in the last decade. In this work, we suggest that the Neptune Trojans (together with the Jovian Trojans) could represent an additional significant source of Centaurs. Using dynamical simulations of the first Neptune Trojan discovered (2001 QR322), together with integrations following the evolution of clouds of theoretical Neptune Trojans obtained during simulations of planetary migration, we show that the Neptune Trojan population contains a great number of objects which are unstable on both Myr and Gyr timescales. Using individual examples, we show how objects that leave the Neptunian Trojan cloud evolve onto orbits indistinguishable from those of the…
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