Reassessing the origin of Triton
E. Nogueira, R. Brasser, R. Gomes

TL;DR
This paper reevaluates Triton's origin, suggesting it was captured via binary disruption and evolved through tides, with a low capture probability indicating a significant primordial binary population in the trans-Neptunian region.
Contribution
It extends previous models by incorporating the Nice model framework and Sun perturbations to better understand Triton's capture and orbital evolution.
Findings
Capture probability of Triton is approximately 0.7%.
Primordial binary fraction with Triton-sized bodies is estimated at 10%.
Triton's current orbit aligns with capture and tidal evolution scenarios.
Abstract
Agnor & Hamilton (2006) demonstrated that the disruption of a binary was an effective mechanism to capture Triton. The subsequent evolution of Triton's post-capture orbit could have proceeded through gravitational tides. The study by Agnor & Hamilton (2006) is repeated in the framework of the Nice model to determine the post-capture orbit of Triton. After capture it is then subjected to tidal evolution. The perturbations from the Sun and the figure of Neptune are included. The perturbations from the Sun acting on Triton cause it to spend a long time in its high-eccentricity phase, usually of the order of 10 Myr, while the typical time to circularise to its current orbit is some 200 Myr. The current orbit of Triton is consistent with an origin through binary capture and tidal evolution, even though the model prefers Triton to be closer to Neptune than it is today. The probability of…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
