Neptune migration model with one extra planet
Lun-Wen Yeh, Hsiang-Kuang Chang

TL;DR
This study investigates a modified Neptune migration model with an extra planet to better explain Kuiper belt structures, but finds it has low probability and some observational inconsistencies.
Contribution
It introduces a Neptune migration model with an additional planet in resonance, aiming to improve Kuiper belt structure explanations over traditional models.
Findings
Better explanation of Kuiper belt features compared to standard models
Low probability of the proposed scenario
Potential inconsistency with observed low-inclination Kuiper belt objects
Abstract
We explore conventional Neptune migration model with one additional planet of mass at 0.1-2.0 Me. This planet inhabited in the 3:2 mean motion resonance with Neptune during planet migration epoch, and then escaped from the Kuiper belt when Jovian planets parked near the present orbits. Adding this extra planet and assuming the primordial disk truncated at about 45 AU in the conventional Neptune migration model, it is able to explain the complex structure of the observed Kuiper belt better than the usual Neptune migration model did in several respects. However, numerical experiments imply that this model is a low-probability event. In addition to the low probability, two features produced by this model may be inconsistent with the observations. They are small number of low-inclination particles in the classical belt, and the production of a remnant population with near-circular and…
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.
