Producing Distant Planets by Mutual Scattering of Planetary Embryos
Kedron Silsbee, Scott Tremaine

TL;DR
This paper explores how planetary embryos formed in the outer solar system could be scattered into distant orbits, potentially surviving today and influencing the structure of the Kuiper belt and detached disk.
Contribution
It introduces N-body simulations demonstrating the likelihood of surviving distant planetary embryos and their impact on the solar system's outer regions.
Findings
Potential existence of sub-Earth mass embryos beyond Neptune
Embryo orbits typically have perihelia of 40-70 AU and semi-major axes less than 200 AU
Surviving embryos could be detectable or influence solar system dynamics
Abstract
It is likely that multiple bodies with masses between those of Mars and Earth ("planetary embryos") formed in the outer planetesimal disk of the solar system. Some of these were likely scattered by the giant planets into orbits with semi-major axes of hundreds of AU. Mutual torques between these embryos may lift the perihelia of some of them beyond the orbit of Neptune, where they are no longer perturbed by the giant planets so their semi-major axes are frozen in place. We conduct N-body simulations of this process, and its effect on smaller planetesimals in the region of the giant planets and the Kuiper belt. We find that (i) there is a significant possibility that one sub-Earth mass embryo, or possibly more, is still present in the outer solar system; (ii) the orbit of the surviving embryo(s) typically has perihelion of 40--70 AU, semi-major axis less than 200 AU, and inclination less…
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.
