Signatures of a Distant Planet on the Inclination Distribution of the Detached Kuiper Belt

A distant, massive planet in the outer solar system has recently been proposed to explain some observed features of extreme trans-Neptunian objects (TNOs). Here we use N-body simulations of the formation of the Kuiper belt and Oort cloud as well as a survey simulator to compare models of the solar s...

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Veröffentlicht in:arXiv.org 2021-09
Hauptverfasser: Anderson, Kalee E, Kaib, Nathan A
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Sprache:eng
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