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arXiv · 2109.13307

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

Kalee E. Anderson·Nathan A. Kaib
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Abstract

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 system with and without a 9th planet to one another as well as to observations. The main mechanism for TNOs to be deposited into the distant ($a$ > au), detached ($q$ > au) region of the Kuiper Belt in the 8-planet model is Kozai-Lidov oscillation of objects in mean motion resonances (MMR) with Neptune. This effect does not deposit low-inclination ($i \lesssim$ 20{\deg}) objects into this region. However, we find that the 9th planet generates a group of distant, detached TNOs at low inclinations that are not present in the 8-planet model. This disparity between the 8-planet and the 9-planet models could provide a strong constraint on a possible planet 9 with further detections of TNOs in the distant, detached region of the Kuiper Belt.

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Kalee E. Anderson, Nathan A. Kaib. 2021-09-27. Signatures of a Distant Planet on the Inclination Distribution of the Detached Kuiper Belt. https://doi.org/10.3847/2041-8213%2Fac26ca

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