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Discovery of a Dwarf Planet Candidate in an Extremely Wide Orbit: 2017 OF201

2025/05/21 by Sihao Cheng, Jiaxuan 嘉轩 Li 李, Jiaxuan Li +4 · 11 voices · 2 citations
Physics and Astronomy · #Astro and Planetary Science #Stellar, planetary, and galactic studies #Gamma-ray bursts and supernovae

paper · pdf · doi:10.3847/2041-8213/ae3a75

Abstract

Abstract We report the discovery of a dwarf planet candidate, 2017 OF201, currently located at a distance of 90 au. Its orbit is extremely wide and extends to the inner Oort cloud, with a semimajor axis of 830 au and a perihelion of 45 au, precisely determined from 24 observations over 20 yr. Assuming a typical albedo of 0.13, we estimate a diameter ∼700 km, making it the second-largest known object in this dynamical population and a dwarf planet candidate with the widest orbit. Its high eccentricity suggests that an unseen population of similar objects would total ∼1% of Earth’s mass. Notably, the longitude of perihelion of 2017 OF201 lies outside the clustering observed in extreme trans-Neptunian objects, posing a challenge to the proposed dynamical evidence for the hypothetical Planet Nine.

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