2022
DOI: 10.48550/arxiv.2204.13573
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A low-eccentricity migration pathway for a 13-h-period Earth analogue in a four-planet system

Luisa Maria Serrano,
Davide Gandolfi,
Alexander J. Mustill
et al.

Abstract: It is commonly accepted that exoplanets with orbital periods shorter than 1 day, also known as ultra-short period (USP) planets, formed further out within their natal protoplanetary disk, before migrating to their current-day orbits via dynamical interactions. One of the most accepted theories suggests a violent scenario involving high-eccentricity migration followed by tidal circularization. Here, we present the discovery of a four planet system orbiting the bright (V=10.5) K6 dwarf star TOI-500. The innermos… Show more

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“…At the end of this process, the innermost planet becomes a USP planet, while the second planet, an Earth-or super-Earth-sized planet, stabilizes itself on a 10 day orbit. TOI-500 is the first four-planet system for which this mechanism has been proven to work (Serrano et al 2022). Millholland & Spalding (2020) proposed an obliquity-driven tidal migration mechanism.…”
Section: Introductionmentioning
confidence: 99%
“…At the end of this process, the innermost planet becomes a USP planet, while the second planet, an Earth-or super-Earth-sized planet, stabilizes itself on a 10 day orbit. TOI-500 is the first four-planet system for which this mechanism has been proven to work (Serrano et al 2022). Millholland & Spalding (2020) proposed an obliquity-driven tidal migration mechanism.…”
Section: Introductionmentioning
confidence: 99%