Polar Neptunes are Stable to Tides
Emma Louden, Sarah Millholland

TL;DR
This study investigates the long-term stability of polar Neptune-sized exoplanets' orbits, demonstrating that such orbits are stable over billions of years and are consistent with observed systems given certain tidal quality factors.
Contribution
The paper provides the first extensive analysis showing that polar Neptune orbits remain stable over Gyr timescales, challenging previous assumptions about tidal realignment effects.
Findings
Polar orbits are stable over Gyr timescales.
Inclination damping does not affect polar cases.
Case studies of WASP-107 b and HAT-P-11 b support the theory.
Abstract
There is an intriguing and growing population of Neptune-sized planets with stellar obliquities near . One previously proposed formation pathway is a disk-driven resonance, which can take place at the end stages of planet formation in a system containing an inner Neptune, outer cold Jupiter, and protoplanetary disk. This mechanism occurs within the first Myr, but most of the polar Neptunes we see today are Gyrs old. Up until now, there has not been an extensive analysis of whether the polar orbits are stable over Gyr timescales. Tidal realignment mechanisms are known to operate in other systems, and if they are active here, this would cause theoretical tension with a primordial misalignment story. In this paper, we explore the effects of tidal evolution on the disk-driven resonance theory. We use both -body and secular simulations to study tidal…
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Taxonomy
TopicsAstro and Planetary Science · Space Exploration and Technology · Isotope Analysis in Ecology
