A radius valley between migrated steam worlds and evaporated rocky cores
Remo Burn, Christoph Mordasini, Lokesh Mishra, Jonas Haldemann, Julia, Venturini, Alexandre Emsenhuber, Thomas Henning

TL;DR
This study presents a comprehensive model that explains the observed exoplanet radius gap by combining planet formation, migration, and atmospheric escape, emphasizing water-rich planets' role in the distribution.
Contribution
It introduces an advanced coupled formation and evolution model that naturally reproduces the radius valley by considering water as vapor mixed with H/He, integrating migration and atmospheric escape effects.
Findings
The model reproduces the observed radius valley location.
Water-rich planets are mainly ex-situ, while rocky super-Earths are in-situ.
Atmospheric photoevaporation explains the radius cliff.
Abstract
The radius valley (or gap) in the observed distribution of exoplanet radii, which separates smaller super-Earths from larger sub-Neptunes, is a key feature that theoretical models must explain. Conventionally, it is interpreted as the result of the loss of primordial H/He envelopes atop rocky cores. However, planet formation models predict that water-rich planets migrate from regions outside the snowline toward the star. Assuming water to be in the form of solid ice in their interior, many of these planets would be located in the radius gap, in disagreement with observations. Here we use an advanced coupled formation and evolution model that describes the planets' origin and evolution starting from moon-sized, planetary seed embryos in the protoplanetary disk to mature Gyr-old planetary systems. Employing new equations of state and interior structure models to treat water as vapor mixed…
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Taxonomy
TopicsAstro and Planetary Science · Stellar, planetary, and galactic studies · Scientific Research and Discoveries
