The Role of Formation Location in Shaping Sulfur-, Nitrogen-, and Carbon-Bearing Species in Super-Earth and Sub-Neptune Atmospheres
Aaron Werlen, Remo Burn, Caroline Dorn, Lukas Felix, Annika Salmi
astro-ph.EP
Submitted: 2026-05-14
Comments: Accepted for publication in The Astrophysical Journal
Code: https://github.com/magmasource/alphaMELTS
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- JWST Reveals CH$_4$, CO$_2$, and H$_2$O in a Metal-rich Miscible Atmosphere on a Two-Earth-Radius Exoplanet
- Water-rich sub-Neptunes and rocky super Earths around different Stars: Radii shaped by Volatile Partitioning, Formation, and Evolution
- A New Global Chemical Equilibrium Code: Refractory Element Signatures in Super-Earths and Sub-Neptunes
- A water-rich interior in the temperate sub-Neptune K2-18 b revealed by JWST
- The Influences of Hydrogen-Silicate-Iron Miscibility on the Demographics of Sub-Neptunes and Super-Earths
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