The Rocky Planet Picture Show: Implementation of Surface Reflection and Emission in POSEIDON with Application to and Interpretation of JWST Data
Elijah Mullens, Ryan J. MacDonald, Marina E. Gemma, Ishan Mishra, Esteban Gazel, Nikole K. Lewis
astro-ph.EP, astro-ph.IM
Submitted: 2026-05-01
Comments: 16 pages (main text), 24 pages (appendix), 7 figures, submitted to PSJ. This paper coincides with the public release of POSEIDON v1.4
Code: https://github.com/MartianColonist/POSEIDON
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Detecting Surface Liquid Water on Exoplanets
- Identifying rocky planets and water worlds among sub-Neptune-sized exoplanets with the Habitable Worlds Observatory
- Wavelength Requirements for Life Detection via Reflected Light Spectroscopy of Rocky Exoplanets
- Coupled atmospHere Interior modeL Intercomparison (CHILI) Protocol Version 1.0: A CUISINES Intercomparison Project of Magma Ocean Models
- A dark, bare rock for TOI-1685 b from a JWST NIRSpec G395H phase curve
- Impact of Subsurface Temperature Gradients on Emission Spectra of Airless Exoplanets: the Solid-state Greenhouse and Anti-Greenhouse
- Mantle Convection and Nightside Volcanism on Lava World K2-141 b
- Evidence for an Atmosphere on the Ultra-Short Period super-Earth HD 3167 b
- What's Inside Matters: The Effect of Oxygen Fugacity and Initial Volatile Abundance on the Atmospheres of the TRAPPIST-1 Planets
- A Thick Volatile Atmosphere on the Ultrahot Super-Earth TOI-561 b
- Sensitivity of Dry Lava Planet Atmospheric Emission Spectra to Changes in Lava Compositions
- The Thermal Emission Spectrum of the Nearby Rocky Exoplanet LTT 1445A b from JWST MIRI/LRS
- Characterizing the Dynamics and Chemistry of Transiting Exoplanets with the Habitable World Observatory
- Identifying Surface Degeneracies in Single-Visit Reflected Light Observations of Modern Earth using the Habitable Worlds Observatory
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