Reinterpreting the JWST Observations of 55 Cancri e with a Non-Grey General Circulation Model
Ruizhi Zhan, Daniel D. B. Koll
astro-ph.EP
Submitted: 2026-06-10
Comments: Accepted for publication in ApJ
Code: https://github.com/Trovemaster/exocross
Project page: https://hitran.org
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Magma Ocean Waves and Thermal Variability on Lava Worlds
- The Cosmic Shoreline Revisited: A Metric for Atmospheric Retention Informed by Hydrodynamic Escape
- Extreme Weather Variability on Hot Rocky Exoplanet 55 Cancri e Explained by Magma Temperature-Cloud Feedback
- JWST reveals a rapid and strong day side variability of 55 Cancri e
- Characterising the Atmosphere of 55 Cancri e: 1D Forward Model Grid for Current and Future JWST Observations
Related papers
- PDS 70 c and SR 12 c: Observational Constraints on Giant-Planet and Satellite Formation
- Two-stage disruption of resonant chains
- Detectability of resolved hydrogen lines from the accretion shock at gas giants and their CPDs
- Binary-lens Microlensing Degeneracy: Impact on Planetary Sensitivity and Mass-ratio Function
- Atmospheric escape fractionates secondary but not primary atmospheres
- The Occurrence Rate of Nearby Planetary Companions to Hot Jupiters