CO: Detection H2O: Detection Phase curve: Yes |
G-B: High resolution IR | Unraveling the Mystery of the Peculiar and Young Hot Jupiter CoRoT-2b II: Phase Resolved Emission Spectroscopy with VLT/CRIRES+ and Gemini-S/IGRINS2026, Aurora Y. Kesseli, Siddharth Gandhi et al. |
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Albedo: 0.33 Phase curve: Yes Dayside Temperature (occultation): 1760 K |
Spitzer | A Comprehensive Analysis Spitzer 4.5 $μ$m Phase Curve of Hot Jupiters2024, Lisa Dang, Taylor J. Bell et al. |
Dayside and nightside temperatures from phase curve at 4.5 um. |
Dayside Temperature (occultation): 999999 K |
Spitzer | Warm Spitzer Photometry of the Transiting Exoplanets CoRoT-1 and CoRoT-2 at Secondary Eclipse2011, Deming, Drake, Knutson, Heather et al. |
The spectrum of CoRoT-2 is unusual because the 8 μm contrast is anomalously low. |
Dayside Temperature (occultation): 999999 K |
Spitzer | The thermal emission of the young and massive planet CoRoT-2b at 4.5 and 8 μm2010, Gillon, M., Lanotte, A. A. et al. |
Poor heat distribution on the night side of the planet and agree better with an atmosphere free of temperature inversion |
CO: Detection H2O: Detection
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G-B: High resolution IR | Astro-ph arXiv:2605.20340 |