Dayside Temperature (occultation): 999999 K |
JWST-MIRI | Improved Constraints on the Surface of LHS 3844 b from its Mid-Infrared Spectrum2026, Kimberly Paragas, Heather A. Knutson et al. |
emission spectrum resembles a blackbody shortward of 10 μm |
Featureless spectra: Detection
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JWST-MIRI | The dark and featureless surface of rocky exoplanet LHS 3844 b from JWST mid-infrared spectroscopy2026, Sebastian Zieba, Laura Kreidberg et al. |
results are well fit by an old, space-weathered surface with no evidence of accumulated volcanic gases. |
Phase curve: Yes |
Spitzer | Super-Earth LHS3844b is tidally locked2023, Xintong Lyu, Daniel D. B. Koll et al. |
Super-Earth LHS3844b is tidally locked |
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G-B: Low resolution visible | Optical Transmission Spectroscopy of the Terrestrial Exoplanet LHS 3844b from 13 Ground-based Transit Observations2020, Diamond-Lowe, Hannah, Charbonneau, David et al. |
No clear, low mean molecular weight (H/He-dominated) atmosphere |