JWST mid-IR spectroscopy shows LHS 3844 b has a dark, space-weathered, low-silica surface with no evidence of accumulated CO2 or SO2 gases.
P.et al.Population-level Hypothesis Testing with Rocky Planet Emis- sion Data: A Tentative Trend in the Brightness Temperatures of M-Earths
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The dark and featureless surface of rocky exoplanet LHS 3844 b from JWST mid-infrared spectroscopy
JWST mid-IR spectroscopy shows LHS 3844 b has a dark, space-weathered, low-silica surface with no evidence of accumulated CO2 or SO2 gases.