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.
A.et al.The Detectability of Rocky Planet Surface and Atmo- sphere Composition with the JWST: The Case of LHS 3844b.Astron
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.EP 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
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.