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Astronomers using the James Webb Space Telescope have, for the first time, directly characterised the surface of a rocky exoplanet.
Observations published in Nature Astronomy on May 4, 2026, show LHS 3844 b ā a superāEarth about 30% larger than Earth and 48.5 lightāyears away ā is a dark, airless world with a dayside temperature near 1,000 K (ā725°C). The team, led by Laura Kreidberg (Max Planck Institute for Astronomy) and Sebastian Zieba (Center for Astrophysics | Harvard & Smithsonian), used JWSTās MidāInfrared Instrument (MIRI) to measure thermal emission between 5ā12 micrometres during secondary eclipses observed in 2023ā24.
Spectral analysis rules out an Earthālike, silicaārich crust and favours basaltic or mantleālike materials rich in iron and magnesium.
The data are consistent with two scenarios: a geologically fresh basaltic surface from recent volcanism (though volcanic gases such as SO2 were not detected) or an old, spaceāweathered regolith similar to Mercury or the Moon.
Followāup JWST observations are planned to refine surface texture and composition and to test whether the surface is solid rock or loose regolith.








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