Webb Maps Olivine-Rich Surface of Nearby Airless Super-Earth

TL;DR Summary
JWST’s mid-infrared spectroscopy reveals LHS 3844 b, a rocky super-Earth about 50 light-years away, has a dark, olivine-rich crust with no detectable CO2 or SO2 and likely no atmosphere. The planet is roughly 30% larger than Earth, orbits its red dwarf in 11 hours, and is tidally locked, resulting in a scorching dayside and a barren surface. This demonstrates JWST’s ability to infer surface texture and geology of distant worlds, opening new possibilities for direct exoplanet terrain characterization via infrared data.
Topics:science#exoplanets#james-webb-space-telescope#lhs-3844-b#mid-infrared-spectroscopy#space#super-earth
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