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Webb Maps Basaltic Surface of a Nearby Super-Earth and Finds No Atmosphere

The mid‑infrared technique lets scientists read a rocky planet’s surface from its heat.

Overview

  • The peer‑reviewed Nature Astronomy paper published Monday uses JWST’s Mid‑Infrared Instrument to measure the dayside heat spectrum of LHS 3844 b.
  • The spectrum best matches dark basaltic or mantle‑like rock and rules out an Earth‑style, silica‑rich continental crust.
  • Webb detected no atmospheric gases in the mid‑infrared, including sulfur dioxide, pointing to an airless and likely quiet surface today.
  • The team weighs fresh volcanic rock against an old, space‑weathered regolith and now favors the weathered scenario, with follow‑up angle‑dependent tests queued to tell solid slabs from dusty layers.
  • The planet is about 30% larger than Earth, orbits a red dwarf every 11 hours, and reaches roughly 1,000 K on its dayside, conditions that make it ideal for pioneering surface geology via thermal emission.