James Webb measures the heat of a rocky exoplanet with no atmosphere

Published on May 13, 2026 | Translated from Spanish

The James Webb Telescope has achieved a technical milestone: detecting heat emitted directly from the surface of an exoplanet. Until now, studies focused on atmospheres, but LHS 3844b, a rocky world similar to Mercury without a gaseous layer, has allowed observation of its perpetual day side, burning at high temperatures 50 light-years away.

In the image, the exoplanet LHS 3844b, rocky and without an atmosphere, shows its scorching day side under the light of its red dwarf star, with the James Webb Telescope capturing its infrared heat 50 light-years away.

How Webb Managed to Capture the Heat of a Rock 50 Light-Years Away 🔥

The team used Webb's MIRI instrument to measure the thermal emission of LHS 3844b in infrared light. Being tidally locked, its day side always faces the red dwarf star. The absence of an atmosphere allowed the telescope to record direct heat from the surface, without filters or intermediate layers. The data confirms it is a volcanic and barren desert.

A Planet with More Attitude Than a Monday Morning ☀️

LHS 3844b is the neighbor you wouldn't want. With one side always in daylight and no atmosphere, its surface must be a literal hell. If a cosmic toaster existed, this planet would be the most efficient model: constant heat, no clouds to spoil the view. At least, Webb didn't need sunscreen to take its temperature.