Dark, Chilled Planet Without Volcanoes: JWST’s Gaze ✎ express

Original: "The dark and featureless surface of rocky exoplanet LHS 3844 b from JWST mid-infrared spectroscopy"
arXiv:2605.00100 · 2026-04-30 · arXiv non-exclusive · independent analysis · 1 min
Astronomers studied the thermal radiation of planet LHS 3844 b and found a dark, old surface with no trace of volcanic gases.

📄 Showing the "Simple" version — "Popular" is not ready yet. Add it to favorites to help prioritize it.

Astronomers aimed JWST at the rocky exoplanet LHS 3844 b — a world orbiting another star, where a year lasts just 11 hours. The planet is tidally locked: one side always faces the star, with a permanent scorch of 770°C, while the night side is plunged into icy darkness. JWST captured heat from the blazing hemisphere and, using spectroscopy — splitting light into a rainbow of colors — teased out the surface composition. Each mineral leaves its own unique hue, like a glowing ember in a campfire.

The surface turned out to be dark and quartz-poor, more like basalt or olivine. Such material recalls cooled embers: maybe the planet was once hot and churning, but now its internal fire is stone dead. Volcanic gases — carbon dioxide and sulfur dioxide, the usual markers of a living mantle — are nowhere to be found. Even the sensitive JWST couldn’t spot a whiff of steaming fissures. This is a dead world where the geological furnace has gone out for good.

LHS 3844 b whips around its star in just 11 hours. Its dayside roasts at 770°C, while the nightside stays invisible — thermal emission comes only from the hot half.

Scientists
Adam RiessBrian SchmidtEdwin HubbleGeorges LemaîtreMaarten SchmidtSaul Perlmutter
Concepts
jwst exoplanet atmospheres terrestrial exoplanet JWST james webb space telescope rocky planet miri nirspec hot jupiter atmospheres sulfur dioxide erosita brown dwarf phenomena super earth mantle OISST v2.1 carbon monoxide