
NASA’s James Webb Space Telescope unveils a barren super-Earth resembling Mercury, proving American ingenuity pierces cosmic distances to reveal harsh truths about alien worlds.
Story Highlights
- JWST directly observes dayside of LHS 3844 b, a super-Earth 48 light-years away with surface like a scaled-up Mercury or Moon.
- Dark, rocky, airless world shows no signs of active volcanism or atmosphere, challenging prior exoplanet models.
- Breakthrough validates $10 billion JWST investment, advancing U.S. leadership in space exploration.
- Researchers led by Sebastian Zieba and Laura Kreidberg confirm low-albedo crust via mid-infrared data.
- Findings inform planetary evolution, suggesting many super-Earths end as lifeless rocks.
Discovery Details
NASA’s James Webb Space Telescope targeted LHS 3844 b using its Mid-Infrared Instrument in late 2025. This super-Earth, 30% larger than Earth at 1.3 Earth radii, orbits red dwarf LHS 3844 every 4.2 days. Tidally locked, its dayside reaches 1,100 K, hot enough to vaporize rocks. Observations detected thermal emission from a dark, rocky surface with low albedo, akin to basaltic crust or dust-covered regolith. No sulfur dioxide appeared, ruling out recent volcanism.
Research Leadership
Sebastian Zieba from Harvard-Smithsonian Center for Astrophysics led the study, with Laura Kreidberg of Max Planck Institute for Astronomy as principal investigator. Penn State researchers, including Avi Mandell, contributed analysis. The team published findings in Nature in March 2026, with May reports from Phys.org and Penn State detailing the Mercury-like traits. NASA’s TESS satellite discovered the planet in 2020, enabling JWST follow-up. This U.S.-Europe collaboration showcases efficient use of taxpayer-funded tools.
Experts favor a dust-covered surface over hard crust, matching low thermal inertia. Kreidberg stated JWST’s sensitivity revealed light from the bare surface, devoid of atmosphere. The data contrasts with TOI-561 b, which retains a thick atmosphere despite similar conditions, broadening understanding of super-Earth diversity.
Scientific Implications
Results validate JWST for direct surface studies of exoplanets, refining models for ultra-short-period planets around M-dwarfs. Such worlds, common at 0.5-1% of these stars, often lose atmospheres, leaving barren rock. This informs planetary formation and evolution, suggesting many super-Earths become “dead” worlds with stagnant lid tectonics, like our Moon or Mercury. Follow-up observations will test regolith versus solid slabs.
George McInerney finds this interesting 👍 Webb space telescope reveals a scorching “super-Earth” that looks like Mercury https://t.co/9NEKwuegq8
— George McInerney (@gmcinerney) May 6, 2026
Short-term, the discovery boosts proposals for 100 similar targets in JWST Cycle 3. Long-term, it aids designs for future missions like Habitable Worlds Observatory. The $10 billion JWST investment yields returns, inspiring public interest in space while reinforcing American innovation against global competitors. No policy changes emerge, but it underscores limited government’s role in high-impact science.
Sources:
First look at distant rocky planet reveals moon-like world (Penn State University Science News)
Astronomers explore the surface composition of a nearby super-Earth (ScienceDaily)
Astronomers explore the surface composition of a nearby super-Earth (Phys.org)
Dark, airless super-Earth like Mercury (Daily Galaxy)
JWST spots a nearby super-Earth that could look like the Moon or Mercury (Discover Magazine)
Dark dust instead of hard crust near super-Earth reminds of known planets (Ground News)



