What is LHS 3844 b?
LHS 3844 b is a rocky exoplanet about 30% larger than Earth, located nearly 50 light-years away.
Space / Exoplanets
The James Webb Space Telescope (JWST) has achieved a groundbreaking milestone by directly analyzing the surface of an exoplanet for the first time. This achievement provides unprecedented insights into the composition and geology of planets...
The James Webb Space Telescope's Mid-Infrared Instrument (MIRI) was used to measure the infrared light emitted from the intensely hot dayside of LHS 3844 b. By comparing the signal with known rocks and minerals from Earth, the Moon, and Mars, researchers determined that the surface is dominated by basalt, a dark volcanic rock rich in iron and magnesium.
The absence of an Earth-like crust suggests that LHS 3844 b lacks the plate tectonics and water-driven geological processes that shape our planet. The exoplanet's proximity to its star results in extreme temperatures and tidal locking, with one side constantly facing the star.
Two scenarios are proposed for the planet's surface: recent volcanic activity creating a fresh basalt surface, or prolonged space weathering resulting in a dark, fine-grained material similar to the Moon or Mercury. Follow-up observations are planned to further refine the planet’s surface properties and determine whether it is solid rock or loose, weathered material.
LHS 3844 b is a rocky exoplanet about 30% larger than Earth, located nearly 50 light-years away.
The dayside temperature reaches about 1,340 degrees Fahrenheit (725 degrees Celsius).
The surface is likely composed of basalt, similar to the Moon or Mercury.
No, observations suggest that LHS 3844 b is a barren, airless world.
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