Wednesday, 28 October 2026
Science•Factual Reporting

James Webb Space Telescope Identifies Carbon-Rich Atmosphere on Temperate Super-Earth

Spectroscopic observations of LHS 1140 b reveal clear signatures of carbon dioxide and water vapor, positioning the world as a prime candidate for habitable zone study.

Dr. Vaneet Rao
By Dr. Vaneet Rao
Sunday, October 25, 2026 at 03:20 PM UTC
James Webb Space Telescope Identifies Carbon-Rich Atmosphere on Temperate Super-Earth
Artist concept of exoplanet LHS 1140 b orbiting its cool red dwarf host star 48 light-years away.Photo: NASA / ESA / CSA / STScI
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Astronomers analyzing deep infrared transmission spectra from the James Webb Space Telescope have reported the strongest evidence to date of a secondary atmosphere enveloping the temperate exoplanet LHS 1140 b.

Located approximately 48 light-years from Earth in the constellation Cetus, the planet orbits comfortably within the circumstellar habitable zone of a low-activity red dwarf star.

The detection of prominent absorption dips corresponding to carbon dioxide and methane, without corresponding helium or hydrogen envelopes, strongly indicates a differentiated rocky mantle with potential global surface ocean coverage.

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Dr. Vaneet Rao
About the Journalist

Dr. Vaneet Rao

Covers planetary science, astronomy, and orbital missions.

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