First atmosphere found around Earth-like planet LHS 1140b

by | Jul 17, 2026 | Science

News summary produced by Claude AI

An international team of researchers has announced the detection of an atmosphere surrounding LHS 1140b, a rocky planet located approximately 48 light-years from Earth in the habitable zone of a red dwarf star. The finding represents a significant milestone in the study of exoplanets, as it is the first time an atmosphere has been confirmed around an Earth-like, rocky world orbiting within the region where liquid water could theoretically exist.

The atmosphere was detected using spectroscopic analysis, which identified helium as the primary gas component currently confirmed in the upper atmosphere. While helium alone cannot sustain life, researchers suggest that additional gases capable of supporting biological processes may exist in lower atmospheric layers. The discovery was published in the journal Science and was led by Dr. Collin Cherubim of Harvard University, with contributions from colleagues including Dr. David Charbonneau.

The significance of this discovery lies in its contribution to understanding the prevalence of potentially habitable worlds beyond our solar system. Among the more than 6,000 known exoplanets, hundreds have been identified within habitable zones, but only a few dozen possess the small, rocky composition similar to Earth. The detection of an atmosphere on such a world represents a crucial step toward determining whether conditions suitable for life exist elsewhere in the universe.

The finding comes as part of ongoing efforts to search for biosignatures and habitable environments on distant worlds. Other planets of interest in this research include K2-18b, which showed potential signs of dimethyl sulphide until recent analysis suggested the signal was too weak to confirm, and the TRAPPIST-1 system’s seven rocky worlds, which continue to present inconclusive or negative results regarding Earth-like atmospheric compositions. The work underscores the expanding capability of modern telescopes and analytical techniques to characterize distant planetary atmospheres.

Article Attribution | Read More at Article Source