Researchers have discovered the first atmosphere surrounding a rocky planet similar to Tierra orbiting within the habitable zone of a distant star.
The planet, called LHS 1140 b, is 48 light years from Earth and orbits a red star much smaller and cooler than our Sun.
More than 6,000 worlds have been discovered orbiting distant stars. But this discovery is significant because it brings us one step closer to one of the greatest achievements of science: the discovery of life on another world.
The researchers, in an article published in the journal Scienceare clear: they have not achieved it yet, at least not yet.
But for a planet to support life, it must have water and, to do so, it must be at the appropriate distance from its star: neither too close, because it will be too hot, nor too far, because it will be too cold, but somewhere in between where the conditions are optimal.
Planetary scientists call it the “Goldilocks zone,” after the fairy-tale girl who was very picky about the temperature of her porridge.
Hundreds of planets have been discovered in the habitable zones of their respective stars, but only a few dozen are small and rocky, like our own Earth, which is another point in favor of a planet’s ability to support life.
But none of them have been found to have an atmosphere. Until now.
Of course, the only gas discovered at the moment in the atmosphere of LHS 1140 b is helium, probably in the upper atmosphere, which alone could not support life.
There may be other gases more essential for life, at lower depths.
David Charbonneau, a scientist also at Harvard, stated that The important thing was the discovery of a planet similar to Earth outside our solar system and with an atmosphere.
“People are often interested in the big questions: ‘Are we alone? Is there life beyond Earth or beyond our solar system?’ In that sense, this study reveals the first atmosphere discovered on a rocky planet in the habitable zone of a star outside our solar system,” he said.
LHS 1140b is not the only world under scrutiny in the search for life. K2-18b, a sub-Neptunian planet with a possible water-rich interior, made headlines when scientists detected traces of dimethyl sulfide, a gas linked to marine life on Earth.
However, a new analysis led by NASA in 2025 determined that the signal was too weak to confirm and demonstrated that the gas can form without biological intervention.
The seven rocky worlds of TRAPPIST-1 remain intriguing: NASA’s James Webb Space Telescope ruled out an Earth-like atmosphere in TRAPPIST-1d, while the data from TRAPPIST-1e remains frustratingly inconclusive.
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