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- TRAPPIST-1e is the 4th of seven planets<\/strong> in the TRAPPIST-1 planetary system, about 40 light-years away. It is a rocky world similar in size to Earth. Does it have an atmosphere? Could it be habitable?<\/li>\n
- First results from the James Webb Space Telescope<\/strong> hint at a possible atmosphere of nitrogen and methane. But more observations are needed to know for sure.<\/li>\n
- TRAPPIST-1e is in the habitable zone of its star.<\/strong> Having an atmosphere would mean it could possibly have liquid water on its surface.<\/li>\n<\/ul>\n
An atmosphere on exoplanet TRAPPIST-1e?<\/h3>\n
Scientists regard exoplanet TRAPPIST-1e as one of the most \u2013 if not the most \u2013 likely of the seven TRAPPIST-1 planets to have an atmosphere and be potentially habitable. This remarkable system of planets is less than 40 light-years away. Now, two teams of researchers report the first results from observations of TRAPPIST-1e by the James Webb Space Telescope. They said on September 8, 2025, that while the planet likely no longer has a primordial atmosphere of hydrogen, there is tentative evidence for a possible secondary atmosphere. That atmosphere \u2013 if it does indeed exist \u2013 would most likely be composed of nitrogen and methane, reminiscent of Earth\u2019s atmosphere. But it might also not have any atmosphere at all. So additional observations are needed to narrow down the possibilities.<\/p>\n
TRAPPIST-1e orbits within the habitable zone of its red dwarf star. The habitable zone is the region where temperatures could allow liquid water to exist, if there is an atmosphere. Like the other six planets in the system, the planet is rocky and close in size to Earth.<\/p>\n
So far, researchers have analyzed data from four transits of TRAPPIST-1e. That\u2019s when the planet passes in front of its star, as seen from Earth. Webb can then analyze the transmission spectrum coming from the planet for clues to its composition and atmosphere.<\/p>\n
The researchers published their peer-reviewed findings in two new papers in The Astrophysical Journal Letters<\/em> on September 8, 2025. You can read them here and here.<\/p>\n
Read more: What does habitable mean to astronomers?<\/p>\n
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? ? Seven Earth-sized worlds orbit the star TRAPPIST-1, but it is much more volatile than our sun. Scientists think the system\u2019s fourth planet is the best candidate for maintaining an atmosphere and a habitable surface: <\/p>\n
\u2014 Space Telescope Science Institute (@stsci.edu) 2025-09-08T14:04:02.648121211Z<\/p>\n<\/blockquote>\n
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A monumental sign of an atmosphere on TRAPPIST-1e could be the precursor to finally finding a living world around another star<\/p>\n
\u2014 Scientific American (@sciam.bsky.social) 2025-09-09T19:23:29.206Z<\/p>\n<\/blockquote>\n
No primordial atmosphere<\/h3>\n
Although the results are still preliminary after only four transits, the researchers said TRAPPIST-1e most likely does not have any primordial atmosphere left, if it ever had one. That\u2019s the original lightweight hydrogen atmosphere the planet formed with. Planets orbiting red dwarf stars can easily lose their atmosphere as a result of bombardment by intense radiation from the star.<\/p>\n
But it\u2019s still possible that TRAPPIST-1e could have a secondary atmosphere that formed later on.<\/p>\n
A nitrogen atmosphere on TRAPPIST-1e? Maybe<\/h3>\n
So, no primordial atmosphere. But the data so far point to another \u2013 and more interesting \u2013 possibility. The planet could have a secondary atmosphere. That\u2019s a heavier atmosphere composed of gases such as nitrogen or carbon dioxide. Those atmospheres, including Earth\u2019s, as an example, form later on in a rocky planet\u2019s lifetime. TRAPPIST-1e doesn\u2019t appear to have a primarily carbon dioxide atmosphere, like Venus and Mars.<\/p>\n
However, the researchers say that as of now, the data do<\/em> fit best with a nitrogen atmosphere. Those hints in the spectrum of the planet are very small though. They are near the limits of the detection capabilities of Webb. While the spectra of the two innermost planets, TRAPPIST-1b and TRAPPIST-1c, showed flat lines<\/em>, meaning likely little to no atmospheres, the spectrum of TRAPPIST-1e is almost flat<\/em>, with little bumps. This hints at an atmosphere, although it is still possible that there isn\u2019t one on this planet either. TRAPPIST-1d also showed hints of a possible atmosphere, maybe.<\/p>\n
![\"Graph](\"https:\/\/earthsky.org\/upl\/2025\/09\/TRAPPIST1e-transmission-spectrum-James-Webb-Space-Telescope-September-8-2025.jpg\")
View larger. | Transmission spectrum of TRAPPIST-1e, from the Webb Space Telescope. Image via NASA\/ ESA\/ CSA\/ STScI\/ Joseph Olmsted (STScI)\/ Webb Space Telescope.<\/figcaption><\/figure>\n And methane, too?<\/h3>\n
Ryan MacDonald at the University of St. Andrews, U.K., is an author on both papers. He made some interesting comments in an article for New Scientist<\/em>:<\/p>\n
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It does look like there are some bumps and wiggles in the data that, based on our atmospheric modelling, are well fit by a nitrogen-rich atmosphere, and potentially with molecules like methane.<\/p>\n
Of all the spectra we have obtained so far of the planets in the TRAPPIST-1 system, this is the one that\u2019s the most promising, that\u2019s pointing towards there potentially being something there. Obviously, I\u2019m hoping that the planet right in the middle of the habitable zone of this star has an atmosphere, because that would have incredible implications for astrobiology, our search for life and habitability.<\/p>\n<\/blockquote>\n
In response to a question I posed on Bluesky, he also noted:<\/p>\n
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CH4 (methane) is the best explanation we found for the potential bumps on the spectrum. N2 (nitrogen) doesn\u2019t have any notable absorption of its own, but we need a background gas heavier than CH4 (~ 16 proton masses) to match the data, and N2 (~ 28 proton masses) does a good job.<\/p>\n<\/blockquote>\n
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CH4 is the best explanation we found for the potential bumps on the spectrum. N2 doesn’t have any notable absorption of its own, but we need a background gas heavier than CH4 (~ 16 proton masses) to match the data, and N2 (~ 28 proton masses) does a good job.<\/p>\n
\u2014 Dr Ryan MacDonald (@distantworlds.space) 2025-09-09T06:56:34.587Z<\/p>\n<\/blockquote>\n
![\"Planet](\"https:\/\/earthsky.org\/upl\/2025\/09\/TRAPPIST1e-exoplanets-James-Webb-Space-Telescope-artists-concept-2-September-8-2025.jpg\")
View larger. | Another artist\u2019s concept of TRAPPIST-1e. Image via NASA\/ JPL-Caltech\/ New Scientist.<\/figcaption><\/figure>\n Is exoplanet TRAPPIST-1e a habitable world?<\/h3>\n
If the nitrogen and methane atmosphere really is there, then TRAPPIST-1e could potentially be habitable. If temperatures were warm enough, liquid water might be able to exist on its surface. And if<\/em> there is any water, it could be anything from a global ocean to a small sea surrounded by ice.<\/p>\n
And although the atmosphere likely isn\u2019t dominated by carbon dioxide, the researchers said there could still be enough to have a greenhouse effect, warming the planet.<\/p>\n
Nikole Lewis at Cornell University in Ithaca, New York, is also an author on both papers. She said:<\/p>\n
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A little greenhouse effect goes a long way. TRAPPIST-1 is a very different star from our sun, and so the planetary system around it is also very different, which challenges both our observational and theoretical assumptions.<\/p>\n<\/blockquote>\n
Scientists estimate the TRAPPIST-1 system to be 7.6 billion years old, significantly older than our own solar system (4.6 billion years). So maybe, just maybe<\/em>, life was able to begin on one of these enigmatic worlds.<\/p>\n
Only further observations will help determine just what atmosphere TRAPPIST-1e has, if any. Luckily, scientists are planning at least 15 more observations over the next year or so, so stay tuned!<\/p>\n
Bottom line: The first analysis results from the James Webb Space Telescope indicate that exoplanet TRAPPIST-1e might have an atmosphere of nitrogen and methane.<\/p>\n
Source: JWST-TST DREAMS: NIRSpec\/PRISM Transmission Spectroscopy of the Habitable Zone Planet TRAPPIST-1 e<\/p>\n
Source: JWST-TST DREAMS: Secondary Atmosphere Constraints for the Habitable Zone Planet TRAPPIST-1 e<\/p>\n
Via Webb Space Telescope<\/p>\n
Via New Scientist<\/p>\n
Read more: An atmosphere on TRAPPIST-1 d? New observations say maybe<\/p>\n
Read more: Innermost TRAPPIST-1 exoplanet is hot and airless<\/p>\n
<\/div>\n
\n - First results from the James Webb Space Telescope<\/strong> hint at a possible atmosphere of nitrogen and methane. But more observations are needed to know for sure.<\/li>\n