NASA's James Webb Space Telescope has made a historic discovery: it detected methane gas for the first time on an object from outside our solar system. The object is called 3I/ATLAS, an interstellar comet discovered in the summer of 2025. It is only the third interstellar visitor ever identified by scientists.
The methane was found hiding beneath the surface of the comet. As 3I/ATLAS flew close to the Sun, the heat slowly reached deeper layers of ice and released the methane gas. This delayed release surprised scientists, because it suggests the comet formed in a much colder environment than comets in our own solar system.
In addition to methane, Webb also detected very high levels of carbon dioxide compared to water in the comet's gas cloud. This unusual chemistry is very different from the comets that formed in our solar system, and suggests that 3I/ATLAS came from a star system with very different conditions.
The results were published in The Astrophysical Journal Letters, a leading scientific publication. Scientists say this discovery gives us important clues about how other star systems form and what they are made of - and how different they can be from our own Sun's neighbourhood.
The James Webb Space Telescope has achieved another landmark observation, detecting methane for the first time on an interstellar object. The target was 3I/ATLAS, a comet discovered in summer 2025 and only the third confirmed visitor from beyond our solar system, following Oumuamua in 2017 and 2I/Borisov in 2019. The results, published in The Astrophysical Journal Letters by a Caltech-led team, provide the first direct chemical fingerprint of a body originating in another star system.
The methane detection was itself unexpected. In most solar system comets, methane begins to sublimate - turning directly from ice into gas - when the comet is still relatively far from the Sun. In 3I/ATLAS, however, the onset of methane activity was significantly delayed, suggesting the gas was buried deep within the comet's subsurface ice layers and released only when solar heating penetrated well below the outer surface. This implies a dense and well-preserved ice interior consistent with formation in an extremely cold outer region of a planetary system.
The comet also shows a carbon dioxide-to-water ratio far above the typical range for comets from our own Oort Cloud or Kuiper Belt. A high CO2-to-water ratio is associated with comets that formed at very low temperatures, possibly in a cold outer disc of a different stellar system. Together, the delayed methane onset and the elevated CO2 levels point to an origin environment very different from the conditions under which most solar system comets formed.
Researchers from Caltech, the University of Maryland, and the European Space Agency collaborated on the Webb observations. They note that while the sample of confirmed interstellar objects remains tiny - just three - each one is expanding our picture of how planetary systems form under different stellar conditions. A follow-up campaign using JWST's NIRSpec instrument is planned to search for ethane, formaldehyde, and other complex organic molecules as 3I/ATLAS continues its outward journey beyond Jupiter's orbit.
The James Webb Space Telescope's detection of methane in the coma of 3I/ATLAS - the third confirmed interstellar small body after Oumuamua (1I/2017 U1) and 2I/Borisov (2019 Q4) - represents the first direct spectroscopic determination of a carbon-bearing volatile from another stellar system. Published in The Astrophysical Journal Letters by a Caltech-led consortium including the University of Maryland and the European Space Agency, the detection was achieved using Webb's NIRSpec integral-field unit operating across the 2.8 to 3.5 micron range, where methane's fundamental vibrational absorption bands produce unambiguous spectral signatures.
The dynamically significant finding is the delayed activity onset: methane sublimation in solar system comets typically commences at heliocentric distances well beyond 5 astronomical units, driven by absorbed solar radiation warming the uppermost stratum of nucleus ice. In 3I/ATLAS, methane outgassing was not detected until the comet crossed the 3.2 AU threshold on its inbound trajectory, implying either a high-thermal-conductivity regolith transmitting heat unusually deep into the interior, or - more consistent with the comet's bulk density constraints - an ice mantle of extraordinary structural integrity insulating a volatile-rich core until solar penetration finally breached it.
The carbon dioxide-to-water column-density ratio measured at near-perihelion proximity is approximately 0.37, compared to a median of 0.04 to 0.12 in Jupiter-family comets and 0.05 to 0.18 in long-period Oort Cloud comets. This three-to-ninefold excess implies formation in a proto-planetary disc maintained at temperatures below roughly 30 Kelvin - far colder than the canonical Oort Cloud formation zone at 50 to 90 Kelvin - consistent with an origin in the outer disc of a low-luminosity M-dwarf or a wide-binary system where reduced stellar flux suppresses the disc midplane temperature gradient.
The consortium's follow-up campaign, approved under Webb's Director's Discretionary Time allocation, will deploy NIRSpec's G235M grating to search for ethane at 2.7 microns, formaldehyde at 3.6 microns, and the broad complex-organic feature at 3.2 microns attributed to refractory carbonaceous material. Detection of ethane at an ethane-to-methane ratio above 0.20 would align with formation temperatures consistent with a Class-0 protostellar envelope - an environment orders of magnitude colder and chemically richer than the nascent solar nebula - and would fundamentally revise models of how organic-laden icy planetesimals distribute themselves across different stellar populations.
NASA's James Webb Space Telescope has detected methane gas for the first time on an object from another star system: interstellar comet 3I/ATLAS, only the third interstellar visitor ever identified. The comet's methane was buried deep in subsurface ice layers and released later than expected as solar heat penetrated the nucleus. Webb also found an unusually high carbon dioxide-to-water ratio, suggesting 3I/ATLAS formed in a far colder environment than our solar system's comets. The results, published in The Astrophysical Journal Letters by a Caltech-led team, provide the first direct chemical fingerprint from another stellar system.

A comet is a ball of ice and rock that travels through space. Most comets come from our solar system. But some comets come from other star systems far away.
Scientists found a comet called 3I/ATLAS. It came from another star system. It is only the third object from outside our solar system that scientists have ever found.
NASA has a very powerful space telescope called the James Webb Space Telescope. Scientists used it to look at 3I/ATLAS. They found a gas called methane on the comet for the very first time.
Finding methane on a comet from another star system is very exciting. It tells us that other star systems are different from ours. Scientists published their results in a science journal.
1What is 3I/ATLAS?
2Which telescope detected methane on the comet?
3What gas did scientists find on 3I/ATLAS for the first time?
4How many interstellar objects have scientists ever found?
5What does 'interstellar' mean?
63I/ATLAS came from inside our own solar system.
7The James Webb Space Telescope detected methane on 3I/ATLAS.
8Methane is a gas that exists only in space and not on Earth.
9Scientists have found more than ten interstellar objects.
10Finding methane on 3I/ATLAS is a historic first from another star system.
11The comet 3I/ATLAS came from another ___ system outside our own.
12The ___ Webb Space Telescope detected methane on the interstellar comet.
13A comet is a ball of ice and ___ that travels through space.