NASA’s James Webb Space Telescope Detects Methane on Interstellar Comet 3I/ATLAS
NASA and ESA’s James Webb Space Telescope (JWST) made the first direct detection of methane on the interstellar comet 3I/ATLAS during December 2025 observations. JWST’s Mid-Infrared Instrument (MIRI) recorded mid-infrared spectra revealing a high methane-to-water ratio and unusually high carbon dioxide levels. This discovery highlights the unique chemical composition of 3I/ATLAS compared to typical Solar System comets and provides insights into its distinct formation environment.
On this page

Key Facts
- 3I/ATLAS was discovered on July 1, 2025, by the NASA-funded ATLAS survey telescope in Chile.
- The James Webb Space Telescope observed 3I/ATLAS using its Mid-Infrared Instrument (MIRI) on two occasions: December 15-16 and December 27, 2025.
- During these observations, the comet was approximately 329 million kilometers (205 million miles) and 379 million kilometers (236 million miles) from the Sun, respectively.
- This marked the first direct detection of methane gas in an interstellar object.
- The methane was found to sublimate from ice buried beneath the comet’s surface layers as it heated during its perihelion passage.
- The methane-to-water ratio is unusually high, and the comet exhibits elevated carbon dioxide relative to water compared to typical Solar System comets.
- The research results were published in The Astrophysical Journal Letters on April 8, 2026.
Background & Context
An interstellar object (ISO) is a natural celestial body originating outside the Solar System and passing through it on a hyperbolic trajectory. 3I/ATLAS is the third confirmed ISO after 1I/ʻOumuamua and 2I/Borisov. Methane (CH4) is a hydrocarbon molecule that is highly volatile and important for understanding the volatile composition in cometary and protoplanetary systems. JWST’s MIRI instrument can detect mid-infrared light, ideal for studying gases like methane and carbon dioxide in cold objects such as comets.
Why This Matters for Exams / Exam Relevance
This landmark discovery demonstrates the advanced capabilities of modern space telescopes like JWST, provides direct evidence of methane in an interstellar visitor, and enhances our understanding of chemical diversity in planetary system formation beyond our own Solar System. Details such as discovery dates, technological instruments, chemical compositions, and interstellar object characteristics are frequently examined in competitive science and current affairs exams.
Points to Remember
- 3I/ATLAS is the third confirmed interstellar object passing through the Solar System.
- Methane gas was directly detected on 3I/ATLAS for the first time by JWST’s MIRI instrument in December 2025.
- The comet’s volatile composition—especially methane and carbon dioxide content—is distinct from most Solar System comets, indicating a different formation environment.
- The findings were published in a peer-reviewed journal in April 2026.
- The delayed release of methane suggests it was buried beneath the comet’s surface and released due to solar heating during perihelion.
Sources & Further Reading
| Document / Website | Link |
|---|---|
| NASA’s Webb Detects Methane on Interstellar Comet 3I/ATLAS - NASA Science | Open NASA’s Webb Detects Methane on Interstellar Comet 3I/ATLAS - NASA Science ↗science.nasa.gov |