Interstellar Comet 3I/ATLAS Exhibits Increased Activity Post-Perihelion
NASA's SPHEREx telescope observed a significant rise in activity from interstellar comet 3I/ATLAS in December 2025, detecting increased emissions of water vapor, carbon dioxide, and organic molecules.
In December 2025, NASA's SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) observed a notable increase in activity from interstellar comet 3I/ATLAS, approximately two months after its closest approach to the Sun in late October. The telescope detected heightened emissions of water vapor, carbon dioxide, and organic molecules within the comet's coma, indicating that the Sun's heat had penetrated the comet's surface, causing the sublimation of volatile compounds.
The observations revealed a significant rise in water production, nearly 40 times higher than levels recorded in August 2025. Carbon dioxide emissions increased by a factor of 80, and the ratio of carbon monoxide to carbon dioxide adjusted to 2.5, aligning with typical values observed in solar system comets. Additionally, the presence of organic molecules such as methanol, formaldehyde, methane, and ethane was detected, along with a spectral line indicating cyanide outgassing.
These findings suggest that 3I/ATLAS, the third confirmed interstellar object, is undergoing significant compositional changes as it interacts with solar radiation. The comet's activity provides a unique opportunity to study the behavior and composition of interstellar objects as they traverse the solar system.