Interstellar Visitor 3I/Atlas Ejects Life Precursors While Receding from the Sun

Edited by: Uliana S.

A new image of the interstellar comet 3I/ATLAS, obtained with the Hubble Space Telescope. At the moment the image was taken, the object was approximately 286 million kilometers from Earth.

Astrochemists working with the National Aeronautics and Space Administration (NASA) have confirmed that the interstellar object 3I/Atlas, the third known visitor from beyond our solar system, is actively venting essential chemical compounds crucial for abiogenesis. This activity is occurring as the object moves away from the Sun following its closest approach to the star on October 29, 2025.

Observations conducted throughout 2025 provided tangible evidence supporting astrobiological theories, particularly those related to panspermia. The Atacama Large Millimeter/submillimeter Array (ALMA) in Chile proved instrumental in gathering highly detailed spectroscopic data. The analysis, spearheaded by NASA’s team under Dr. Martin Cordiner at the Goddard Space Flight Center, uncovered unexpectedly high concentrations of two key life precursors: hydrogen cyanide (HCN) and methanol (CH3OH) within the comet’s coma. Methanol accounts for roughly eight percent of the total material being vaporized, a level approximately four times greater than what has been recorded in native Solar System comets. Hydrogen cyanide is being released from the rocky nucleus at a rate estimated between 250 and 500 grams per second.

The object 3I/Atlas was first spotted on July 1, 2025, by the ATLAS telescope system. Its perihelion—the point of closest proximity to the Sun—was successfully navigated on October 29, 2025. Dr. Cordiner concluded that such a prolific output of methanol suggests that achieving high levels of chemical complexity might be unattainable without its prior formation. This finding bolsters the hypothesis that objects like 3I/Atlas could have seeded life on Earth billions of years ago. Furthermore, the ratio of methanol to hydrogen cyanide, as measured by ALMA across various solar distances, stands at 124 to 79, surpassing most Solar System comets, second only to C/2016 R2 (PanSTARRS).

Harvard University astrophysicist Avi Loeb offered an interpretation linking this chemical profile to his theory of directed panspermia. He suggested the object possesses a 'benign nature,' based on the unusually high ratio of methanol to hydrogen cyanide. However, Loeb also pointed out persistent anomalies, such as the seven distinct jets emanating from the surface. He argued that a naturally formed comet would lack the necessary surface area to sustain the observed mass flow rate from these jets.

Object 3I/Atlas exhibits a hyperbolic orbital eccentricity of 6.139, which definitively confirms its extrasolar origin. Estimates suggest it may have traversed the Milky Way disk for anywhere between 7 and 11 billion years. The closest approach to Earth is scheduled for December 19, 2025, at a distance of roughly 270 million kilometers (1.8 astronomical units). At that time, the comet will be too faint for the naked eye, registering around a visual magnitude of +14.75m. The European Space Agency’s JUICE mission is slated to provide additional data following its own perihelion passage on November 4, 2025, while NASA’s Juno probe will make a close pass on March 16, 2026. The scientific community, including Nathan Roth’s team at the Goddard Center, continues to scrutinize the data to ascertain whether these chemical signatures stem from galactic radiation exposure or point toward entirely different formation processes. As 3I/Atlas departs the Solar System at a velocity of approximately 58 km/s, it offers an invaluable opportunity to study the chemistry inherent in exoplanetary systems.

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