A newly discovered interstellar comet, known as 3I/ATLAS, has surprised scientists with its unusually high levels of methanol, a type of alcohol. This discovery suggests that the comet formed under conditions very different from those in our solar system. Using the Atacama Large Millimeter/submillimeter Array (ALMA), astronomers observed the comet in late 2025 as it approached the Sun. As the comet warmed, gas and dust were released, forming a bright cloud, or coma, around its core. By analyzing the molecules in this coma, scientists determined the comet's chemical composition. Their focus was on methanol (CH₃OH) and hydrogen cyanide (HCN), a nitrogen-containing organic molecule commonly found in comets. ALMA revealed that 3I/ATLAS has an unusually high ratio of methanol to hydrogen cyanide, with measurements showing ratios of about 70 and 120 on two observation dates. This makes 3I/ATLAS one of the most methanol-rich comets ever studied.
Earlier observations using the James Webb Space Telescope found that 3I/ATLAS had a coma dominated by carbon dioxide when it was still far from the Sun. The new ALMA data now show a significant amount of methanol, adding to the list of unusual features in the comet's chemical makeup. ALMA's high-resolution imaging also allowed scientists to track how different molecules are released and travel away from the comet. They observed a notable difference in the behavior of methanol and hydrogen cyanide. Hydrogen cyanide mainly originates from the comet's central body, or nucleus, which is typical for comets in our solar system. Methanol, however, seems to come from both the nucleus and from tiny ice particles floating in the coma. These icy grains act like miniature comets, releasing methanol as they warm up and turn into gas.
As 3I/ATLAS gets closer to the Sun, the increasing temperatures cause the ice in these grains to vaporize, releasing more methanol into the coma. This behavior has been seen in some comets from our solar system, but it is the first time scientists have observed this process in an interstellar object. Comet 3I/ATLAS is only the third confirmed object to have entered our solar system from interstellar space, following 1I/'Oumuamua and 2I/Borisov. Previous studies of these interstellar visitors also revealed unusual characteristics. As astronomers discover and study more interstellar objects, each one offers a chance to compare our solar system with those around other stars. The unusual chemistry of 3I/ATLAS adds to the growing understanding of how planets, comets, and other small bodies form around distant stars.
Interstellar Comet 3I/ATLAS Contains High Levels of Methanol
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