Turns out, when a visitor from another star system drops by, it doesn't just bring good vibes. Sometimes, it brings a lot of methanol. Comet 3I/ATLAS, only the third confirmed interstellar object to grace our solar system with its presence, is making astronomers raise an eyebrow, then quickly grab their telescopes.
New observations reveal this cosmic wanderer is absolutely brimming with methanol — a type of alcohol — in amounts rarely seen in our own solar system's comets. As lead author Nathan Roth put it, observing 3I/ATLAS is like getting a "fingerprint from another solar system." A very boozy fingerprint, apparently.
What's in a Comet's Cloud?
Researchers pointed the ALMA telescope in Chile at 3I/ATLAS in late 2025. As the comet swung by the Sun, its icy surface warmed up, spewing gas and dust into a bright, swirling cloud around its core. Think of it as a celestial exhaust plume.
We're a new kind of news feed.
Regular news is designed to drain you. We're a non-profit built to restore you. Every story we publish is scored for impact, progress, and hope.
Start Your News DetoxBy dissecting the molecules in this cloud, astronomers could essentially read the comet's chemical resume. Since 3I/ATLAS is an outsider, these measurements offer a rare peek into how icy bodies form around other, distant stars. And what a peek it was.
Scientists zeroed in on methanol and hydrogen cyanide (a common organic molecule in comets). ALMA showed 3I/ATLAS has a wildly high methanol-to-hydrogen cyanide ratio, making it one of the most methanol-rich comets ever put under the cosmic microscope. Someone's star system has a serious affinity for alcohol.
Tiny Ice Grains, Big Revelations
This unusual chemical cocktail suggests 3I/ATLAS formed under conditions quite different from the comets we're used to. Earlier peeks with the James Webb Space Telescope showed it had a lot of carbon dioxide when it was far from the Sun. Now, ALMA confirms the methanol abundance, adding to its already unique profile.
Even more fascinating? ALMA could track how these molecules were released. Hydrogen cyanide mostly oozed from the comet's central body, or nucleus – pretty standard. But methanol? That came from both the nucleus and from tiny ice particles floating around in the comet's cloud. Essentially, these little ice grains were acting like mini-comets, turning into gas and releasing even more methanol as they warmed up.
It's the first time astronomers have traced this detailed process in an object from interstellar space. And it adds another layer to the mystery of these cosmic tourists. First 'Oumuamua, then Borisov, and now ATLAS, each showing off some truly peculiar characteristics. Each new visitor helps us compare our familiar solar neighborhood with the wild, chemical diversity of the wider galaxy. And if that's not enough to make you want to tell someone, what is?











