Key Takeaways

  • Webb's NIRSpec found 3I/ATLAS holds about 30 times more deuterium (heavy hydrogen) in its water than any comet from our own solar system.
  • It also showed only traces of carbon-13, another marker of a very old, chemically primitive origin.
  • Together those clues suggest the comet formed 10 to 12 billion years ago — well before the Sun, and not far off the age of the universe itself.
  • It likely formed in a deeply frozen, dense cloud during 'cosmic noon', when the galaxy was building stars at its fastest rate.
  • The findings were published on 22 June 2026 in the journal Nature, led by NASA Goddard astro-chemist Martin Cordiner.
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What Did JWST Discover About 3I/ATLAS?

Back in March we wrote about 3I/ATLAS, the third interstellar comet ever found, and the strange alien chemistry it was carrying through our solar system. At the time the headline was its water and its alcohol. Now the James Webb Space Telescope has gone a step further, and the new result is even bigger: this comet may be one of the oldest objects we have ever measured.

As 3I/ATLAS began pulling away from the Sun in December 2025, freshly warmed from its closest pass, astronomers got approval to interrupt Webb's planned schedule and point its NIRSpec (Near-Infrared Spectrograph) instrument at it. The comet's ancient ice had boiled off into a bright cloud of gas, which is exactly what you want for reading chemistry. Webb measured the ratios of carbon and hydrogen isotopes in that gas, and the numbers came back unlike anything seen in a comet before.

The findings were published on 22 June 2026 in the journal Nature, in a study led by astro-chemist Martin Cordiner of NASA's Goddard Space Flight Center. "This was a unique opportunity to study an ancient object from the distant galaxy, probably pre-dating our Sun and solar system," Cordiner said.

Artist's impression of interstellar comet 3I/ATLAS with a glowing coma of gas streaming from its icy nucleus as it moves away from the Sun, observed by the James Webb Space Telescope
As 3I/ATLAS pulled away from the Sun, its ice boiled into a bright coma of gas — the perfect target for Webb's NIRSpec to read its chemistry. Artist's impression.

How Old Is Comet 3I/ATLAS?

The research team estimates 3I/ATLAS could have formed as long as 10 to 12 billion years ago. That is a number worth sitting with for a moment.

Our Sun and everything in our solar system formed about 4.5 billion years ago. The universe itself is roughly 13.8 billion years old. So if these estimates hold, 3I/ATLAS predates the Sun by something like seven or eight billion years, and it has been drifting between the stars for almost the entire history of the galaxy. It is, in effect, a frozen sample from a time when the Milky Way was still young.

This is not a direct measurement, like reading tree rings. Nobody can put an age stamp on a comet. Instead the age comes from its chemistry, and specifically from two isotope clues that both point in the same direction: a very old, very cold beginning.

What Is Deuterium, and Why Does It Matter?

The first clue is deuterium. Deuterium is a heavier version of hydrogen with an extra neutron in its nucleus, which is why it is often called heavy hydrogen. When deuterium takes the place of ordinary hydrogen inside a water molecule, you get what is known as heavy water.

The ratio of deuterium to ordinary hydrogen in a comet's ice is one of the most reliable fingerprints astronomers have. It records the temperature and conditions of the place where that ice first froze, billions of years ago, and it tends to stay locked in unless the ice is later warmed and reprocessed.

Webb measured roughly 30 times more deuterium in the water of 3I/ATLAS than is found in any comet from our own solar system. That is an enormous gap. It tells scientists the comet's water froze in an extraordinarily cold environment and was then left alone — exposed to plenty of radiation but never to the long-term warmth that would have converted its heavy-water ice into the more familiar kind we have on Earth. In other words, it has been kept in deep freeze, chemically untouched, since it formed.

Chart comparing heavy carbon and heavy hydrogen ratios in solar system comets versus interstellar comet 3I/ATLAS, showing 3I/ATLAS as a clear outlier on both scales
On both heavy carbon and heavy hydrogen, 3I/ATLAS sits far outside the cluster of solar system comets — the signature of a very different, much older birthplace. Chart: WatchTheStars, based on data from Cordiner et al. (2026) / NASA.

The Carbon Clue

The second clue comes from carbon. Webb found that 3I/ATLAS contains only traces of carbon-13, the heavier form of carbon, compared with ordinary carbon-12.

This matters because of how the galaxy enriches itself over time. Heavier isotopes like carbon-13 are forged and scattered by generations of stars as they live and die. The longer a galaxy has been making and recycling stars, the more carbon-13 ends up in the gas that later forms new stars and planets. Our Sun, which formed relatively recently at 4.5 billion years old, carries a healthy amount of it.

A comet with almost no carbon-13 must have formed when the galaxy was still chemically young, before many generations of stars had a chance to seed it with heavier elements. That fits neatly with the deuterium result. Two independent isotope clues, both saying the same thing: this object is very, very old.

What 'Cosmic Noon' Means

The team places the comet's likely birth during a period astronomers call "cosmic noon" — the stretch of cosmic history, several billion years after the Big Bang, when galaxies were forming stars at their highest rate. If midday is when the Sun is at its peak, cosmic noon is when the universe was at its busiest building stars.

3I/ATLAS probably took shape in a cold, dense cloud of gas and dust somewhere in that early, fast-growing galaxy, around a star we will never identify. The abundance of heavy water tells us it spent its formative years deeply frozen, and it has carried that frozen chemistry across the galaxy ever since. When it dropped through our solar system, it brought a near-perfectly preserved sample of conditions from the dawn of star formation straight to Webb's instruments.

Artist's impression of the young Milky Way during cosmic noon, glowing with intense star formation, where ancient comet 3I/ATLAS may have formed in a cold dense cloud
During "cosmic noon" the young galaxy was forming stars at its fastest rate. 3I/ATLAS likely froze together in a cold, dense cloud during this era — and has been drifting ever since. Artist's impression.

How This Builds on the Earlier 3I/ATLAS Findings

If you read our March piece on 3I/ATLAS, some of this will sound familiar — and that is the point. Earlier observations had already flagged that this comet's water carried an unusual deuterium ratio, a few times higher than Earth's oceans, alongside its strange load of methanol and water vapour. Those were the first hints that 3I/ATLAS had formed somewhere very different from home.

What the new Webb study does is sharpen that hint into a much harder claim. With NIRSpec able to measure the isotopes far more precisely, and with the carbon-13 data added alongside the deuterium, the picture has shifted from "this formed somewhere unusual" to "this formed at a specific, astonishingly early moment in the galaxy's life." It is a good example of how science tightens over time: the same object, observed again with the right instrument at the right moment, gives up a far deeper part of its story.

A separate study using the European Southern Observatory's Very Large Telescope, led by astronomer Cyrielle Opitom of the University of Edinburgh, looked at the comet's carbon and nitrogen through its cyanide gas, and supports the same broad conclusion.

Why It Matters for the Search for Life

It is easy to file "very old comet" under interesting trivia, but the researchers are after something larger. Comets like this are carrying the raw chemical ingredients — water, carbon compounds, the building blocks of organic chemistry — that, in our own solar system, eventually fed into the story of life on Earth.

"So far, we know of only one place in the vast cosmos where chemical ingredients led to life — our solar system, our Earth," said Stefanie Milam of NASA Goddard, a co-author of the study. "Analysis of these interstellar objects is a major step towards learning how common, or uncommon, the conditions for the evolution of life are in the universe."

Finding those ingredients already assembled in an object that formed near the dawn of the galaxy suggests the chemistry that matters for life has been in place for a very long time, and in places utterly unlike our own corner of space.

Where Is 3I/ATLAS Now?

Sadly for anyone hoping to point a telescope at it, the show is essentially over. 3I/ATLAS made its closest pass of the Sun on 30 October 2025 and its closest approach to Earth on 19 December 2025, and it is now climbing back out of the solar system on a one-way hyperbolic path. It will never return. By now it has faded well beyond the reach of backyard telescopes, and within a few years it will be too faint for even the largest observatories on the ground.

The June 2026 results came from data Webb gathered as the comet was already moving away from us, not from a fresh sighting. In a sense that makes them more remarkable: a brief visitor that is already gone has left behind a chemical message from the early galaxy, and we are still reading it. Three interstellar comets in, the lesson keeps repeating — the universe sends samples, and each one we manage to catch tells us we know less than we thought, and that there is far more out there to find.


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Frequently Asked Questions

New James Webb Space Telescope observations suggest 3I/ATLAS could have formed as long as 10 to 12 billion years ago. That makes it far older than the Sun, which formed about 4.5 billion years ago, and nearly as old as the universe itself, which is roughly 13.8 billion years old. The estimate comes from the comet's chemistry rather than direct dating: its very high deuterium levels and very low carbon-13 content both point to a primitive, ancient origin early in the galaxy's history.
Using its NIRSpec (Near-Infrared Spectrograph) instrument, Webb measured the chemical make-up of 3I/ATLAS as it moved away from the Sun in December 2025. It found about 30 times more deuterium, a heavy form of hydrogen, locked into the comet's water than is seen in any comet from our solar system. It also detected only traces of carbon-13 compared with ordinary carbon-12. Both signatures indicate the comet formed in an extremely cold environment very early in the Milky Way's history. The results were published in Nature on 22 June 2026.
Deuterium is a heavy isotope of hydrogen with an extra neutron, sometimes called heavy hydrogen. When it takes the place of ordinary hydrogen in water, the result is 'heavy water'. The ratio of deuterium to ordinary hydrogen in a comet's ice records the temperature and conditions where that ice first formed. 3I/ATLAS holds roughly 30 times more deuterium than solar system comets, which tells scientists it froze in an exceptionally cold, ancient setting and was never warmed enough afterward to reset that chemistry.
No, not for amateur observers. 3I/ATLAS made its closest pass of the Sun on 30 October 2025 and its closest approach to Earth on 19 December 2025, then began heading back out of the solar system on a one-way hyperbolic path. By mid-2026 it has faded far beyond the reach of backyard telescopes, and within a few years it will be too faint for even the largest ground-based observatories. The June 2026 findings came from data Webb gathered as the comet moved away from the Sun, not from a new sighting.

Ian Clayton

About Ian Clayton

Amateur astronomer and founder of WatchTheStars.co.uk, dedicated to helping others explore the wonders of our universe.

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