This image of interstellar comet 3I/ATLAS was taken on 18 January 2026 with the FORS2 instrument on ESO’s Very Large Telescope (VLT). It is a stack of several images spanning 14 minutes. As the comet moves on the sky, the stars appear as trails in the background. Credit: ESO/ O Hainaut. CC BY.
Astronomers have found new clues to the origin of 3I/ATLAS, suggesting the interstellar comet might be older than our Sun.
Astronomers have used the European Southern Observatory’s Very Large Telescope (ESO’s VLT) to study the composition of 3I/ATLAS, the brightest interstellar object ever seen, in detail.
By measuring specific chemical fingerprints – the first observations of this kind for a comet that formed outside the Solar System – they found that 3I/ATLAS likely originated in the outskirts of an old star system.
The findings shine new light on the formation history of this comet, indicating that it may be much older than the Sun.
‘Sort of fossils’
Interstellar comets are icy objects formed around a star other than the Sun that occasionally wander into our Solar System.
Astronomer Cyrielle Opitom, a researcher at the University of Edinburgh, said: “They are sort of fossils from a planetary formation process that happened very far away, but that we get the chance to study from much closer.”
Unprecedented brightness
3I/ATLAS is the third interstellar object ever discovered, after 1I/ʻOumuamua and 2I/Borisov.
It was found as it was approaching the Sun, spending enough time in our Solar System for astronomers to study it in detail.
While it was difficult to measure the composition of the first two interstellar objects, with astronomers unable to detect gas in the first, and the second was too faint, this was not the case for 3I/ATLAS.
Thanks to the object’s unprecedented brightness, Opitom, along with Jean Manfroid and Damien Hutsemékers of the University of Liège, were able to measure the comet’s isotopic ratios: the relative amounts of different forms of the same element.
Using the UVES instrument on ESO’s VLT, the team measured ratios of carbon and nitrogen isotopes in cyanide molecules present in the gas around the comet.
These ratios are known to be a good indicator of a comet’s origin, as they are very sensitive to the physical conditions in the formation environment and are not expected to change much as the comet travels on through space.
Aravind Krishnakumar, a researcher at the University of Liège and co-author on the new study, said: “Unlike comets from our Solar System, this interstellar visitor carries unusually high carbon and nitrogen isotopic ratios.”
‘Low-metallicity star’
A similar study led by Martin Cordiner at the NASA Goddard Space Flight Center, US, that was published late last month in Nature, found a similar isotopic ratio of carbon, as well as elevated levels of deuterium, also called heavy hydrogen.
The study used data from the James Webb Space Telescope, a joint project of the US, European and Canadian space agencies.
Overall, the findings by Opitom’s team indicate that the comet likely formed in the outer regions around an old, ‘low-metallicity’ star.
A low-metallicity star is one with few elements heavier than helium in its composition, that is thought to have formed when the Universe was much younger and less chemically rich than it is now.
The team suspects that 3I/ATLAS therefore originated around a star much older than the Sun.
Co-author Rosemary Dorsey, a researcher at the University of Helsinki, said: “3I/ATLAS is a really exciting opportunity to probe the composition of another planetary system, one that formed long before our Sun and Solar System even existed.”
Evidence from the studies by the different teams points to 3I/ATLAS being more than twice as old as the Sun.
As 3I/ATLAS moves away from the Sun and gets progressively fainter, its observations at the VLT are also nearing their end.
ESO’s upcoming Extremely Large Telescope (ELT) will allow similar measurements for future interstellar objects, including those less bright than 3I/ATLAS.
Opitom said: “The field of interstellar objects is still very new, and we do not really know what to expect. Every time a new one is discovered, we have new surprises.”
The study is published in Nature Astronomy.
