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\t\t\t\t\t\t22\/06\/2026<\/span> The third identified interstellar comet in human history has a surprising chemical makeup, raising questions as to how common, or unusual, conditions in our own Solar System may be.<\/p>\n<\/div>\n As interstellar Comet 3I\/ATLAS began moving away from the Sun in December 2025, astronomers took the opportunity to turn the powerful NASA\/ESA\/CSA James Webb Space Telescope in its direction and capture detailed measurements of its chemical components. The comet was freshly warmed from its closest pass by the Sun, and its ancient ice had been converted to a bright coma of gas ideal for observation.<\/p>\n Webb captured detailed data, including chemical ratios of carbon and deuterium, also known as heavy hydrogen, that are not found in Solar System comets. The results surprised researchers. Working backward, astronomers used the components that make up Comet 3I\/ATLAS to understand the environment in which it formed.<\/p>\n A paper detailing the findings was\u00a0published\u00a0on 22 June 2026 in the journal\u00a0Nature.<\/i><\/p>\n The comet\u2019s name comes from its status as the third confirmed interstellar comet, meaning it originated outside the Solar System, and the telescope that first spotted it, the NASA-funded ATLAS (Asteroid Terrestrial-impact Last Alert System).<\/p>\n \u201cThis was a unique opportunity to study an ancient object from the distant Galaxy, probably pre-dating our Sun and Solar System,\u201d said astro-chemist Martin Cordiner of NASA\u2019s Goddard Space Flight Center in Greenbelt, Maryland, and lead author of the study.\u00a0\u201cOn the one hand, we get direct insight into that distant time and place, and on the other, we learn something about how unusual our own Solar System may be.\u201d<\/p>\n Cordiner and the research team joined astronomers from many sub-disciplines in taking the opportunity to get a look at 3I\/ATLAS on its journey through the Solar System. They received approval to interrupt Webb\u2019s planned schedule of observations to make use of its NIRSpec (Near-Infrared Spectrograph) instrument to study the comet.<\/p>\n NIRSpec revealed exceptionally high levels of deuterium, about 30 times more than seen in Solar System comets. This implies that 3I\/ATLAS may have originated in a very cold system much earlier in the history of our galaxy. During its formation, the material that became incorporated into 3I\/ATLAS was likely exposed to plenty of radiation, but not any long-term warmth that would have reprocessed its ‘heavy water’ ice, with deuterium, into the type of H2O ice we are familiar with on Earth.<\/p>\n Additionally, NIRSpec showed only traces of carbon-13 compared to lighter-weight carbon-12. This also points to a very old origin for 3I\/ATLAS, as stellar systems become enriched with carbon-13 over time as generations of stars are born and die in the galaxy. That is why there are higher levels of carbon-13 in our system, around our Sun, which formed relatively recently, 4.5 billion years ago.<\/p>\n The research team estimates that 3I\/ATLAS could have formed as long as 10 to 12 billion years ago, during the Universe\u2019s ‘cosmic noon,’ when star formation was at its height. Its young origin system was likely ensconced in a relatively cold, dense cloud. The abundance of heavy water shows that 3I\/ATLAS spent its formative years in a deeply frozen state.<\/p>\n<\/p><\/div>\n A\u00a0separate study\u00a0using the European Southern Observatory’s Very Large Telescope, led by astronomer Cyrielle Opitom of the University of Edinburgh, complements Webb\u2019s findings with an analysis of 3I\/ATLAS\u2019s carbon and nitrogen varieties in the form of the chemical cyanide.<\/p>\n \u201cFor us as scientists, finding these rare isotopes is fascinating, but the bigger picture here is looking at the possibilities of prebiotic chemistry elsewhere in the galaxy,\u201d\u00a0said Stefanie Milam of NASA Goddard and co-author of the study with Cordiner.\u00a0\u201cSo far, we know of only one place in the vast cosmos where chemical ingredients led to life \u2013 our Solar System, our Earth. 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.\u201d<\/p>\n<\/p><\/div>\n \nMore information<\/b> Webb is an international partnership between NASA, ESA and the Canadian Space Agency (CSA).<\/p>\n Release on esawebb.org<\/p>\n Science paper<\/p>\n Release on NASA website<\/p>\n \u00a0<\/p>\n \nContact:<\/b>
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Webb\u00a0is the largest, most powerful telescope ever launched into space. Under an international collaboration agreement, ESA provided the telescope\u2019s launch service, using the Ariane 5 launch vehicle. Working with partners, ESA was responsible for the development and qualification of Ariane 5 adaptations for the Webb mission and for the procurement of the launch service by Arianespace. ESA also provided the workhorse spectrograph\u00a0NIRSpec\u00a0and 50% of the mid-infrared instrument\u00a0MIRI, which was designed and built by a consortium of nationally funded European Institutes (The MIRI European Consortium) in partnership with JPL and the University of Arizona.<\/p>\n
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