Scientists revealed the strange chemistry of a rare comet from far beyond our solar system.

Scientists revealed the strange chemistry of a rare comet from far beyond our solar system.


July 2, 2026 | Sammy Tran

Scientists revealed the strange chemistry of a rare comet from far beyond our solar system.


A Visitor From Afar

The discovery of 3I/ATLAS gave astronomers a rare opportunity to study material that formed around another star. As only the third confirmed interstellar object ever observed passing through our Solar System, it quickly became one of the most important astronomical discoveries of 2025 and 2026.

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Discovery Of 3I

3I/ATLAS was discovered on July 1, 2025, by the Asteroid Terrestrial-impact Last Alert System telescope in Río Hurtado, Chile. It was initially designated A11pl3Z before receiving the official comet designation C/2025 N1 (ATLAS) and later the interstellar designation 3I/ATLAS.

A deep image of interstellar Comet 3I/ATLAS captured by the Gemini Multi-Object Spectrograph (GMOS) on Gemini North on Maunakea in Hawai‘i, one half of the International Gemini Observatory, partly funded by the U.S. National Science Foundation (NSF) and oInternational Gemini Observatory/NOIRLab/NSF/AURA/B. Bolin Image Processing: J. Miller & M. Rodriguez (International Gemini Observatory/NSF NOIRLab), T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani (NSF NOIRLab), Wikimedia Commons

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The Third Interstellar Object

The object became the third confirmed interstellar visitor ever detected. It followed the discoveries of 1I/ʻOumuamua in 2017 and 2I/Borisov in 2019, making such detections exceptionally uncommon events in modern astronomy.

1I/ʻOumuamua as shown here imaged with the 4.2 meter William Herschel Telescope on the Canary Islands is seen as a point of light in the centre of the image. Background stars appear linear because the telescope was centred on tracking the object through 5Alan Fitzsimmons (Astrophysics Research Centre, Queen's University Belfast), Isaac Newton Group (https://www.ing.iac.es/ - Instituto de Astrofísica de Canarias) Derivative: nagualdesign, Wikimedia Commons

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Evidence Of Origin

Astronomers quickly realized that 3I/ATLAS was not gravitationally bound to the Sun. Its trajectory showed that it originated from outside the Solar System and would eventually leave again after passing through the inner planetary region.

NASA’s Hubble Space Telescope reobserved interstellar comet 3I/ATLAS Nov. 30, with its Wide Field Camera 3 instrument. At the time, the comet was about 178 million miles (286 million kilometers) from Earth. Hubble tracked the comet as it moved across the NASA, ESA, STScI, D. Jewitt (UCLA), M.-T. Hui (Shanghai Astronomical Observatory). Image Processing: J. DePasquale (STScI), Wikimedia Commons

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A Large Comet

Early observations suggested that 3I/ATLAS was significantly larger than previous interstellar visitors. Estimates indicated a nucleus roughly 20 kilometers across, although later studies suggested the solid core itself could be smaller and obscured by surrounding material.

Two-frame animation of interstellar comet 3I/ATLAS (gray fuzzy blob, centered), seen moving across a field of stars in Hubble Space Telescope images taken on 21 July 2025 16:29 and 16:32 UTC. Each frame is a 40-second exposure taken with the WFC3 camera'sImages taken by David Jewitt/NASA/ESA/Space Telescope Science Institute (STScI), processed by Nrco0e., Wikimedia Commons

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Extremely Active Appearance

The comet displayed a bright coma (halo around it's head) and tail as it approached the Sun. This activity resulted from volatile materials vaporizing and carrying dust away from the nucleus, creating the spectacular appearance observed by astronomers.

This striking image from the science camera on ESA’s Jupiter Icy Moons Explorer (Juice) shows interstellar comet 3I/ATLAS spewing dust and gas. The tiny nucleus of the comet (not visible) is surrounded by a bright halo of gas known as the coma. A long taiESA/Juice/JANUS, Wikimedia Commons

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Speed Through Space

Before entering the Solar System, 3I/ATLAS traveled through interstellar space at approximately 57 kilometers per second relative to the Sun. Its high velocity was one of the clearest indications that it originated around another star.

This is a Hubble Space telescope image of the interstellar comet 3I/ATLAS. Hubble photographed the comet on 21 July 2025, when the comet was 365 million kilometres from Earth. Hubble shows that the comet has a teardrop-shaped cocoon of dust coming off itsNASA, ESA, D. Jewitt (UCLA); Image Processing: J. DePasquale (STScI), Wikimedia Commons

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Approaching The Sun

The comet's closest approach to the Sun was predicted to occur on October 29, 2025. At perihelion it would pass inside the orbit of Mars, reaching a distance of about 1.36 astronomical units from the Sun.

Interstellar comet 3I/ATLAS photographed by the 8.2-meter Gemini South telescope on 27 August 2025 during 23:55-23:57 UTC. This is a median stack of two 30-second exposures; the combination of these images helps make the comet appear more clearly by reducImages taken by Elena Sabbi, Brian Lemaux, Siyi Xu, Leilani Lozi, and Manuel Paredes as part of program GS-2025B-DD-103,

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Why It Matters

Interstellar objects provide direct samples of material formed around distant stars. Unlike meteorites and comets native to our Solar System, 3I/ATLAS offers a rare opportunity to compare the chemistry of another planetary system with our own.

Hyperbolic path of interstellar comet 3I/ATLAS (white) with orbits of other planets (labeled and colored). White dots with labels represent positions of the respective object. Data as of 3 Jul 2025.NASA/JPL-Caltech, Wikimedia Commons

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Webb Takes A Look

Scientists used NASA's James Webb Space Telescope to investigate the comet's composition. Webb's infrared instruments allowed researchers to identify gases escaping from the comet as sunlight heated its icy surface.

Caption: During cryogenic testing, the mirrors will be subjected to temperatures dipping to 24 Kelvins, permitting engineers to measure in extreme detail how the shape of each mirror changes as it cools. More information: Click hereNASA/MSFC/David Higginbotham/Emmett Given, Wikimedia Commons

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Detecting Methane

The Webb observations revealed methane gas within 3I/ATLAS. According to the researchers, this was the first clear detection of methane in an interstellar comet, providing an important new clue about its chemical makeup.

NASA engineer Ernie Wright looks on as the first six flight ready James Webb Space Telescope's primary mirror segments are prepped to begin final cryogenic testing at NASA's Marshall Space Flight Center.NASA/MSFC/David Higginbotham, Wikimedia Commons

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Methane's Importance

Methane is a volatile molecule that forms under specific conditions in protoplanetary disks. Detecting it in 3I/ATLAS gave astronomers a new way to compare the environments where different planetary systems form and evolve.

Structure of methaneChristinelmiller, Wikimedia Commons

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Carbon Monoxide Discovery

The Webb team also detected carbon monoxide. Measurements indicated that carbon monoxide was approximately ten times more abundant than methane in the comet's coma, revealing an unusual balance of volatile compounds.

Electrochemical Carbon Monoxide sensor from a First Alert Smoke+CO alarm (brown cylinder).Aug wiki 1257, Wikimedia Commons

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Similar Yet Different

Researchers noted that the methane abundance was similar to levels seen in many Solar System comets. However, the much larger abundance of carbon monoxide distinguished 3I/ATLAS from many familiar comet populations.

A deep image of interstellar Comet 3I/ATLAS captured by the Gemini Multi-Object Spectrograph (GMOS) on Gemini South at Cerro Pachón in Chile, one half of the International Gemini Observatory, partly funded by the U.S. National Science Foundation (NSF) andInternational Gemini Observatory/NOIRLab/NSF/AURA/Shadow the Scientist Image Processing: J. Miller & M. Rodriguez (International Gemini Observatory/NSF NOIRLab), T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), M. Zamani (NSF NOIRLab), Wikimedia

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An Ancient Survivor

Scientists suggested that the comet likely formed in a cold outer region of its home planetary system. Such environments can preserve volatile compounds for billions of years before objects are eventually ejected into interstellar space.

A diagram showing the appearance of 3I/ATLAS's coma. Shown on the left panel is an image of 3I/ATLAS among background stars, taken by the Very Large Telescope on 4 July 2025. The image is annotated with the following:
On the bottom left corner is a scale Nrco0e, Wikimedia Commons

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Michigan Team Investigation

A separate study led by researchers at the University of Michigan examined the comet using spectroscopic observations. Their work focused on measuring the abundance of water and comparing it with other molecules released by the comet.

Built in 1908-1910, this Classical Revival-style building was designed by Donaldson and Meier to serve as the Alumni Memorial Hall for the University of Michigan, home to the university’s alumni department, which moved out of the building in 1967 due to tw_lemay, Wikimedia Commons

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Strange Water Results

The Michigan team found that water appeared surprisingly scarce compared with the comet's dust production and overall activity. This unusual relationship immediately drew attention because it differed from expectations based on many Solar System comets.

This animation shows the observations of comet 3I/ATLAS when it was discovered on July 1, 2025. The NASA-funded ATLAS survey telescope in Chile first reported that the comet originated from interstellar space.ATLAS/University of Hawaii/NASA, Wikimedia Commons

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Dust Without Water

The researchers reported that the comet was producing substantial amounts of dust while displaying relatively weak evidence of water vapor. This combination suggested that other volatile materials might be driving much of the activity.

On 3 October, ESA’s ExoMars Trace Gas Orbiter (TGO) turned its eyes towards interstellar comet 3I/ATLAS as it passed close to Mars.Together with Mars Express, ExoMars TGO had the closest view of the comet of all ESA spacecraft. It looked towards the interEuropean Space Agency, Wikimedia Commons

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Carbon-Rich Chemistry

The University of Michigan study found evidence that carbon-bearing molecules played a major role in the comet's behavior. The findings reinforced the idea that 3I/ATLAS differs chemically from many comets formed around the Sun.

Measurements of specific element varieties by Webb’s NIRSpec (Near-Infrared Spectrograph) instrument show how different the interstellar comet 3I/ATLAS is from comets originating in our own Solar System. Researchers used NIRSpec to measure carbon-13, whicNASA, ESA, CSA, M. Cordiner, L. Hustak (STScI), Wikimedia Commons

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A Different Birthplace

According to the researchers, the unusual chemical composition may reflect conditions in the distant planetary system where the comet formed. Those conditions may have favored the preservation of different volatile compounds than those common in Solar System comets.

From left to right, the graphic features: the Sun, Mercury, Earth, Moon, Mars, Ceres, Asteroid Belt, Jupiter, Saturn, Comets, Uranus, Neptune, Pluto, Makemake, Kuiper Belt Objects, Eris.NASA, Wikimedia Commons

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Two Studies Converge

Although the NASA and University of Michigan teams used different observational approaches, both studies pointed toward a chemically unusual object. Together they painted a picture of a comet rich in carbon-based volatiles and unexpectedly poor in water.

Comet 3I/ATLAS streaks across a dense star field in this image captured by the Gemini North telescope's Gemini Multi-Object Spectrograph (GMOS-N). The left panel captures the comet’s colorful trail as it moves through the Solar System. The image was compoInternational Gemini Observatory/NOIRLab/NSF/AURA/K. Meech (IfA/U. Hawaii) Image Processing: Jen Miller & Mahdi Zamani (NSF NOIRLab), Wikimedia Commons

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Expanding The Sample

Before 3I/ATLAS, astronomers had only two confirmed interstellar objects available for study. Every new visitor dramatically expands the scientific sample and improves understanding of how planetary systems form across the galaxy.

Plot of the trajectory of interstellar comet 3I/ATLAS against the stellar background from 2024 to 2026.
Made with Python using packages Starplot [1] and Skyfield [2]. Heliocentric orbital elements are from the MPC.Thunkii, Wikimedia Commons

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A Natural Messenger

Because it formed around another star, 3I/ATLAS acts as a natural messenger carrying information from a distant planetary system. Its gases, dust, and ice preserve evidence of conditions that astronomers cannot observe directly.

Webb is looking at the chemical fingerprints of interstellar comet 3I/ATLAS 🔎
Using Webb’s Mid-Infrared Instrument (MIRI), scientists have obtained the first mid-infrared chemical fingerprints of this object, which traveled to our solar system from an entJames Webb Space Telescope, Wikimedia Commons

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Lessons From 3I

The methane detected by Webb and the unusual water findings reported by the Michigan team demonstrate that planetary systems can produce comets with chemical signatures different from those commonly seen in our own Solar System.

Webb is looking at the chemical fingerprints of interstellar comet 3I/ATLAS 🔎
Using Webb’s Mid-Infrared Instrument (MIRI), scientists have obtained the first mid-infrared chemical fingerprints of this object, which traveled to our solar system from an entJames Webb Space Telescope, Wikimedia Commons

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A Rare Scientific Opportunity

As 3I/ATLAS continues its journey back into interstellar space, scientists are gathering as much data as possible. The object may not return, making these observations a unique chance to study material formed around another star.

This image shows the observation of comet 3I/ATLAS when it was discovered on July 1, 2025. The NASA-funded ATLAS survey telescope in Chile first reported that the comet originated from interstellar space.ATLAS/University of Hawaii/NASA, Wikimedia Commons

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Sources: 1, 2, 3


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