3I/ATLAS: An Interstellar Comet Passes Through Our Solar System
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Interstellar Comet 3I/ATLAS (C/2025 N1): Increased Activity, Refined Orbit, and Rumor Clarifications

Originally published July 3, 2025 — updated October 5, 2025

Since its discovery by the ATLAS telescope network on July 1, the interstellar comet 3I/ATLAS has continued to captivate the scientific community. As it approaches its closest passage to the Sun—expected between October 29 and 30, 2025—observations from NASA, ESA, the Gran Telescopio Canarias (GTC), and the Gemini South telescope have refined our understanding of this visitor from another star system.

A Better-Defined Trajectory

The latest data published by NASA’s Jet Propulsion Laboratory (JPL) confirm the interstellar nature of 3I/ATLAS. Its hyperbolic orbit, with an eccentricity now estimated at 6.1 ± 0.01, clearly indicates that it will not return to our Solar System after its passage. The comet is currently traveling at about 57 km/s relative to the Sun and will reach its perihelion at 1.36 astronomical units, roughly the average distance between the Sun and Mars.

Animation showing the trajectory of the interstellar comet 3I/ATLAS (C/2025 N1) crossing the inner Solar System, with the orbits of Venus, Earth, Mars, and Jupiter.
Visualization of the interstellar comet 3I/ATLAS (C/2025 N1) traveling through the inner Solar System. Its hyperbolic path confirms that it originates from beyond our Solar System and will not return after its passage near the Sun in late October 2025. Credit: NASA/JPL-Caltech

Contrary to recent speculation, no deviation from its trajectory has been detected. Radar and optical measurements confirm that the comet continues on its course without any significant change in direction and will not come closer than 1.8 AU from Earth.

Increasingly Active Cometary Behavior

As 3I/ATLAS draws nearer to the Sun, its activity is intensifying. The newly operational NASA SPHEREx space telescope has detected strong emissions of carbon dioxide (CO₂) and cyanogen (CN) — two gases commonly observed in “classical” comets. Infrared spectra captured by SPHEREx suggest that the comet’s surface still contains volatile ices capable of sublimating despite billions of years of exposure to interstellar radiation.

Infrared image from NASA’s SPHEREx showing comet 3I/ATLAS marked by a green cross among a dense star field, highlighting CO₂ emission around 4.1 microns.
Infrared image of interstellar comet 3I/ATLAS (C/2025 N1) captured by NASA’s SPHEREx mission at a wavelength of 4.121 microns. The comet, marked by a green cross, shows a strong emission of carbon dioxide (CO₂), revealing the presence of volatile ices on its surface despite billions of years of interstellar exposure. Credit: NASA/JPL-Caltech

Observations from the Hubble Space Telescope have helped estimate the size of 3I/ATLAS’s solid nucleus. Based on NASA’s photometric data, the maximum diameter is around 5.6 kilometers, though the actual size could be much smaller — down to about 300 meters — depending on the assumed surface reflectivity (albedo).

Hubble Space Telescope image of interstellar comet 3I/ATLAS showing a bright blue core and a faint dust halo, with streaked background stars.
Image of interstellar comet 3I/ATLAS (C/2025 N1) captured by the Hubble Space Telescope on July 21, 2025, using the Wide Field Camera 3 with filter F350LP. The comet’s icy nucleus appears surrounded by a faint “tear-shaped” dust halo. The background stars are seen as streaks because Hubble tracked the comet’s motion during the exposure. Credit: NASA / ESA / David Jewitt / STScI

Addressing “Alien Spacecraft” Rumors

I didn’t think I’d have to write such a paragraph about this visitor, but clarification is needed. Several media outlets have echoed claims of “unusual behavior,” even comparing 3I/ATLAS to ʻOumuamua, discovered in 2017. The excitement grew after astrophysicist Avi Loeb published a paper briefly — and purely speculatively — considering a possible artificial origin if certain non-gravitational accelerations were confirmed.

However, the currently available data do not support any of these extraordinary hypotheses. NASA, ESA, and multiple independent observatories have officially confirmed that 3I/ATLAS is a natural object, whose dynamics and composition are perfectly consistent with those of an interstellar comet. No abnormal radio emissions or unexplained accelerations have been detected.

A Unique Witness to the Interstellar Medium

Researchers now regard 3I/ATLAS as the first interstellar comet observed with such a high level of detail. Its chemical composition—dominated by CO₂ and carbon-rich dust—suggests that it originated from a planetary system formed in an environment abundant in volatile ices. Ongoing comparisons with 2I/Borisov will help scientists determine how the chemistry of the interstellar medium influences comet and planet formation.

Beyond speculation, 3I/ATLAS represents a remarkable scientific opportunity: to observe an unaltered fragment of another star system, carrying clues about the diversity of worlds that populate our galaxy.

Source

Find the latest updates on NASA’s website here.

Article published on July 4, 2025

3I/ATLAS: An Interstellar Comet Passes Through Our Solar System

Interstellar objects—those originating from beyond our Solar System—have captivated astronomers and the public alike since the first detection of ʻOumuamua in 2017, followed by comet 2I/Borisov in 2019. Today, a third such visitor has been confirmed: the interstellar comet 3I/ATLAS (C/2025 N1) is currently traveling through our cosmic neighborhood, offering a rare opportunity to deepen our understanding of the universe beyond our Sun.

Recent Discovery and Rapid Confirmation

Comet 3I/ATLAS was discovered on July 1, 2025, by the ATLAS telescope network based in Río Hurtado, Chile. Its highly hyperbolic orbit—with an eccentricity close to 6—quickly confirmed its origin outside our Solar System. By analyzing archival images, astronomers were able to trace its path back to June 14, reinforcing the certainty that this object is indeed a celestial body from another star system.

ESA observes interstellar comet 3I/ATLAS
The comet is only the third of its kind ever observed, following the famous 1I/ʻOumuamua in 2017 and 2I/Borisov in 2019. It was first spotted on 1 July 2025 by the Asteroid Terrestrial-impact Last Alert System (ATLAS) telescope in Río Hurtado, Chile. Its unusual trajectory immediately raised suspicions that it originated from interstellar space. This was later confirmed by astronomers around the world, and the object was given its formal designation: 3I/ATLAS, indicating its status as the third known interstellar object. As of 3 July, 3I/ATLAS is approximately 670 million kilometres from the Sun and will make its closest approach in late October 2025, passing just inside the orbit of Mars. It is thought to be up to 20 kilometres wide and is travelling roughly 60 km/s relative to the Sun. It poses no danger to Earth, coming no closer than 240 million kilometres – over 1.5 times the distance between Earth and the Sun. Credit: ESA / Las Cumbres Observatory

Fascinating Characteristics of 3I/ATLAS

This interstellar comet stands out with an extraordinary velocity of about 60 km/s, surpassing the speeds recorded by its predecessors. Its active nucleus is estimated to measure between a few kilometers and up to twenty kilometers in diameter. Unlike ʻOumuamua, 3I/ATLAS displays a visible coma (or « hair ») and a small tail—typical cometary features—though its observed activity remains moderate.

This diagram shows the path of the interstellar comet 3I/ATLAS
This diagram shows the path of the interstellar comet 3I/ATLAS as it passes through the solar system. It will be at its closest approach to the Sun in October. Credit: NASA/JPL-Caltech

ESA Takes the Lead

Upon the detection of 3I/ATLAS, the European Space Agency’s Planetary Defence Office swiftly activated its automated monitoring systems. Through rapid analysis and archival research (so-called « precovery »), ESA confirmed the comet’s interstellar origin with high precision and ruled out any threat to Earth.

Origin and Trajectory

According to initial analyses, 3I/ATLAS likely originates from the distant regions of our galaxy, probably coming from the direction of the constellation Sagittarius. Currently located about 4.5 AU (approximately 670 million kilometers) from the Sun, it is expected to reach its closest point to the Sun—known as perihelion—between October 29 and 30, 2025, at a distance of around 1.38 AU. At no point will it approach closer than 1.6 AU (about 240 million kilometers) from Earth, ensuring that it poses no threat to our planet.

An Exceptional Scientific Opportunity

The arrival of 3I/ATLAS is currently mobilizing international teams of astronomers. NASA, the European Space Agency (ESA), the Gran Telescopio Canarias (GTC), and the Zwicky Transient Facility (ZTF), among others, are conducting extensive observations. This unprecedented effort aims to better understand the chemical composition, physical characteristics, and precise origin of this object from another star. Comparing its properties with those of 2I/Borisov and ʻOumuamua may yield valuable insights into the formation and evolution of planetary systems across our galaxy.

The discovery of 3I/ATLAS reinforces the idea that interstellar objects may not be as rare as previously thought. This comet offers a unique window into the diversity of extrasolar matter, helping us better understand not only the origin of our own Solar System but also the astonishing variety of potential worlds scattered throughout our galaxy. As we eagerly await its perihelion passage at the end of October, 3I/ATLAS has already entered the annals of astronomical history, promising to unveil key secrets about the distant worlds that surround us.

Sources

Find a NASA article published on July 1, 2025 [here], and an ESA article published on July 3, 2025 [here].