Solar System Comet C/2025 K1 Breaks Up Unexpectedly | Hubble Space Telescope
This series of Hubble Space Telescope images of the fragmenting comet C/2025 K1 (ATLAS), or K1 for short, was taken over the course of three consecutive days: November 8, 9, and 10, 2025. Captured by Hubble’s Space Telescope Imaging Spectrograph (STIS) instrument, the sequence shows the progressive disintegration of the comet over this brief period. This is the first time Hubble has witnessed a comet so early in the process of breaking up.
This diagram shows the path the long-period comet C/2025 K1 (ATLAS), or K1 for short, took as it swung past the Sun and began its journey out of the Solar System. On November 10, 2025, Hubble captured the inset image of the fragmenting comet. Hubble took this image just a month after K1’s closest approach to the Sun, called perihelion.
Image Description: Diagram showing comet K1’s path. With the Sun near middle right of image, truncated nearly circular orbits of Mercury, Venus, Earth, and Mars appear against black background. K1’s tight parabolic curve, marked by solid, light blue curving line, illustrates how K1 swooped toward the Sun from above. It curved around the Sun, coming closest inside Mercury’s orbit, and continued its outbound journey.
Comet K1, whose full name is Comet C/2025 K1 (ATLAS), had just passed its closest approach to the Sun and was heading out of the Solar System. Although it had been intact just days before, K1 fragmented into at least four pieces while the NASA/European Space Agency Hubble Space Telescope was watching. The odds of that happening while Hubble viewed the comet are extraordinarily miniscule.
C/2025 K1 (ATLAS) is a non-periodic comet first seen in May 2025. It is one of many comets discovered by the Asteroid Terrestrial-impact Last Alert System (ATLAS) funded by NASA. The comet is dynamically new, having come directly from the Oort cloud. With perihelion only 0.33 AU (49 million km; 31 million mi) from the Sun, the comet was not expected to survive perihelion passage, but it did and was recovered on October 18, 2025. The comet has since broken into multiple fragments and fragments A+B+C+D may be ejected from the Solar System.
Comet K1, whose full name is Comet C/2025 K1 (ATLAS)—not to be confused with interstellar comet 3I/ATLAS—was not the original target of a recent Hubble study. The findings were published today in the journal Icarus.
“Sometimes the best science happens by accident,” said co-investigator John Noonan, a research professor in the Department of Physics at Auburn University in Alabama in the United States. “This comet got observed because our original comet was not viewable due to some new technical constraints after we won our proposal. We had to find a new target—and right when we observed it, it happened to break apart, which is the slimmest of slim chances.”
Noonan did not know K1 was fragmenting until he viewed the images the day after Hubble took them. “While I was taking an initial look at the data, I saw that there were four comets in those images when we only proposed to look at one,” said Noonan. “So we knew this was something really, really special.”
This is an experiment the researchers always wanted to do with Hubble. They had proposed many Hubble observations to catch a comet breaking up. Unfortunately, these are very difficult to schedule, and they were never successful.
“The irony is now we’re just studying a regular comet and it crumbles in front of our eyes,” said principal investigator Dennis Bodewits, also a professor in Auburn University’s Department of Physics.
“Comets are leftovers of the era of Solar System formation, so they’re made of ‘old stuff’—the primordial materials that made our Solar System,” explained Bodewits. “But they are not pristine—they’ve been heated, they’ve been irradiated by the Sun and by cosmic rays. So, when looking at a comet’s composition, the question that we always have is, ‘Is this a primitive property or is this due to evolution?’ By cracking open a comet, you can see the ancient material that has not been processed.”
Hubble caught K1 fragmenting into at least four pieces, each with a distinct coma, the fuzzy envelope of gas and dust that surrounds a comet’s icy nucleus. Hubble cleanly resolved the fragments, but to ground-based telescopes, at they time they only appeared as barely distinguishable blobs.
Hubble’s images were taken just a month after K1’s closest approach to the Sun, called perihelion. The comet's perihelion was inside Mercury’s orbit, about one-third the distance of the Earth from the Sun. During perihelion, a comet experiences its most intense heating and maximum stress. Just past perihelion is when long-period comets like K1 tend to fall apart.
Before it fragmented, K1 was likely a bit larger than an average comet, probably about 8 kilometres across. The team estimates the comet began to disintegrate eight days before Hubble viewed it. Hubble took three 20-second images, one on each day from November 8 through November 10, 2025. As it watched the comet, one of K1’s smaller pieces also broke up.
Because Hubble’s sharp vision can distinguish extremely fine details, the team could trace the history of the fragments back to when they were one piece. That allowed them to reconstruct the timeline. However, in doing so, they uncovered a mystery. Why was there a delay between when the comet broke up and when bright outbursts were seen from the ground? When the comet fragmented and exposed fresh ice, why did it not brighten almost instantaneously?
The team has theories. Most of a comet’s brightness is sunlight reflected off of dust grains. When a comet cracks open, it reveals pure ice. Maybe a layer of dry dust needs to form over the pure ice and then blow off. Or maybe heat needs to get below the surface, build up pressure, and then eject an expanding shell of dust.
“Never before has Hubble caught a fragmenting comet this close to when it actually fell apart. Most of the time, it’s a few weeks to a month later. And in this case, we were able to see it just days after,” said Noonan. “This is telling us something very important about the physics of what’s happening at the comet’s surface. We may be seeing the timescale it takes to form a substantial dust layer that can then be ejected by the gas.”
The team is looking forward to finishing the analysis of the gases to come from the comet. Already, ground-based analysis shows that K1 is chemically very strange—it is significantly depleted in carbon, compared with other comets. Spectroscopic analysis from Hubble’s Space Telescope Imaging Spectrograph (STIS) and Cosmic Origins Spectrograph (COS) instruments is likely to reveal much more about the composition of K1 and the very origins of our Solar System.
The comet K1 is now a collection of fragments about 400 million kilometers from Earth. Located in the constellation Pisces, it is heading out of the Solar System, not likely to ever return. Astronomers see that long-period comets, such as K1, are more likely to fragment than their short-period cousins, such as 67P/Churyumov-Gerasimenko that was visited by the European Space Agency's Rosetta Mission, but it is not known why. Launching towards the end of the decade, the European Space Agency's Comet Interceptor will be the first mission to visit a long-period comet. “Hubble’s chance observation of K1 will help us understand why some long-period comets split apart and give us a first view of their interiors,” said co-author Prof. Colin Snodgrass of the University of Edinburgh in Scotland and an Interdisciplinary Scientist for the Comet Interceptor Mission. “These new results will complement the detailed view of a long-period comet that we will obtain from Comet Interceptor, as well as helping astronomers to select the mission’s target.”
Image Credit: NASA, ESA, D. Bodewits (Auburn) Image Processing: J. DePasquale (STScI)
Release Date: March 18, 2026
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