Sequential Fragmentation of C/2025 K1 (ATLAS) After Its Near-Sun Passage
Dennis Bodewits, John W. Noonan, Michael S. P. Kelley, Carrie E. Holt, Tim A. Lister, Helen Usher, Colin Snodgrass, Bjorn Davidsson, and Sarah Greenstreet

TL;DR
This study documents the rapid fragmentation of comet C/2025 K1 (ATLAS) near perihelion, revealing hierarchical breakup sequences, timing of outbursts, and insights into the thermal and structural evolution of the nucleus.
Contribution
First high-resolution imaging of a comet nucleus during early fragmentation, linking outbursts to physical disintegration processes and rotational instability.
Findings
Hierarchical fragmentation sequence observed
Breakup events preceded outbursts by 1-3 days
Rapid warming of interior material after exposure
Abstract
Comet C/2025 K1 (ATLAS) reached perihelion at 0.33 au on 2025 October 8. Daily monitoring by the LCO Outbursting Objects Key Project revealed a major activity increase between November 2 and 4, accompanied by rapid changes in coma morphology. Serendipitous HST/STIS acquisition images obtained on November 8-10 captured the comet only days after this event and resolved five fragments, providing an early high-resolution view of a nucleus in the process of disruption. Fragment motions and morphologies indicate a hierarchical fragmentation sequence, including a slow secondary split of fragment II. Back extrapolation shows that both the primary and secondary breakups preceded their associated photometric outbursts by roughly one to three days. This consistent lag, together with the appearance of thin, short-lived arclets around fragment I in the first HST epoch, suggests that freshly exposed…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstro and Planetary Science · Astrophysics and Star Formation Studies · High-pressure geophysics and materials
