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Scientists Discover New Type of Cosmic Explosion

Published on June 22, 2026, 2:04 p.m.
Scientists Discover New Type of Cosmic Explosion

Topic: Space

Astronomers may have found a strange new kind of cosmic explosion. This event, called a superkilonova, is different from the usual supernovae and kilonovae.

When massive stars die, they explode as supernovae, scattering elements like carbon and iron across space. Another type of explosion happens when two neutron stars collide, producing even heavier elements like gold and uranium. These materials are essential for forming stars, planets, and everything we see around us.

A team led by Mansi Kasliwal from Caltech believes they may have found evidence of a second kilonova, although the situation is complex. The candidate event, named AT2025ulz, appears to be tied to a supernova that happened just hours earlier.

The first sign of this rare event appeared on August 18, 2025. LIGO detectors recorded a new gravitational-wave signal, which was quickly followed by an alert to astronomers worldwide. The signal likely came from two merging objects, and at least one of those objects seemed unusually small.

A few hours later, the Zwicky Transient Facility identified a fading red source about 1.3 billion light years away, located in the same region as the gravitational-wave signal. Roughly a dozen telescopes around the world quickly began observing the event, including the W. M. Keck Observatory and facilities connected to the GROWTH program.

Early observations showed the object fading rapidly and glowing red, similar to what was seen in the 2017 kilonova. However, the behavior of AT2025ulz soon changed. A few days after the initial flash, it brightened again, shifted to bluer light, and showed hydrogen in its spectra.

The team suggests that this unusual event could represent something entirely new, a superkilonova, meaning a kilonova triggered by a supernova. While scientists have proposed this idea before, it has never been observed.

Why It Matters

This discovery is important because it can help us understand the formation of stars and planets in distant galaxies. It also shows that there are still many mysteries to uncover in the universe.

Key Facts

  • Astronomers may have found a new type of cosmic explosion called a superkilonova.
  • The event, named AT2025ulz, appears to be tied to a supernova that happened just hours earlier.
  • LIGO detectors recorded a new gravitational-wave signal on August 18, 2025.

Key Terms

Kilonova
A type of cosmic explosion that occurs when two neutron stars collide.

Implications

This discovery is important because it can help us understand the formation of stars and planets in distant galaxies. It also shows that there are still many mysteries to uncover in the universe.


Source: https://www.sciencedaily.com/releases/2026/04/260423031532.htm

Journal Reference:

  1. Mansi M. Kasliwal, Tomás Ahumada, Robert Stein, Viraj Karambelkar, Xander J. Hall, Avinash Singh, Christoffer Fremling, Brian D. Metzger, Mattia Bulla, Vishwajeet Swain, Sarah Antier, Marion Pillas, Malte Busmann, James Freeburn, Sergey Karpov, Aleksandra Bochenek, Brendan O’Connor, Daniel A. Perley, Dalya Akl, Shreya Anand, Andrew Toivonen, Sam Rose, Theophile Jegou du Laz, Chang Liu, Kaustav Das, Sushant Sharma Chaudhary, Tyler Barna, Aditya Pawan Saikia, Igor Andreoni, Eric C. Bellm, Varun Bhalerao, S. Bradley Cenko, Michael W. Coughlin, Daniel Gruen, Daniel Kasen, Adam A. Miller, Samaya Nissanke, Antonella Palmese, Jesper Sollerman, Niharika Sravan, G.C. Anupama, Smaranika Banerjee, Sudhanshu Barway, Joshua S. Bloom, Tomás Cabrera, Tracy Chen, Chris Copperwheat, Alessandra Corsi, Richard Dekany, Nicholas Earley, Matthew Graham, Patrice Hello, George Helou, Lei Hu, Yves Kini, Ashish Mahabal, Frank Masci, Tanishk Mohan, Natalya Pletskova, Josiah Purdum, Yu-Jing Qin, Nabeel Rehemtulla, Anirudh Salgundi, Yuankun Wang. ZTF25abjmnps (AT2025ulz) and S250818k: A Candidate Superkilonova from a Subthreshold Subsolar Gravitational-wave Trigger. The Astrophysical Journal Letters, 2025; 995 (2): L59 DOI: 10.3847/2041-8213/ae2000

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