This article has been reviewed according to Science X's editorial process and policies. Editors have highlighted the following attributes while ensuring the content's credibility: A star's explosive demise has added a shiny new feature to NGC 1433, a barred spiral galaxy approximately 50 million light-years away in the southern constellation Horologium (the Pendulum Clock). New images of supernova SN 2026ahvu from the U.S.
Department of Energy–fabricated Dark Energy Camera (DECam) and the Gemini South telescope capture the explosion against its galactic surroundings, recording an event that is changing in appearance from night to night. DECam is mounted on the U.S. National Science Foundation Víctor M.
Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory (CTIO) in Chile, a program of NSF NOIRLab. Gemini South is one half of the International Gemini Observatory, an international collaboration led by the NSF, in partnership with Canada, Chile, Brazil, Argentina, and the Republic of Korea, and operated by NSF NOIRLab. The Asteroid Terrestrial-impact Last Alert System (ATLAS) discovered the object on Nov. 2, 2026.
Initially designated AT 2026ahvu, it was subsequently confirmed through spectroscopy to be a young Type Ia supernova—an explosion of a white dwarf that has accreted matter from a close companion star—and received the designation SN 2026ahvu. At discovery, its apparent magnitude was approximately 17; within days, observations reported it at magnitude 13.5. The supernova, visible in the image above to the right and slightly below the galaxy's center, is expected to reach a maximum brightness of magnitude 10.5–12.1 between Nov. 18 and 23.
Its discovery well before reaching peak brightness, combined with its relative proximity, gives astronomers the rare and valuable opportunity to witness the early development of the explosion and gather evidence that can quickly disappear as the expanding debris evolves. This is one of the nearest Type Ia supernovae observed since SN 2011fe was discovered in the Pinwheel Galaxy (Messier 101) in 2011. Type Ia supernovae arise from the thermonuclear destruction of white dwarfs, the dense remnants of stars like our sun.
Although astronomers use these explosions to measure cosmic distances, important questions remain about the stellar systems that produce them and precisely how they ignite. Observations during the earliest stages can help distinguish between possible explosion scenarios and search for signs of interaction with a companion star or surrounding material. DECam also captured images of NGC 1433 before the explosion during observations for the Dark Energy Survey (DES), a survey led by DOE's Fermi National Accelerator Laboratory, conducted from 2013 to 2019, to investigate the nature of dark energy.
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