Astronomers Capture 30-Solar-Mass Star's Death From Start to Finish

3 articles · Updated · Sight Magazine · Aug 10

SN 2026gzf gave astronomers a rare full view of a supernova, from a brief X-ray shock breakout in March through nearly three months of follow-up before the site passed behind the sun.
China's Einstein Probe first caught the flare on March 21, only the first observed shock breakout since 2008, letting researchers trace how the collapsing star's shock wave tore through its surface.
The star lay about 500 million light-years away and was estimated at roughly 30 times the sun's mass; the blast likely left a black hole and hurled material at a bit more than 10% of light speed.
That broad-lined Type Ic explosion showed traits often linked to gamma-ray bursts but produced none, pointing to a possible 'choked' jet trapped by the star or dense surrounding material.
Researchers said the event marks the first supernova of its type seen without a gamma-ray burst, suggesting the most massive stars can die in more ways than previously thought.