Astronomers at Guangxi University in China may have observed the birth of a strange star - a theoretical, compact star that is extremely dense.
Strange stars are composed of up, down, and strange quarks, and could be more stable than traditional neutron stars.
The researchers found evidence in a gamma-ray burst known as GRB 240529A, which exhibited emission episodes representing different phases of collapse, potentially supporting the theory of a strange star's birth.
Further testing and confirmation by other researchers is needed to solidify the findings and advance experimental astrophysics.