Astronomers Predict V Sagittae Star System to Go Supernova, Visible in Daytime Skies
The binary star system V Sagittae, located about 10,000 light-years away in the constellation Sagitta, is predicted to end in a spectacular supernova within the next century. This system consists of a white dwarf and a more massive stellar companion, which are locked in a tight orbit, completing a cycle every 12.3 hours. The white dwarf is currently accreting material from its companion at an unprecedented rate, leading researchers to anticipate a nova outburst in the coming years. This event could make V Sagittae visible to the naked eye, even during daylight. The study, led by an international team and published in the Monthly Notices of the Royal Astronomical Society, utilized data from the X-Shooter spectrograph at the European Southern Observatory's Very Large Telescope to analyze the light emitted by the system, providing insights into its composition and behavior.