Image Credit: NASA/Goddard Space Flight Center

Despite expectations of a star exploding in May and June, the 'Blaze Star' or T Coronae Borealis has not yet exhibited any signs of impending explosion. However, it is anticipated that the event is on the horizon. T Coronae Borealis, also known as Blaze Star, shines at a magnitude of +2, akin to the North Star. As a recurring nova, it will briefly illuminate the sky before returning to its original brightness level. Currently situated in the Corona Borealis constellation approximately 3,000 light-years away from Earth, Blaze Star is part of a binary star system. It consists of a large, cool red giant star and a small, hot white dwarf star orbiting each other. The red giant continuously feeds matter into the white dwarf, leading to periodic detonations and bright eruptions in the sky known as novae. This spectacular event is estimated to occur every 80 years, with the previous one observed in 1946. However, the forthcoming explosion is set to be two years earlier than predicted, as the precursor event has already taken place. The cyclical nature of this occurrence has been documented for over 800 years. Astronomers suggest that the explosion could happen at any moment.Although an exact date cannot be determined, experts anticipate that the event will most likely occur towards the end of September. To find it, look for the star in the constellation Corona Borealis, which will only become visible after the thermonuclear eruption. It can still be located using other astronomical methods. One simple way is to first locate the Big Dipper, then follow the curve of its handle. You will come across a bright red star named Arcturus. Next, find another star named Vega in the northeast direction, and in between these two stars, you will find the Blaze Star.