For decades, astronomers and stargazers have been waiting for the return of one of the night sky’s rarest spectacles — a nova explosion. Now, attention is once again focused on T Coronae Borealis — also known as the “Blaze Star” — after researchers identified June 25, 2026, as the statistically most likely date for its long-awaited eruption.
An artist's rendering of T Coronae Borealis, also known as T CrB, a recurrent nova in the constellation Corona Borealis. It is a binary system composed of a red giant star and a white dwarf star, surrounded by an accretion disc, and has outbursts approximately every 80 years.
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T Coronae Borealis is a recurrent nova located around 3,000 light-years from the solar system in Corona Borealis, a crescent-shaped constellation of seven stars between the bright stars Vega and Arcturus.
The star system erupts roughly every 80 years — almost the perfect definition of a once-in-a-lifetime event — with previous outbursts recorded in 1866 and 1946.
Astronomers expect it to brighten from its usual 10th magnitude to around magnitude +2 or +3, making it visible to the naked eye for a few days or weeks. Its explosion will be one of the most unusual astronomical events visible without any special equipment.
According to Sky & Telescope, if the nova does not occur around that date, the next most likely eruption window would be February 8, 2027.
T Coronae Borealis (T CrB) is located in the constellation Corona Borealis, also known as the Northern Crown. Although astronomers refer to the event as an explosion, the phenomenon does not destroy the star — that’s a supernova. A nova is a sudden brightening caused by a thermonuclear eruption on the surface of a white dwarf star. T CrB is actually two stars — a red giant and a small white dwarf. As the red giant expands, it ejects material onto the cooler, denser white dwarf. Over time, enough matter accumulates to trigger a thermonuclear reaction, causing the system to shine dramatically brighter before eventually fading back to its normal state.
Astronomers have been closely monitoring T CrB for years. Interest intensified after the star exhibited a characteristic dimming event in 2023 and 2024, which was thought to be very similar to what happened just before its last explosion in 1946. Researchers predicted the nova could occur between April and September 2025, making T CrB one of the most closely watched stars in the sky. However, that did not happen. A paper was published in Research Notes of the American Astronomical Society in October 2024 that stated that June 25, 2026, is the statistically most likely date for T CrB’s next eruption. If that date passes without an outburst, the next most likely eruption window will be Feb. 8, 2027.
Despite the BBC describing the star as on the cusp of a dazzling celestial show, observers should manage their expectations. T CrB is expected to reach between magnitude +2 and +3, making it comparable in brightness to well-known stars such as Polaris, Mizar and Alpheratz — but certainly nothing brighter. According to Sky & Telescope, the nova will become visible to the naked eye, but it will not rank among the brightest objects in the night sky. Nevertheless, its sudden appearance where no obvious star previously existed will make it a fascinating target for skywatchers.
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