Astronomers are still waiting for the Blaze Star to erupt, and a new study suggests the first sign of the blast might not be light at all. According to EarthSky, researchers have proposed that neutrinos, tiny particles that barely interact with anything, could reach Earth about 9 to 10 hours before the flash of light and gamma rays, giving telescopes a head start.
The Blaze Star, formally T Coronae Borealis or T CrB, is a recurring nova that has run late. Scientists expected another outburst as early as 2024, but so far it has not happened. When it does, EarthSky reported, the star could briefly become bright enough to see without a telescope.
A nova is not a supernova. The star system does not destroy itself, so it can brighten again and again. In this system, the swollen red giant keeps passing material to the white dwarf, which gathers it in a surrounding disk. All of this sits inside a dense cloud of gas shed by the red giant.
The study was published April 14, 2026, in The Astrophysical Journal Letters. EarthSky described it as the first to suggest neutrinos as a possible early warning for the Blaze Star's next nova. Neutrinos rarely interact with matter, so they can slip out of dense regions that trap other kinds of signals.
The researchers modeled two ways particles might gain energy. In the first, material thrown off the white dwarf slams into the gas around it, and those shock waves could produce high-energy gamma rays and neutrinos. In the second, magnetic field lines in the star's superheated plasma break and reconnect, releasing energy that speeds up particles near the white dwarf. In that case, the dense surrounding material might hold back gamma rays while neutrinos escape toward Earth.
The team also looked at another recurring nova, RS Ophiuchi, which erupted in 2021, and used those observations to help predict what the Blaze Star might do. The 9-to-10-hour advance applies to the magnetic reconnection model.
Neutrinos carry no electric charge, so they cannot be seen directly. Scientists detect them by looking for the charged particles or flashes of light produced on the rare occasions when one collides with an atom.
For astronomers, a few hours of notice could make a real difference. They could point their instruments at the system before the light arrives instead of scrambling afterward. The timing and type of neutrino signal could also help show which process is driving the eruption inside the system.
For everyone else, the Blaze Star remains a patience game. The eruption has not yet occurred, and this study describes models of what could happen, not an observed warning.
Corona Borealis is easy to find. It forms a shape like the letter C and lies roughly on a line between the bright stars Arcturus and Vega, next to the squarish Keystone pattern in Hercules. From mid-northern latitudes it is up for much of the year, though not all of it, and in northern fall it sits low in the west-northwest. EarthSky said binoculars are not required but are always a good idea.
In the Southern Hemisphere, the constellation stays low in the northern sky, so observers there need a dark sky and a clear view to the north. If the eruption comes, EarthSky said the star might briefly rival Gemma, also called Alphecca, the brightest star in Corona Borealis.
Around Prague, based on reporting by EarthSky