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The night sky could soon offer a spectacle of a lifetime as the T Coronae Borealis star system gears up for a potential nova explosion.
This rare astronomical event, marked by a dramatic increase in brightness, promises to enthrall stargazers and scientists alike.
The system is overdue for an explosion, and while not normally visible with the naked eye, when it occurs, T Coronae Borealis will rival the North Star (Polaris) in brightness.
The eruption could happen at literally any moment.

M. Kornmesser, L. Calçada/ESO
What Is T Coronae Borealis?
T Coronae Borealis, nicknamed “The Blaze Star,” is a recurring nova located in the constellation Corona Borealis, about 3,000 light-years from Earth.
This extraordinary system consists of two aging stars: a red giant and a white dwarf. The white dwarf acts as a cosmic thief, pulling material from its red giant companion in a process called accretion.
White dwarves are the end products of stars like our sun. Once it has used all of its nuclear fuel and passed through the red giant phase, the star blasts off its outer layers, leaving an extremely hot and dense core.
The accumulation of matter triggers a buildup of pressure and temperature on the white dwarf’s surface, eventually leading to a thermonuclear reaction—a nova explosion.
Unlike supernovae, which signify the death of a massive star, novae are surface-level events and can repeat as long as the white dwarf continues to draw material from its companion.
Historically, T Coronae Borealis has erupted in 1787, 1866, and 1946—with possible earlier eruptions recorded as far back as 1217.
When Could the T Coronae Borealis Appear?
Astronomers predicted that the explosion would occur before September 2024. But nova explosions are unpredictable, and stargazers are still waiting as the calendar flips over to 2025.
Observations since 2016 have revealed patterns of increasing brightness and a shift toward blue light—precursors to the 1946 nova event.
T Coronae Borealis is currently too dim to see without a telescope. However, during the nova, the system increases in brightness over 1,000 times, becoming visible to the naked eye, adding a “new star” to the familiar Corona Borealis constellation.
When the explosion occurs, it will be visible for just under a week, or a little longer with a telescope.
What Are People Saying
Rebekah Hounsell, a nova specialist at NASA‘s Goddard Space Flight Center, said in a statement: “It’s a once-in-a-lifetime event that will create a lot of new astronomers out there, giving young people a cosmic event they can observe for themselves, ask their own questions, and collect their own data.
“There are a few recurrent novae with very short cycles, but typically, we don’t often see a repeated outburst in a human lifetime, and rarely one so relatively close to our own system. It’s incredibly exciting to have this front-row seat.”
How to Prepare for the Show
For those eager to catch this once-in-a-lifetime event, preparation is key.
Corona Borealis is a horseshoe-shaped arc of stars nestled west of the Hercules constellation, best viewed under clear night skies.
To locate it, look for two of the Northern Hemisphere’s brightest stars, Arcturus and Vega. Draw an imaginary straight line between them, and this path will guide your gaze to the Hercules constellation and the curve of the Corona Borealis.
Stargazers can familiarize themselves with the Corona Borealis constellation using star charts or smartphone apps.
NASA’s Fermi telescope is already monitoring the system daily, collecting vital data in hopes of capturing the nova in action.
Do you have a tip on a science story that Newsweek should be covering? Do you have a question about T Coronae Borealis? Let us know via science@newsweek.com.
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