Have you ever heard of the Blaze Star? It\u2019s a star in the constellation Corona Borealis, the Northern Crown, that was supposed to go nova<\/em> last year. Well, we\u2019re still waiting. But when it finally does erupt, it\u2019ll be a once-in-a-lifetime show in our night sky. <\/p>\n The eagerly awaited Blaze Star nova is a real opportunity for keen night sky observers to witness a \u201cnew star\u201d in the sky \u2026 but only for a few days before it fades away again. Here\u2019s more about why we\u2019re still waiting on the Blaze Star. And about how you can see when it does finally erupt as a nova.<\/p>\n The 2025 EarthSky Lunar Calendar is now available! A unique and beautiful poster-sized calendar. Get yours today!<\/p>\n Predicting eruptions of stars is not an exact science. The Blaze Star (T Coronae Borealis) underwent two known eruptions recorded by astronomers. Those events were on May 12, 1866, and on February 9, 1946. Those eruptions were 80 years apart. So scientists thought that, in another 80 years, the star would erupt again. So, 80 years from 1946 would be 2026. Which raises the question: Why did astronomers think the eruption would happen in 2024?<\/p>\n Well, the star brightened and dimmed before its last eruption in 1946. And it has been brightening and dimming now as well, leading some to think the nova would happen sooner rather than later. But it appears as if later is more likely. And so we wait \u2026<\/p>\n In the meantime, here\u2019s how to find Corona Borealis and be ready to see it when the nova arrives.<\/p>\n The Blaze Star isn\u2019t one star but two. It\u2019s a binary system with a white dwarf and a red giant. White dwarfs are stellar remnants, the exposed core of a sunlike star that shed its outer layers at the end of its main-sequence life. It\u2019s a super-dense star with the mass of our sun but only the size of Earth.<\/p>\n Blaze Star\u2019s white dwarf has built up material on its surface, siphoned off from the red giant star. Periodically, it \u201ccan\u2019t take no more\u201d and explodes, about every 80 years.<\/p>\n This is our best opportunity to see a nova with some warning. Plus we have great visual context from the surrounding C-shape of stars. So cross your fingers for good weather when it happens.<\/p>\n The constellation Corona Borealis is back from a month hiding below the horizon. It rotates around Polaris just outside of what we traditionally think of as the circumpolar constellations. This mean it\u2019s not visible all year round for much of the Northern Hemisphere.<\/p>\n The easy-to-find constellation looks distinctly like a backward C at this time of year. It lies between the bright star Arcturus and the squarish four-star shape of Hercules. Look east at the stars coming over the horizon before dawn. Find the bright orange star Arcturus. Then, to the bottom left of Arcturus is the backward C shape of Corona Borealis \u2026 unless there\u2019s a guest star messing up the shape!<\/p>\n By the summer these constellations will be high in the sky again. You always need to spend some time dark-adapting your eyes before you see the constellations properly. Plus, binoculars would be a good idea. And you need to be ready to go when we get the news, as it will only be there for a couple of days.<\/p>\n The actual explosion of the Blaze Star nova will likely dwarf any explosion you\u2019ll ever see. But the star is far away. How bright will it get in our sky? Astronomers expect it to reach an apparent magnitude of 2. That\u2019s a respectable brightness for a star. It\u2019s conveniently comparable to the brightest star in the Northern Crown, the Jewel of the Crown, Alphecca. So, for a few days, the Northern Crown will have two jewels!<\/p>\n T Corana Borealis \u2013 the Blaze Star \u2013 also one of the most distant stars you\u2019ll ever see. Alphecca is around 75 light-years away, while the Blaze Star is closer to 3,000 light-years away. So that gives you some perspective on the absolute magnitude (brightness) of this enormous blast. And since the light of this explosion has travelled for 3,000 years to get here, in relative terms the nova happened during the Bronze Age.<\/p>\n Remember that, when they are side-by-side with approximately the same brightness, the nova is 40 times farther away than Alphecca. Also, we are not seeing the two stars at the same moment in time. One we see as it was 75 years ago and the other we see as it was 3,000 years ago. It can be hard to get your head around that!<\/p>\n The nova will brighten the star by thousands of times, typically over just a few hours, and then take some days to fade away again. When it\u2019s done, it will go back to its normal appearance.<\/p>\n If you are not familiar with the Northern Crown, get out and have a look at it before this nova happens. And then, clouds willing, when it does erupt we can go out and see the C shape is harder to spot. Instead, the dominant feature will be two bright-ish stars, Alphecca (the brightest star in Corona Borealis), and the Blaze Star. <\/p>\n The Blaze Star is normally invisible to the unaided eye. On a regular day, it sits at around magnitude 10, making it only the 19th brightest star in the constellation. But as it undergoes a colossal outburst of energy, it will brighten.<\/p>\n Bottom line: We\u2019re still waiting for the Blaze Star to go nova! Here\u2019s how to find the constellation so you\u2019re ready when it happens.<\/p>\n![\"Blaze](\"https:\/\/earthsky.org\/upl\/2024\/07\/Corona-Borealis-T-CrB-Paul-Henkiel-April-2024-.jpg\")
Why hasn\u2019t it happened yet?<\/h3>\n
Why will it go nova?<\/h3>\n
![\"Animation](\"https:\/\/earthsky.org\/upl\/2024\/03\/NovaCygni_ArtistConcept_watermarked-ezgif.com-gif-to-webp-converter.webp\")
Where to look to find the Blaze Star<\/h3>\n
![\"Star](\"https:\/\/earthsky.org\/upl\/2025\/02\/BlazeStarChrisHarvey-600.gif\")
How bright will the Blaze Star be?<\/h3>\n
![\"Star](\"https:\/\/earthsky.org\/upl\/2024\/03\/Hercules-Corona-Borealis-Bootes-NASA.jpg\")
Finding Corona Borealis, the Northern Crown<\/h3>\n