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Get ready to watch a rare explosive star system blaze into life

So bright you'll be able to see it without a telescope, a “new” star system, T Coronae Borealis, will become visible for the first time in 80 years between now and September. Abigail Beall explains where to spot it

A red giant star and white dwarf orbit each other in this animation of a nova similar to T Coronae Borealis. The red giant is a large sphere in shades of red, orange, and white, with the side facing the white dwarf the lightest shades. The white dwarf is hidden in a bright glow of white and yellows, which represent an accretion disk around the star. A stream of material, shown as a diffuse cloud of red, flows from the red giant to the white dwarf. When the red giant moves behind the white dwarf, a nova explosion on the white dwarf ignites, creating a ball of ejected nova material shown in pale orange. After the fog of material clears, a small white spot remains, indicating that the white dwarf has survived the explosion. NASA/Goddard Space Flight Center

This week we are focusing on what is currently a dark patch in the sky, but won’t be for much longer. That’s because a “new” star is expected to appear in the night sky over the next few months.

Of course, the star isn’t actually new – it has been around for billions of years. What’s new is that it will be visible to the naked eye, temporarily, while undergoing an explosive event called a nova.

The object in question, called T Coronae Borealis – or the much catchier “blaze star” – is actually a binary star system made up of a white dwarf and a red giant orbiting each other. The hungry white dwarf has been stealing hydrogen from its companion star by means of its gravitational pull. “Once sufficient material has built up, [it] will reach a critical temperature, igniting hydrogen fusion,” says , an astronomer at the University of Warwick in the UK. “This powerful nuclear detonation ejects the gas from the white dwarf surface in a hot, luminous shell. What we then see is the system becoming thousands of times brighter.”

While the exact date this explosion will happen isn’t known, astronomers have been watching the system and expect it to be soon. After observing a dip in brightness since March 2023, which happens before a nova, they predict it will occur between now and September. Once it explodes, the system will become almost as bright as Polaris, the North Star, for a few days.

The best way to prepare for the event is to get familiar with the patch of sky the star system sits in. T Coronae Borealis is in a small constellation called Corona Borealis. This sits between Boötes and Hercules, two much larger constellations in the northern sky.

The best way to find Corona Borealis is by first finding two stars: Arcturus, which will be high in the south in the northern hemisphere, and Vega, which will be lower in the sky and towards the east. These are the two brightest stars in the northern hemisphere, so they should be easy to see from there. Looking directly between the two, you should spot a horseshoe-shaped group of stars: this is Corona Borealis. From the southern hemisphere, Arcturus will be low in the north-east. If Vega is visible, it will be near the eastern horizon and Corona Borealis will be low in the north-eastern sky.

When it makes its appearance, the “new” star will be the brightest in the constellation, making it hard to miss. It will appear just below and to the left of the main horseshoe shape. This kind of event doesn’t come around often – this star system is one of 10 known repeating novae and it explodes roughly every 80 years.

I hope you enjoy watching the sky change. It is a lovely reminder that the stars aren’t fixed points of light as they seem to be, but dynamic monsters that are growing and evolving.

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