Never seen an exploding star? This year, you'll have your chance (2024)

An artist's rendering shows the T Coronae Borealis star system, which contains a white dwarf and a red giant. Conceptual Image Lab/Goddard Space Flight Center/NASA hide caption

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Conceptual Image Lab/Goddard Space Flight Center/NASA

An artist's rendering shows the T Coronae Borealis star system, which contains a white dwarf and a red giant.

Conceptual Image Lab/Goddard Space Flight Center/NASA

Space enthusiasts, thank your lucky stars.

Astronomers expect that this year you'll be able to see the explosion of a star system in our Milky Way galaxy by simply looking up at the sky.

Yes, we know you just spent all that time figuring out how to catch the solar eclipse.

But the upcoming nova of the T Coronae Borealis star system is far less common, occurring roughly once every 80 years. A novatakes place when a small star suddenly and dramatically brightens for a short period.

"Seeing that star blow up is much rarer than a solar eclipse," NASA astronomer Bill Cooke told NPR in March. "So it's kind of a once-in-a-lifetime thing."

T Coronae Borealis is expected to nova at any moment between now and September. Located about 3,000 light years from Earth, the binary star system contains both a white dwarf and a red giant.

As the red giant heats up and its pressure grows, it starts spewing matter that's collected by the white dwarf, according to NASA. The smaller star, roughly the size of Earth, gets so overloaded with that matter that explodes.

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"Eventually it accumulates so much material that literally a thermonuclear reaction starts and the star brightens by hundreds of times. It just gets super bright," Cooke said.

Such an event is called a nova, derived from the Latin for "new star," because a once-dim celestial object suddenly becomes illuminated, giving the impression of a new star.

Dr. Rebekah Hounsell, an assistant research scientist at NASA’s Goddard Space Flight Center who specializes in nova events, said in a press release earlier this month that such explosions typically occur on the same star in repeated intervals.

“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,” said Hounsell.

When the nova occurs, the star system could surge from a +10 magnitude, which can't be seen by the naked eye, to a +2 magnitude, roughly the same level of brightness as the North Star. (Higher positive numbers indicate dimmer stars.)

Astronomers say that once the nova reaches its peak brightness, it will be visible to viewers for several days. Those using binoculars will be able to see it for just over a week before it dims again.

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An outburst of T Coronae Borealis was scientifically observed in 1866, but it may have also been spotted as far back as 1217 by a German monk who documented an object that "shone with great light" for "many days." The star system last exploded in 1946.

Astrophysicists plan to closely observe the impending nova with the hope of better understanding these recurrent phenomena, NASA noted.

Among the tools that will be used to collect data on the eruption are the space agency’s Fermi Gamma-ray Space Telescope and James Webb Space Telescope. Some of the technology that’ll be in use, such as gamma-ray imagers, were only developed after the last nova in 1946.

“Typically, nova events are so faint and far away that it’s hard to clearly identify where the erupting energy is concentrated,” said NASA Goddard chief of the Astroparticle Physics Laboratory Elizabeth Hays. “This one will be really close, with a lot of eyes on it, studying the various wavelengths and hopefully giving us data to start unlocking the structure and specific processes involved.”

NASA says the nova will be visible in the constellation Corona Borealis, which is a "small, semicircular arc" located between the constellations Bootes and Hercules.

When you do spot the T Coronae Borealis outburst, think about this: because the star system is so far away, the outburst we'll see will have already occurred about 3,000 years earlier.

"The collapse of the Bronze Age," said Cooke. "You know, the great empires of Egypt, Troy, they were falling apart."

Never seen an exploding star? This year, you'll have your chance (2024)

FAQs

Which star will explode in 2024? ›

In the second half of 2024, a nova explosion in the star system called T Coronae Borealis, or T CrB, will once again be visible to people on Earth. T CrB will appear 1,500 times brighter than usual, but it won't be as spectacular as the event in 1054.

How rare is it to see an exploding star? ›

The nova, a binary system comprising two stars in the constellation Corona Borealis, bursts into view about every 80 years. These nova explosions are not unusual, but T Corona Borealis (TCrB) is close enough and bright enough that it will be visible to the naked eye, which is rarer.

How to see the supernova in 2024? ›

Where to look. Corona Borealis is not a prominent constellation. It's nestled above Bootes and to the west of Ursa Major, home to the Big Dipper, in northern skies. To locate the constellation, look due west and find Arcturus, the brightest star in that region of the sky.

What is the meaning of exploding star? ›

noun. an irregular variable star, such as a nova, supernova, or flare star, in which rapid increases in luminosity occur, caused by some form of explosion.

Will we see a star explode in our lifetime? ›

A "star" that hasn't been seen since 1946 will appear once again in the night sky, and astronomers are determined to get a glimpse of the once-in-a-lifetime event. The "star" is an explosion, also known as a nova event, that happens around once every 80 years.

What star is seen every 80 years? ›

The star system T Coronae Borealis, also named the Blaze Star, produces an explosion roughly every 80 years that yields a bright nova viewable from Earth. The nova was last seen in 1946, and its next outburst is expected at any time between now and September.

What is the rarest star to see? ›

Wolf-Rayet stars are among the rarest and most massive stars in the universe, characterized by their strong stellar winds and extremely high temperatures. These stars have shed much of their hydrogen, exposing the hotter, inner layers that burn heavier elements like carbon and oxygen.

Are we ever going to see a supernova? ›

Unfortunately, supernovae visible to the naked eye are rare. One occurs in our galaxy every few hundred years, so there is no guarantee you will ever see one in our galaxy in your lifetime.

What will the nova look like in 2024? ›

To the naked eye, the nova will instead look like a new star has appeared in the sky. People with high-powered telescopes will be able to see the nova's brightly colored luminosity in some detail.

How far are we safe from supernova? ›

Over the years astronomers have done a lot of research into this possibility, and the good news—sort of—is that a supernova would have to be less than about 160 light-years from Earth to inflict this sort of damage.

What are the nearest supernova candidates to Earth? ›

The closest star to the Earth which could possibly become a Supernova is IK Pegasi, which is over a hundred and fifty light years away. At that distance we would see the star get brighter, but experience no other effects.

Are exploding stars rare? ›

“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,” Hounsell said.

What is the exploding star theory? ›

When the pressure drops low enough in a massive star, gravity suddenly takes over and the star collapses in just seconds. This collapse produces the explosion we call a supernova. Supernovae are so powerful they create new atomic nuclei.

How long does an exploding star last? ›

A supernova typically lasts for several weeks to a few months.

Which star is going to blast? ›

T Coronae Borealis, also known as T CrB (pronounced tee-core-bore) or the "Blaze Star," is on the precipice of a massive explosion — one that should be visible from Earth.

What star can burn for 100 billion years? ›

A red dwarf, which is half as massive as the sun, can last 80 to 100 billion years, which is far longer than the universe's age of 13.8 billion years. This long lifetime is one reason red dwarfs are considered to be good sources for planets hosting life, because they are stable for such a long time.

What was the last star to explode? ›

The last supernova directly observed in the Milky Way was Kepler's Supernova in 1604, appearing not long after Tycho's Supernova in 1572, both of which were visible to the naked eye.

How many years does it take for a star to explode? ›

So, how long does a supernova take to explode? A few million years for the star to die, less than a quarter of a second for its core to collapse, a few hours for the shockwave to reach the surface of the star, a few months to brighten, and then just few years to fade away.

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