Skip to main content

A cosmic explosion will create a bright new star in the sky

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.
A red giant star and white dwarf orbit each other in this animation of a nova similar to T Coronae Borealis. NASA/Goddard Space Flight Center

The night sky will soon be getting a brand new star when an expected cosmic explosion that will be visible from Earth even with the naked eye occurs this summer. It is the result of a phenomenon called a nova, where a binary star system called T Corona Borealis (T CrB) will explode in a flash of light that will take it from its dim form, currently visible only with a telescope, to a bright dot visible overhead.

Recommended Videos

A nova eruption happens in binary systems where two stars orbit each other. In the case of T Corona Borealis, the pair consists of a large dim star called a red giant and a smaller, but much denser star called a white dwarf. The white dwarf is the core left behind of what was once a star like our sun, and its density means it has strong gravity that allows it to eat away material from its companion.

“The ultra-dense white dwarf can steal material from the companion star in a process known as accretion, causing a layer of hydrogen to build up on the white dwarf surface,” explains astronomer Mark Hollands from the U.K.’s University of Warwick. “Once sufficient material has built up, this layer will reach a critical temperature, igniting hydrogen fusion. 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 and is responsible for the observed nova.”

Typically, these nova explosions happen just once and are hard to predict. This system, though, is unusual it in that it erupts repeatedly, around every 80 years.

Astronomers have already observed telltale dips in the brightness of the system, and they expect the nova to occur within the next few months. Once the eruption happens, it should be easy to spot in the sky.

“The best thing you can do now is to get familiar with the patch of sky around the constellation Corona Borealis, using a star chart or phone app,” Hollands said. “Once you get to know what stars are visible in that part of the sky, you’ll really appreciate the difference when one night in the next few months there is one extra member of the constellation. The nova will be visible to the naked eye for a few nights and reach a similar brightness to other stars in the Corona Borealis constellation, but if you miss that window, it’ll still be visible for a few weeks with a good pair of binoculars.”

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
A SpaceX Falcon 9 rocket just set a new record
A SpaceX Falcon 9 rocket launching in April 2025.

Following a mission early on Monday, the first stage of a SpaceX Falcon 9 rocket entered the record books by becoming the first one to launch and land 27 times.

The Falcon 9 launched from Cape Canaveral in Florida at midnight on Monday, April 14, in a mission that successfully deployed 27 Starlink satellites to low-Earth orbit.

Read more
James Webb observes a dying star creating a cosmic hourglass
The NASA/ESA/CSA James Webb Space Telescope has taken the most detailed image of planetary nebula NGC 1514 to date thanks to its unique mid-infrared observations. Webb shows its rings as “fuzzy,” intricate clumps of dust. It’s also easier to see holes punched through the bright pink central region.

This strange image may look like a cell dividing, or perhaps even a brain, but it's neither of those things -- it's actually a space nebula, located 1,500 light-years away. Known affectionately as the Crystal Ball Nebula or more technically as NGC 1514, the striking structure of this object was created by the drama of a dying star.

The James Webb Space Telescope captured this image, showing the nebula in more detail than ever before. The object was previously observed using a NASA telescope called the Wide-field Infrared Survey Explorer (WISE) in 2010 by researcher Mike Ressler of NASA’s Jet Propulsion Laboratory, and he had the opportunity to go back and look at the object again using the cutting-edge powers of Webb's MIRI instrument (Mid-Infrared Instrument). That showed up a set of fuzzy rings that were only visible in the infrared and some voids closer to the center of the object.

Read more
James Webb observes what happens when a planet is swallowed by a star
NASA’s James Webb Space Telescope’s observations of what is thought to be the first ever recorded planetary engulfment event revealed a hot accretion disk surrounding the star, with an expanding cloud of cooler dust enveloping the scene. Webb also revealed that the star did not swell to swallow the planet, but the planet’s orbit actually slowly decayed over time.

As planetary demises go, this one is pretty grisly: a planet falls closer and closer to its host star, getting hotter and hotter as it spirals inward, until it finally falls past the point of no return and is swallowed by the star in a tremendous flash of light. That's what happened in an event called ZTF SLRN-2020, and now the James Webb Space Telescope has been observing the aftermath to learn more about this rare event.

“Because this is such a novel event, we didn’t quite know what to expect when we decided to point this telescope in its direction,” said lead researcher Ryan Lau of NOIRLab, who used Webb's MIRI (Mid-Infrared Instrument) and NIRSpec (Near-Infrared Spectrograph) instruments to make observations. “With its high-resolution look in the infrared, we are learning valuable insights about the final fates of planetary systems, possibly including our own.”

Read more