KEY POINTS

  • Many scientists believe Betelgeuse was about to go supernova
  • Researchers simulated a supernova event caused by Betelgeuse
  • Betelgeuse is not in danger of exploding anytime soon

A group of researchers simulated what would happen if the red supergiant star Betelgeuse dies and explode in a powerful supernova. The researchers carried out their study based on the notion that the massive star is already nearing the end of its life cycle.

Betelgeuse is located in the Orion constellation and sits about 700 light-years from Earth. Observations on the star indicated that it is about 1,000 times the size of the Sun.

In the past couple of years, scientists noticed a dip in the star’s overall brightness, prompting many of them to believe that Betelgeuse is nearing its death. Scientists predict that once this happens, the star will collapse under the weight of its own gravity, triggering a powerful stellar explosion known as a supernova.

Given the star’s massive size and location, scientists believe that Betelgeuse’s supernova will be visible from Earth. It will appear as a bright flash in the sky that can last for a long time.

In a new study published in the Astrophysical Journal, researchers from the University of California explained how they were able to create a model of a stellar explosion caused by a pulsating supergiant like Betelgeuse.

As noted by the research, the intensity of supernova events depends on the mass of the star. In the case of Betelgeuse, researchers predicted that once it explodes, it will produce a supernova event similar to that of a static star.

“It just looks like a supernova from a bigger star or a smaller star at different points in the pulsation,” Jared Goldberg, the lead author of the study, said in a statement. “It's when you start considering pulsations that are more complicated, where there's stuff moving in at the same time as stuff moving out — then our model actually does produce noticeable differences.”

Although the study explains Betelgeuse’s simulated supernova, a different paper had already confirmed that the massive star is not in danger of exploding anytime soon. According to the authors of the study, the star’s dimming brightness was caused by the outer material being expelled by Betelgeuse.

The researchers explained that this phenomenon, which occurs naturally, releases dust particles around the star. These particles could block the light emitted by the star, causing it to appear dimmer.

“Red supergiants will occasionally shed material from their surfaces, which will condense around the star as dust,” scientist Emily Levesque of the University of Washington said in a press release. “As it cools and dissipates, the dust grains will absorb some of the light heading toward us and block our view.”

Supernova remnant
Supernova remnants are the debris from exploded stars. G292.0+1.8 is a rare type of supernova remnant observed to contain large amounts of oxygen. Because they are one of the primary sources of the heavy elements (that is, everything other than hydrogen and helium) necessary to form planets and people, these oxygen-rich supernova remnants are important to study. The X-ray image of G292+1.8 from Chandra shows a rapidly expanding, intricately structured field left behind by the shattered star. The image is colored red, green, teal and purple in X-rays ranging from the lowest to highest energy levels.Recently the first detection was made of iron debris from the exploded star. Authors constructed a map of this debris, along with that of silicon and sulphur, to understand more about the explosion. They found that these three elements are mainly located in the upper right of the remnant. This is in the opposite direction from the neutron star that was formed in the explosion, and was then kicked towards the lower left of the remnant. This suggests that the origin of this kick is gravitational and fluid forces from an asymmetric explosion. If more than half of the star’s debris is ejected in one direction, then the neutron star is kicked in the other direction so that momentum is conserved. This finding argues against the idea that the copious amounts of neutrinos formed in the supernova explosion were emitted in a lop-sided direction, imparting a kick to the neutron star. NASA/CXC/SAO