BETELGEUSE - SCI & TECH

News: Explained | If Betelgeuse goes supernova, what would it look like?

 

What's in the news?

       The bright, red star Betelgeuse in the constellation Orion has shown some unexpected behaviour.

 

Key takeaways:

       In late 2019 and 2020 it became fainter than we had ever seen it – at least in records going back more than a century. Briefly it became fainter (just about) than Bellatrix, the third brightest star of Orion. This event became known as the “great dimming”.

       But Betelgeuse has since become bright again. For a few days this year, it was the brightest star in Orion – brighter than we have ever seen it. Both events led to speculation about whether its demise in the form of an explosion is imminent.

 

Betelguese:

       Betelgeuse, the seventh brightest star in the sky (discounting the Sun), is the brightest of the variable stars.

       Sometimes Betelgeuse becomes nearly as bright as Rigel (the blue fourth brightest star in the constellation), while at other times it is notably fainter.

       The variation is caused by pulsations, similar to those of Mira although not as large or as regular.

 

Uniqueness of Betelguese:

       Betelgeuse is about 15 to 20 times more massive than the Sun, and stars of this mass are expected to end their lives in a powerful explosion known as a supernova.

       Betelgeuse’s red colour shows it is a red supergiant, meaning it’s already approaching the end of its life.

 

Go back to basics:

Supernovae:

       Sometimes, a star can briefly become extremely bright. The brightest and rarest among those are the supernovae, formed when an entire star ends its life in a powerful explosion.

       Supernovae can be bright enough to be visible during the day, although that has only happened a few times in the past 1,000 years.

 

Features:

       Supernovae produce high energy particles called cosmic rays, which can get past the shield of the earth’s magnetic field.

       A supernova explosion would also create radioactive iron. In fact, this substance has been found in the earth’s seabed and on the Moon, believed to have formed in a supernova explosion between 2 and 3 million years ago.

 

Challenges of Supernova:

       A very close supernova, closer than 30 light-years, could cause major problems.

       The cosmic rays could cause ozone destruction and dangerous UV levels on the earth.

       It could reduce ozone by half over a period lasting hundreds to thousands of years - this level is considered capable of causing an extinction event. (But such a close supernova would be very rare, and may happen only once per billion years)