This is the fifth installment of our ten-part series on the brightest stars and, with it, we’re pleased to present the red supergiant star, Betelgeuse, the right shoulder of Orion, the hunter.
Even though we’re still in August and Orion is a winter constellation, its prominence as a near-term supernova candidate makes it especially interesting. We’ve recently produced 2 videos and a podcast discussing Betelgeuse, so it’s fitting that we discuss the star here. You’ll see Orion, Betelgeuse and many of the stars of winter if you stay up late enough (later than 4:00 AM now).
Betelgeuse was a bright, hot O-class star before running out of hydrogen fuel and transitioning to helium in its core. Despite its low temperature of around 3,500 Kelvin, it’s more than 100,000 times as luminous as our Sun, meaning it can crack the top 10 brightest stars in spite of being almost 600 light-years distant. When Betelgeuse does go supernova, it will be the brightest star in the sky for weeks and months and visible during the day!
Back in 2019, the red supergiant star had dimmed dramatically and uncharacteristically, resulting in a flurry of speculation that the star was about to end its life in spectacular fashion as a Type-II supernova. That didn’t happen. It was later determined that the star had sustained a large-mass ejection, partially eclipsing the star, thus reducing its apparent brightness. Fierce stellar winds and large-scale mass ejections are consistent with the behavior of high-mass stars nearing the end of their lives.
What would happen if we replaced the sun with Betelgeuse?
Related content:
Betelgeuse – 2 Great New Videos from Astronomy For Change!
Podcast: Does the Brightening of Betelgeuse Herald The Immanent Occurrence of a New Galactic Supernova?
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