Hubble Finds that Betelgeuse's Mysterious Dimming Is Due to a Traumatic Outburst

Summary
Hubble Detects Dense, Heated Material Moving Through the Star's Atmosphere
The aging, bright-red supergiant star Betelgeuse has captivated sky watchers since antiquity. The ancient astronomer Ptolemy was one of the first to note the monster star's red color. It is one of the brightest stars in the night sky and appears even more luminous because it is so close to Earth, only 725 light-years away.
But the star also periodically changes in brightness, which was first noted in the 1830s by British astronomer John Herschel. Astronomers now know that the star expands and contracts, brightening and dimming, on a 420-day cycle.
However, in October 2019, the star dimmed dramatically and continued to become even fainter. By mid-February 2020, the monster star had lost more than two-thirds of its brilliance.
This sudden dimming has mystified astronomers, who scrambled to develop several theories for the abrupt change. Ultraviolet observations by the Hubble Space Telescope suggest that the unexpected dimming was probably caused by an immense amount of superhot material ejected into space. The material cooled and formed a dust cloud that blocked the starlight coming from about a quarter of Betelgeuse's surface.
Hubble captured signs of dense, heated material moving through the star's atmosphere in September, October, and November 2019. Then, in December, several ground-based telescopes observed the star decreasing in brightness in its southern hemisphere.
The giant star is destined to end its life in a supernova blast. Some astronomers think the sudden dimming may be a pre-supernova event. Betelgeuse resides in Orion, one of the most recognizable constellations in the sky. The mammoth star marks the right shoulder of the hunter.
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Full Article
Observations by NASA's Hubble Space Telescope are showing that the unexpected dimming of the supergiant star Betelgeuse was most likely caused by an immense amount of hot material ejected into space, forming a dust cloud that blocked starlight coming from Betelgeuse's surface.Hubble researchers suggest that the dust cloud formed when superhot plasma unleashed from an upwelling of a large convection cell on the star's surface passed through the hot atmosphere to the colder outer layers, where it cooled and formed dust grains. The resulting dust cloud blocked light from about a quarter of the star's ...Visit NASA Science to view the full news release including article text and associated Hubble imagery, graphics, scientific visualizations, videos, captions, text descriptions, and other information.
News releases highlighting the discoveries of NASA’s Hubble Space Telescope are produced for NASA by the Space Telescope Science Institute (STScI) in Baltimore, Maryland, under NASA Contract NAS5-26555. News release content is developed by the News Team in STScI’s Office of Public Outreach.
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