B Betelgeuse unusual dimming - what's up?

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Betelgeuse is currently experiencing significant dimming, reaching its lowest brightness in over 50 years, which has sparked interest among astronomers. This dimming is attributed to complex pulsations and changes in the star's convective surface rather than an imminent supernova event. While Betelgeuse is expected to eventually explode as a Type II supernova, predictions suggest this will not occur in the near future, possibly not within our lifetimes. The star's brightness variations are part of its natural cycle, with historical data showing similar fluctuations. Overall, the current dimming serves as an opportunity for scientific observation and public interest, rather than a direct indication of an impending explosion.
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epenguin said:
The scientists have concluded that some time before the great dimming, the star ejected a large gas bubble. When a patch of its surface cooled shortly afterwards, the temperature decrease was enough for heavier elements, such as silicon, that were contained within the gas to condense into solid particles.
This is an interesting piece that's not mentioned in other published summaries. I take the part about "before the great dimming, the star ejected a large gas bubble" to mean something like a CME, but it was still hot and transparent. Then "when a patch of its surface cooled shortly afterwards, the temperature decrease was enough for heavier elements, such as silicon, that were contained within the gas to condense into solid particles." But isn't it the ejected mass that cooled? Or did the outer surface cool?

In either event, cooling such that Si or perhaps SiO2 precipitated and condensed into dust particles, and perhaps Al2O3, or alumina-silicates.

There is this paper "A dusty veil shading Betelgeuse during its Great Dimming"
https://www.nature.com/articles/s41586-021-03546-8
 

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