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Betelgeuse is shrinking

Betelgeuse continues to dim, fainter than ever recorded before - now down to magnitude +1.37.
Brian-Ottum-Betelgeuse_Fainting_4x4_dated_1577930828_strip.gif

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I think that is a significant, continuing drop - and interesting that it hasn't gone back to the previous cycle.
 
Betelgeuse continues to dim, fainter than ever recorded before...

I think what you meant to say is that Betelguese went through a period of dimming in the late 14th Century.
Wonder what it's up to these days...

Though if we get a supernova that will be pretty awesome, like a bright extra full moon (good bit brighter than that, I think).
Should be fine so long as it doesn't coincide with a polar shift...

Rural crime rates set to rocket.
 
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Both Betelgeuse's visual magnitude and measured normalised flux continue to drop. Visual magnitude now +1.60.
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Betelgeuse has (at least has had until recently) a dominant pulsation period of around 430 days. If this is still the case then we should see the star hit a minimum and then start to brighten at some point in the next 7-14 days. Even if it does so, this will still have been a most unusual, exceptional minimum. Quite possibly some indication of a new phase in its life cycle.

The ESO VLT SPHERE instrument (Paranal, Chile) has directly imaged the surface of Betelgeuse in visible light over the previous two months and it has clearly changed significantly in presentation from near identical observations made about a year earlier:


This could be interpreted as some large scale fluctuation on the surface of the star, part of the early stages prior to going supernova that see very large scale (and hence 'lumpy') convective cells pulsating and bumbling up to the surface (see the simulation back in post #27). It could be some sort of cooling event - perhaps a starspot (cf sunspot). Or possibly it is an ejection of dust in the direction of the observer causing elevated, transient dimming - Betelgeuse is certainly shedding a lot of the outer envelope of its atmosphere at this late stage in its life as illustrated in this infra-red (VLT VISIR instrument) imagery taken December 2019:
eso2003d.jpg

(Note that the bright dot at the centre of the above image is the SPHERE imagery of the star's surface scaled to the correct size and laid over the occulting mask which cuts off the excessively bright output from the stellar surface itself).

More in an ESO press release here.
 
have they found any exoplanets in orbit around Betelgeuse?
No direct evidence. Any that have formed in the short lifetime of the star might have been absorbed in the atmosphere. Alternatively they might still be in that shed atmosphere somewhere but are beyond the reach of current observational techniques.
 
i love that fade in/out sent it to my significant other (astrophysicist) who was disappointingly less than :eek: woah. shame on him and his rational understanding of probability/cosmic timescales :mad:
 
Betelgeuse has (at least has had until recently) a dominant pulsation period of around 430 days. If this is still the case then we should see the star hit a minimum and then start to brighten at some point in the next 7-14 days. Even if it does so, this will still have been a most unusual, exceptional minimum. Quite possibly some indication of a new phase in its life cycle.
And here she goes - we'll likely have to wait a little longer for a firework show - observed to be gradually brightening once more in the last couple of days.
lightcurve_strip.png

Additional observations in the near IR suggest that the luminosity has been fairly constant which implies this is either some extinction event (perhaps ejection of part of the outer stellar envelope) or some other change in surface environment (morphology, temperature, etc) as oppose to a variation in overall power output.
 
So VLT observations point to a cool region of the photosphere itself, cooling an adjacent, recently ejected, cloud of gas leading to dust formation obscuring part of the stellar disk. So an accentuated transient dimming effect (cool photosphere plus dust cloud) was observed.
DOI: 10.1038/s41586-021-03546-8.
 
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