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:
(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.