B Most detailed picture of Antares

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The Very Large Telescope has captured the most detailed image of Antares, a red supergiant star located 550 light years away, showcasing its apparent diameter of 41 milliarcseconds. This image reveals potential surface features that may represent large convective cells, differing significantly from the numerous granules observed on the Sun. The discussion also highlights the challenges of observing stars like Alpha Centauri, which, despite being closer, has a much smaller angular size and is less likely to show significant brightness variations. Observers with smaller telescopes can only see Antares as a bright dot, emphasizing the advanced technology required for such detailed imaging. The remarkable resolution achieved by the VLT underscores the capabilities of modern astronomy in studying distant stars.
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From ESO

An image of Antares, taken with the Very Large Telescope in interferometry mode. It is the most detailed picture of any star apart from the Sun. The star has 900 times the diameter of Sun and is (sort of) nearby at 550 light years distance, making it a great target for these observations. The star has an apparent diameter of 41 milliarcseconds, corresponding to the width of a human hair seen from 500 meters away.
 
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I saw this on a Space.com article yesterday. Pretty incredible that we can see such detail at that distance.
 
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Remarkable image, but the question in my mind is, what are we seeing? Are the bright areas zones of convective upwelling and the dark zones convective downturns? Or vice versa? Or something else. I have not had time to fully grasp the associated paper to determine if my suspicions are valid.

If they are the surface expression of convective cells then they are very large and few in number. I therefore found this paper's prediction, from 1975, intriguing:
"An attempt is made to estimate the sizes of the convective elements which dominate the brightness variations on the photospheres of red giants and supergiants. The data assembled permit the extreme hypothesis that these dominant convective elements are so large that only a modest number of them exists at anyone time on the entire surface of such a star - in contrast with two million granules on the sun."
 
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Wow! Cool photo!
Antares (Alpha Scorpii) is a red supergiant. I see it every night [twinkling reddish] west these days, early night hours, before it sets. It is also a double star. It's companion, Antares B, is much smaller and hard to see.

With my small 60mm refracting telescope (and even bigger telescopes) I only see a bright twinkling reddish dot of course, when I look at Antares. But that picture in the OP is way beyond anything I've seen for a star from earth. I'm wondering how Alpha Centauri (nearest star system to Earth [4.37 light years away]) would look like with similar telescope views?
But it's a much smaller star [system*]! So no big luck:
hubble_friday_09022016.jpg

https://www.nasa.gov/image-feature/goddard/2016/hubbles-best-image-of-alpha-centauri-a-and-b/

*Alpha Centauri is a binary star (A, B), orbited loosly by C (a small and faint red dwarf), the Proxima Centauri (nearest star to Earth [4.24 light years]), way smaller than the other two, which are comparable to our Sun ...
 
Stavros Kiri said:
But that picture in the OP is way beyond anything I've seen for a star from earth.
Antares has one of the largest angular diameters from Earth, and the VLT in interferometry mode has the best angular resolution available. The combination of both is needed to get such a picture. It is no surprise that you can't see details with hobby equipment.

The Sun as exception, of course.
 
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mfb said:
Antares has one of the largest angular diameters from Earth, and the VLT in interferometry mode has the best angular resolution available. The combination of both is needed to get such a picture. It is no surprise that you can't see details with hobby equipment.

Additionally the Alpha Centauri picture above is taken using HST regular cameras and not VLT in interferometry mode. Alpha Centari A has an angular size of 7 milliarcseconds (compared with 41 for Antares and 49 for Betelgeuse) so it too could be resolved using VST.
 
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If there are significant brightness variations there might be something visible, but I don't expect large-scale brightness variations for the Alpha Centauri stars.
 
mfb said:
If there are significant brightness variations there might be something visible, but I don't expect large-scale brightness variations for the Alpha Centauri stars.

I don't expect any significant variations either since the Alpha Centauri stars should be living much more sedate lifes than a red super-giant but it is resolvable which was sort of the question asked (what would it look like using VST).
 
Well, it has 1/6 the angular diameter of Antares, with some goodwill you can see something like 7 brighter/dimmer spots across its diameter "\"-direction, so I guess you can at least compare the brightness of different hemispheres.
 

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