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Event Horizon Telescope Traces Magnetic Fields Around a Black Hole (aasnova.org)
85 points by ofou on Sept 9, 2021 | hide | past | favorite | 13 comments


Nice non-specialist summary of recent EHT work! I'm so used to wincing when I click on pop science articles that it was a relief to see a very accurate and yet easy-to-understand article about work I'm involved with.


Amazing work. Being greedy, are there any observatories or collaborations planned that will increase the angular resolution?

I may be wrong but i thought Sgr A was occluded by too much material to be as plainly visible, would we expect similar imagery there?

TIA!


Our telescope is already as wide as the Earth, so there are two main ways to improve it: one is to launch some satellites, the other is to add more telescopes so that we can see fainter things.

Sgr A* does have a lot of stuff in the way, and it's intrinsically fainter than M87*, but we will eventually publish about it.


> Sgr A* does have a lot of stuff in the way, and it's intrinsically fainter than M87*, but we will eventually publish about it.

Any estimate on when this might happen? :) I've been checking the EHT blog for pictures of Sgr A* for years.


Not to diminish from the great work of the EHT, but keep in mind what "picture" means here and also in the context of their original work:

https://news.ycombinator.com/item?id=28000578


I'm fully aware of that and read (or at least skimmed) the original papers, thank you :)


Can you combine the data over longer periods, so that you can expand the effective size to earth's orbital diameter over the course of 6 months? Just coordinating at the global scale seems like a huge accomplishment, but using orbital travel to expand the scope seems like an obvious step.

Do observatories coordinate over such long periods, or is time at a premium?

Awesome project, thank you for your commentary!


The effective size comes from interfering signals taken simultaneously at widely separated receivers, so no, you cannot increase effective size in that way. What you gain from increasing exposure time is that you can see fainter objects.


Black holes change as their accretion disks rotate. If I recall correctly, that timescale is months for M87* and hours for Sgr A*.


Fair enough. I suppose you can't even directly benefit from increased exposure times. However, tracking the dynamics seems valuable (as I assume you are doing).


Where we're going, we won't need interferometry to see.


For some reason the website did not load for me

https://web.archive.org/web/20210909100116/https://aasnova.o...


It didn’t for me on Comcast’s xfinity.

I turned off WiFi and it loaded instantly over 4G.




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