NASA's Black Hole Visualization/Explanation

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    Black hole Hole
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Discussion Overview

The discussion revolves around NASA's black hole visualization and the implications of the simulation presented in a video and annotated image. Participants explore various aspects of black holes, including their formation, characteristics, and the accuracy of the visual representation, touching on theoretical and conceptual elements.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Conceptual clarification

Main Points Raised

  • Some participants express interest in the black hole simulation and its explanations, noting the complexity of black hole images.
  • One participant highlights the significance of the Event Horizon Telescope's first black hole image and the recognition received by the team, while sharing a related article.
  • Concerns are raised about the portrayal of the speed of rotation of matter in the accretion disk, suggesting it appears to exceed the speed of light, which some participants challenge.
  • Another participant calculates the speed of matter around a black hole based on the simulation, proposing a specific diameter for the black hole.
  • Discussions arise regarding the representation of matter near the event horizon and the expectations of how much matter should be present, with some questioning the visual accuracy.
  • One participant speculates on the effects of redshift and blueshift on the light emitted from the orbiting matter, considering its high velocity.
  • Another participant discusses the relationship between black hole size and the behavior of orbiting matter, suggesting that larger black holes would require faster orbital speeds.
  • A technical point is made regarding the properties of the innermost stable orbit around black holes, noting that these depend on the spin to mass ratio rather than the mass alone.

Areas of Agreement / Disagreement

Participants express differing views on the accuracy of the black hole visualization, particularly regarding the speed of matter and the amount of matter present near the event horizon. The discussion remains unresolved with multiple competing perspectives on these aspects.

Contextual Notes

Participants note limitations in the representation of black holes in the simulation, including assumptions about speed and the scale of matter in the accretion disk. There is also uncertainty regarding the implications of redshift and blueshift in the visual representation.

BillTre
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TL;DR
NASA's video and annotated image of a black hole simulation.
NASA's website has a video and annotated image of a black hole simulation.
It is here.

I found the explanations of some aspects of the weirdness of black hole images interesting, but I'm no expert on these things.

Screen Shot 2019-09-26 at 9.42.01 AM.png
 
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Astronomy news on Phys.org
I found this:

The Team Behind The First Black Hole Image Was Just Awarded $3 Million Prize
BI-logo-50x50.gif

ARIA BENDIX, BUSINESS INSIDER
6 SEP 2019
The heart of every major galaxy is thought to contain a supermassive black hole – a place where gravity is so strong that anything, including light, gets devoured.
Like all black holes, supermassive ones form when stars collapse in on themselves at the end of their life cycles. On average, they're millions of times more massive than the Sun.
[. . . ]
But on April 10, a group of scientists from the international Event Horizon Telescope Collaboration released the first-ever photograph of a supermassive black hole to the public. Though the image was fuzzy, it signified a major milestone for space research.
The accomplishment has now earned the team a 2020 Breakthrough Prize, which was awarded on September 5. The prize was started eight years ago by a team of investors including Sergey Brin and Mark Zuckerberg, and is often referred to as the "Oscars of Science".
The Event Horizon Telescope Collaboration (EHT) team will collectively receive US$3 million, but the money will be divided equally among the group's 347 scientists, giving each person around US$8,600.
[. . .]
https://www.sciencealert.com/the-fi...am-were-just-awarded-a-3-million-dollar-prize
p.s. I'm going to move over in a few days. My husband finally bought me my own computer. I'm typing on his right now. Please be quite because I don't want him to find me out. :biggrin:
 
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Mary Conrads Sanburn said:
Please be quite because I don't want him to find me out.
$$ ➡ 🤏🤐

Lol. . . JK

.
 
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Mary Conrads Sanburn said:
p.s. I'm going to move over in a few days. My husband finally bought me my own computer. I'm typing on his right now. Please be quite because I don't want him to find me out. :biggrin:

Just tell him you're studying an important event that's on the horizon :wink:
 
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There are a couple things that seem a little misleading, first is the speed of rotation of the matter on the accretion disk (if the supermassive Black hole's EH is ~20 million mile in diameter, it looks like the matter is rotating at well over 150 times the speed of light), and the second is the huge amount of "stuff" that appears to be violently rotating so near to the event horizon.

I know this is done for illustration purposes only, but most people will take stuff coming out of NASA at face value and consider it officially true.
 
Staticboson said:
it looks like the matter is rotating at well over 150 times the speed of light),
How do you figure that?
 
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Assuming 30 million mile EH in diameter for a relatively small supermassive black hole (or 94 million mile circumference) and roughly timing the period of stuff rotating around the BH in the movie clip at 4 seconds, gives me about 24,000,000 miles/sec.
 
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Staticboson said:
in the movie clip
Ah, I didn’t see the movie, I was just looking at the still picture.
 
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No one wants to watch this animation drawn out over a day. Alternatively, we can say it is an intermediate mass black hole.
Staticboson said:
and the second is the huge amount of "stuff" that appears to be violently rotating so near to the event horizon
Compared to what? How much stuff is there, how much stuff do you expect?
 
  • #11
mfb said:
No one wants to watch this animation drawn out over a day. Alternatively, we can say it is an intermediate mass black hole.Compared to what? How much stuff is there, how much stuff do you expect?

My bad, I thought I read supermassive black hole somewhere, but I went back to the article and found no such reference. Assuming the matter in the disk is rotating at nearly the speed of light like the article mentions, working it backwards I get a black hole of around 150,000 miles in diameter, so it is a small one.

My understanding on supermassive black holes is that there is very little matter rotating comparatively close to the BH, that it is relatively quiet nearby (comparing black hole size with accretion disc size), but since it is not a supermassive BH, then I don't know.

I wonder though, instead of being brighter as the picture indicates, wouldn't the portion of the stream moving away from us be significantly redshifted, and the portion moving towards us significantly blueshifted, considering it is moving at nearly the speed of light?
 
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  • #12
They don't give a mass, but it shouldn't matter as the accretion disk should be roughly scale-invariant if we scale the time accordingly.
There is no absolute scale for the amount of matter either, we just see it is enough to form a nice accretion disk.
Staticboson said:
I wonder though, instead of being brighter as the picture indicates, wouldn't the portion of the stream moving away from us be significantly redshifted, and the portion moving towards us significantly blueshifted, considering it is moving at nearly the speed of light?
The part moving towards us (left) is brighter than the part moving away (right). As it is a false color image you don't see red/blueshift directly.
 
  • #13
Why is this:
Staticboson said:
My understanding on supermassive black holes is that there is very little matter rotating comparatively close to the BH, that it is relatively quiet nearby (comparing black hole size with accretion disc size), but since it is not a supermassive BH, then I don't know.
Is this because it would take super-c speeds to orbit near a large enough black hole?
Thinking geometrically (I'm only a biologist), the orbit speed would have to increase to orbit a larger black hole. A larger black hole's orbit would have less curvature, so an orbiting object would have to go faster to make up for rate of fall from gravity.
Does this make sense?

Also, regardless of the orbiting matter, it seems like a lot of the light given off by the orbiting stuff (as shown by the orbiting lite-up blobs) would fall into the black hole, decreasing the total amount substance in orbit.
 
  • #14
The ratio of innermost stable orbit to the Schwarzschild radius, and also the speed of the innermost stable orbit, are independent of the mass of the black hole. They depend on the spin to mass ratio only. This black hole here has zero spin.
 

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