How Are Black Holes Detected and Measured?

In summary, there is evidence that black holes exist, and they are detected by their gravitationel effect on nearby stars.
  • #1
shaan_aragorn
43
0
Which are all the methods by which black holes are detected?
How do we get to know how massive a black hole
 
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  • #2
Ted Bunn made a nice http://cosmology.berkeley.edu/Education/BHfaq.html#q7" about black holes, check the section "Is there any evidence that black holes exist?".

There seems to be ample evidence that some objects are above a critical mass/density to be considered black holes. But the fact that these objects exist is obviously no proof of the correctness of general relativity with regards to black holes, but if we assume that general relativity is correct they must be black holes.
 
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  • #3
Black holes that are not eating somthing are virtually invisible. We can only detect them by their gravitationel effect on nearby stars. Black holes that are feeding on a nearby star is another matter. The gas from the star will
go round the black hole in a spirale while heating. This is called an accration disk. This super-hot gas emits a lot of visible light and a lot of radiation.
 
  • #4
lionell said:
Black holes that are not eating somthing are virtually invisible. We can only detect them by their gravitationel effect on nearby stars. Black holes that are feeding on a nearby star is another matter. The gas from the star will
go round the black hole in a spirale while heating. This is called an accration disk. This super-hot gas emits a lot of visible light and a lot of radiation.

As the black hole "feeds" on a nearby star does the black hole become more massive? Theoretically, how many stars could it devour?
 
  • #5
Esnas said:
As the black hole "feeds" on a nearby star does the black hole become more massive? Theoretically, how many stars could it devour?

Classically there is no limit - black holes at the centre of galaxies are very large, the one in the middle of our own milky way is at least 3.5M times the mass of the sun.
It doesn't get all this mass from swallowing stars, but also dust, gas and anything else around it.
 
  • #6
mgb_phys said:
Classically there is no limit - black holes at the centre of galaxies are very large, the one in the middle of our own milky way is at least 3.5M times the mass of the sun.
It doesn't get all this mass from swallowing stars, but also dust, gas and anything else around it.

Wow! 3.5 million times the mass of the sun is pretty great indeed! To take things a bit further, would it be theoretically possible for a black hole to swallow the entire universe? It seems that size of the black hole is irrelavant since even a small one (Tolman-Oppenheimer-Volkoff limit) could grow without limit building an ever increasing gravitational field. Luckily, there is a lot of space in between celestial bodies. What else is there to stop total engulfment?
 
  • #7
Esnas said:
Theoretically, how many stars could it devour?

All of them.
 
  • #8
Theoretically, how many stars could it devour?


Asphodel said:
All of them.

NO in the real world
Theoretically even, chances are billions to 1,

and that's just in a galixcy
some things are just way tooooooo far apart
 
  • #9
Well that's two different questions. How many could it devour? As far as I know, there's not really an upper limit to the size of a black hole. You might want to look at this, for example (which seems a little fishy to me, with "wait but what about entropy?" being my first question...maybe an interesting undergrad research topic for me ;)). How many is it likely to devour is dependent on star density, star size, time, and probably initial black hole size. It's also evaporating at some rate. You have galactic black holes that have a rather monstrous amount of matter, and you can merge those (rather more efficient than hunting down individual stars, if we're going for mass).

I remember reading something about a black hole going through a periodic absorption and discharge in some sort of dense region, causing the region to take on a long-term periodic emission on a larger scale than you'd usually get. Can't find it right now, but really interesting.
 
  • #10
Esnas said:
It seems that size of the black hole is irrelavant since even a small one (Tolman-Oppenheimer-Volkoff limit) could grow without limit building an ever increasing gravitational field.

Object1*object2=x
x/distance between the two objects squared= the amount of force at which gravity pulls the two(or more) objects(calculated in Newtons). This means a black hole with the mass of 4.5 the mass of the sun's core the size of a fork will have MUCH more gravital pull as a black hole with the same mass and the size of the earth.
 
  • #11
Has it already happened that a black hole ate an other black hole?
 
  • #12
lionell said:
Has it already happened that a black hole ate an other black hole?

Yes.
 

1. What is a black hole?

A black hole is a region in space where the gravitational pull is so strong that nothing, not even light, can escape. It is formed when a massive star dies and its core collapses under its own gravity.

2. How do we know black holes exist?

We know black holes exist based on observational evidence such as the distortion of light and stars orbiting around a point of high gravity. We can also detect the radiation emitted by matter falling into a black hole.

3. Can anything escape from a black hole?

Once something crosses the event horizon of a black hole, it cannot escape. However, Hawking radiation suggests that very small particles can escape from a black hole's gravitational pull.

4. Do black holes last forever?

According to current theories, black holes will eventually evaporate due to Hawking radiation. However, this process would take an incredibly long time for a black hole of significant mass.

5. Can we enter a black hole?

Entering a black hole would be a one-way trip, as the intense gravitational forces would stretch and compress anything that enters. Additionally, the extreme conditions near the singularity would make it impossible for a human to survive.

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