Exploring the Unknown: Black Holes

In summary, black holes have never been directly observed, but their existence is inferred by the emissions of matter surrounding them. Nothing can escape from within a black hole's event horizon, and the effects of a black hole's mass are confined to the outside world. While Hawking radiation is a proposed process for black holes to lose mass, it is still a controversial concept.
  • #1
ukmicky
114
1
This may sound silly but is it possible to see a black hole grow, how do we know that black holes consume and hold onto most of what they attract. Unseen by us could black holes convert ordinary matter into something unknown like dark matter made from wimps for example, which are immediately re-emitted back out into space.
 
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  • #2
Well it is all just a theory right now, we are not totally sure if black holes can do anything at all. But from the fact that there is no light in a small circlular area has to mean something. And if the black hole does take things in it has to put it some place. So what you are getting at is a really tough question that will be answered sometime.
 
  • #3
Two comments:

1) Black holes have never been directly observed in the sense that DyeeyD suggested: as a "blank spot" in a field of stars. Instead, they are detected indirectly by the emissions of matter, outside the hole, which is heated as it falls inward toward the hole. Such matter is in the so-called "accretion disc" which surrounds the black hole itself.

2) Nothing which falls into a black hole (i.e. which crosses the event horizon) ever comes back out. Nothing, in any form, even massless photons, can escape from within a black hole's event horizon.

Hawking radiation is a process by which a black hole can appear to lose mass, but it is a fundamentally quantum-mechanical process which actually happens immediately outside a black hole's event horizon. Once inside, nothing ever gets back out.

- Warren
 
  • #4
chroot said:
Two comments:
Nothing which falls into a black hole (i.e. which crosses the event horizon) ever comes back out. Nothing, in any form, even massless photons, can escape from within a black hole's event horizon.
- Warren
Thankyou for the replies

1st
As its impossible to see anything cross through the Event horizon , how do we know that anything does, Is it just a theory,is there any proof.

2nd
if its true that nothing can come out of a black hole as nothing can cross out wards through the EH, how does the mass inside affect the space outside, why isn't the effects of the mass at the singularity confined to the singularity side of the EH
 
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  • #5
1. It would be possible, in theory. We don't currently have any black holes close enough, or any telescopes large enough, to actually "observe" such an event, however.

2. This is correct. Once inside the event horizon, all possible futures end at the singularity. To the outside world, the black hole appears gravitationally to be a mass like any other. In the same way, the Sun would influence the Earth in the same way no matter what substance it were made of. Technically speaking, in the limit of large distances, effects like tidal forces become negligible; the only important gravitational characteristic of a distant body is its mass.

- Warren
 
  • #6
chroot said:
Hawking radiation is a process by which a black hole can appear to lose mass, but it is a fundamentally quantum-mechanical process which actually happens immediately outside a black hole's event horizon. Once inside, nothing ever gets back out.

Hawking radiation, if correct, is a process by which a small black hole does lose mass. Hawking radiation occurs on the very threshold of the event horizon. The concept remains controversial; it is still viewed as a conjecture by many.
 

FAQ: Exploring the Unknown: Black Holes

1. What exactly is a black hole?

A black hole is a region in space with a gravitational pull so strong that nothing, including light, can escape it. This occurs when a massive star dies and collapses in on itself, creating a singularity with infinite density and zero volume.

2. How do we detect black holes?

Black holes themselves cannot be directly observed, but we can detect their presence through their effects on nearby matter and light. For example, we can observe the gravitational lensing of light around a black hole or detect X-rays emitted from gas being pulled 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. This includes light, which is why black holes appear "black" and are not visible to us. However, some theoretical models suggest that quantum particles can escape from a black hole through a process called Hawking radiation.

4. Are there different types of black holes?

Yes, there are three main types of black holes: stellar, intermediate, and supermassive. Stellar black holes are formed from the collapse of a single massive star, while intermediate black holes are believed to form from the merger of multiple stellar black holes. Supermassive black holes are found at the center of most galaxies and are thought to form from the merging of multiple intermediate black holes.

5. What role do black holes play in the universe?

Black holes play a crucial role in the formation and evolution of galaxies. They are also important in shaping the structure of the universe, as their massive gravitational pull can affect the movement and distribution of matter. Additionally, black holes are being studied for their potential use in alternative energy sources and as a way to test the laws of physics in extreme conditions.

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