Does the mass of a blackhole remain the same if it is not feeding ?

In summary, the conversation discusses the mass of a black hole and whether it remains the same or decreases as the black hole shrinks in size. It is stated that we do not know for sure what happens inside a black hole, but the math suggests that the mass stays the same while the volume decreases. The concept of Hawking radiation is also mentioned, which suggests that a black hole will radiate off a small portion of its mass over time. However, it is also stated that a proper theory of quantum gravity is needed to fully understand this phenomenon. The conversation then moves on to discussing the gravitational pull of a black hole and how it would still have the same pull as the original star before its collapse. The concept of an event horizon is
  • #1
abbott287
56
2
Does the mass of a black hole remain the same if it is not "feeding"?

If matter in a black hole keeps crushing down in size to infinity, does the mass stay the same, but the volume decreases? Isn't a black hole constantly shrinking in size? Thanks in advance for the help!
 
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  • #2
We don't actually know WHAT is going on inside a black hole but the math says that the mass shrinks down to a point (but, yes, stays the same amount)
 
  • #3
abbott287 said:
If matter in a black hole keeps crushing down in size to infinity, does the mass stay the same, but the volume decreases? Isn't a black hole constantly shrinking in size? Thanks in advance for the help!

You're thinking of Hawking radiation, which theoretically yes, over a great amount of time, a black hole will radiate off a small portion of it's mass. (Google heat death).

But in the case of our sun, if it were big enough to form into a black hole at collapse, would still have about the same gravitational pull as the sun pre-collapse. You might want to stay away from it in your spaceship though, the event horizon might just swallow you before you find it.
 
  • #4
phinds said:
We don't actually know WHAT is going on inside a black hole but the math says that the mass shrinks down to a point (but, yes, stays the same amount)


:eek: I actually got one right! :smile:


If it shrinks down to a point, what stops it shrinking from there?
 
  • #5
Thats one aspect we don't know. QM feels the minimal size or state is the Planck length. Or could be infitismally tiny. Opinions vary on that
 
  • #6
Once the Pauli exclusion limit is exceeded, theoretically there is nothing to prevent the physical volume of mass in a black hole from shrinking to an infinitesimal point called a singularity. This is widely viewed as the mathematical consequence of an incomplete theory. A proper theory of quantum gravity should resolve this paradox.
 
  • #7
Spourk said:
But in the case of our sun, if it were big enough to form into a black hole at collapse, would still have about the same gravitational pull as the sun pre-collapse.

If that's true, why can light escape from stars with enough mass to form a black hole before they collapse? (If the gravitational pull remains the same, and light can't escape post collapse)
As always, thanks in advance for any help!
 
  • #8
abbott287 said:
If that's true, why can light escape from stars with enough mass to form a black hole before they collapse? (If the gravitational pull remains the same, and light can't escape post collapse)
As always, thanks in advance for any help!

Imagine if the Earth were the same mass, but 3,000 km in radius instead of the 6,000 km that it is now. The matter on the far side of the Earth from you is now half the distance that it used to be, which means that the attractive force of gravity from that matter is four times as great due to the inverse square law. If we re-calculate the gravitational force on the Earth we would find that instead of accelerating at 9.8 m/s2 we are now accelerated at about 40 m/s2. If we keep compacting the Earth into a smaller and smaller volume, the force of gravity continues to increase as the average distance between the matter decreases. Eventually we would reach the point where the Earth is so compact that an event horizon forms.

Note, however, that at distance much greater than the radius of the Earth the gravity barely changes. For example, the Moon orbits the Earth at a distance of about 380,000 km. Since that distance is much greater than the radius of the Earth, the gravitational force remains almost exactly the same before and after we compress the planet. This makes sense when you consider that even though parts of the Earth moved towards the Moon during compression, other parts moved away from it.
 
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  • #9
Drakkith, I always thought the gravity at the moon didn't change at all if the Earth shrinks. Why do you say it is "almost" exactly the same? Is it because our simplification of taking the Earth as a point object becomes more valid as it shrinks in size and that makes a small difference at the moon?
 
  • #10
phinds said:
Drakkith, I always thought the gravity at the moon didn't change at all if the Earth shrinks. Why do you say it is "almost" exactly the same? Is it because our simplification of taking the Earth as a point object becomes more valid as it shrinks in size and that makes a small difference at the moon?

Uh, yes. Let's go with that. :-p
 
  • #11
Drakkith said:
Imagine if the Earth were the same mass, but 3,000 km in radius instead of the 6,000 km that it is now. The matter on the far side of the Earth from you is now half the distance that it used to be, which means that the attractive force of gravity from that matter is four times as great due to the inverse square law. If we re-calculate the gravitational force on the Earth we would find that instead of accelerating at 9.8 m/s2 we are now accelerated at about 40 m/s2. If we keep compacting the Earth into a smaller and smaller volume, the force of gravity continues to increase as the average distance between the matter decreases. Eventually we would reach the point where the Earth is so compact that an event horizon forms.

Note, however, that at distance much greater than the radius of the Earth the gravity barely changes. For example, the Moon orbits the Earth at a distance of about 380,000 km. Since that distance is much greater than the radius of the Earth, the gravitational force remains almost exactly the same before and after we compress the planet. This makes sense when you consider that even though parts of the Earth moved towards the Moon during compression, other parts moved away from it.


Great explanation! Thank you!
 

1. Does the mass of a blackhole decrease if it stops feeding?

Yes, the mass of a blackhole does decrease if it stops feeding. This is because the mass of a blackhole is directly related to the amount of matter it consumes. When a blackhole stops feeding, it no longer gains additional mass, causing its overall mass to decrease over time.

2. Will the mass of a blackhole increase if it starts feeding again?

Yes, the mass of a blackhole will increase if it starts feeding again. As mentioned before, the mass of a blackhole is determined by the amount of matter it consumes. Therefore, if a blackhole begins feeding again, it will gain mass and increase in size.

3. Can a blackhole lose all of its mass if it stops feeding?

No, a blackhole cannot lose all of its mass if it stops feeding. This is because blackholes have a minimum mass, known as the Schwarzschild radius, which is determined by their size. Even if a blackhole stops feeding, it will still have this minimum mass.

4. What happens to the mass of a blackhole when it swallows a star?

The mass of a blackhole increases when it swallows a star. This is because stars contain a large amount of matter, and when they are consumed by a blackhole, their mass is added to the blackhole's overall mass.

5. Can the mass of a blackhole change without feeding?

Yes, the mass of a blackhole can change without feeding. Blackholes can lose mass through processes such as Hawking radiation, which is the gradual emission of particles from the blackhole's event horizon. However, this process is very slow, and the mass loss is minimal compared to the mass gained through feeding.

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