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

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The mass of a black hole remains constant if it is not actively feeding, although it theoretically shrinks to a singularity over time due to gravitational collapse. Hawking radiation suggests that black holes can lose mass gradually, but this process occurs over extremely long timescales. The gravitational pull of a black hole, similar to that of a star before it collapses, remains unchanged at distances far from its event horizon. The discussion highlights the complexities of black hole physics, particularly regarding the nature of singularities and quantum gravity. Understanding these phenomena requires further advancements in theoretical physics.
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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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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)
 
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.
 
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?
 
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
 
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.
 
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!
 
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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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!
 
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