- Oct 2, 2001
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Now why is it that, the larger the hole (physical size), the less gravitational pull? Anyone have any clue?
Hm...where'd you find this information? I've never heard this before and it sounds interesting.Originally posted by: illusion88
Now why is it that, the larger the hole (physical size), the less gravitational pull? Anyone have any clue?
Originally posted by: heliomphalodon
Uh, the more massive the black hole, the larger the area of its event horizon. I don't know what you mean by your statement.
I think what this thread may be trying to discuss is whether the gravitational gradient near the event horizon of a black hole is less for a large black hole than for a small one.Originally posted by: Shalmanese
The gravitational pull is NOT less, it cant be.
Originally posted by: illusion88
Now why is it that, the larger the hole (physical size), the less gravitational pull? Anyone have any clue?
Suppose that, possessing a proper spacecraft and a self-destructive urge, I decide to go black-hole jumping and head for an uncharged, nonrotating ("Schwarzschild") black hole. In this and other kinds of hole, I won't, before I fall in, be able to see anything within the event horizon. But there's nothing locally special about the event horizon; when I get there it won't seem like a particularly unusual place, except that I will see strange optical distortions of the sky around me from all the bending of light that goes on. But as soon as I fall through, I'm doomed. No bungee will help me, since bungees can't keep Sunday from turning into Monday. I have to hit the singularity eventually, and before I get there there will be enormous tidal forces-- forces due to the curvature of spacetime-- which will squash me and my spaceship in some directions and stretch them in another until I look like a piece of spaghetti. At the singularity all of present physics is mute as to what will happen, but I won't care. I'll be dead.
For ordinary black holes of a few solar masses, there are actually large tidal forces well outside the event horizon, so I probably wouldn't even make it into the hole alive and unstretched. For a black hole of 8 solar masses, for instance, the value of r at which tides become fatal is about 400 km, and the Schwarzschild radius is just 24 km. But tidal stresses are proportional to M/r3. Therefore the fatal r goes as the cube root of the mass, whereas the Schwarzschild radius of the black hole is proportional to the mass. So for black holes larger than about 1000 solar masses I could probably fall in alive, and for still larger ones I might not even notice the tidal forces until I'm through the horizon and doomed.
Originally posted by: dzt
gravity is function of mass and distance.
more distance means square less gravity
more mass linearly more gravity
blackholes become smaller as it grows older, it compacting itself and then the size became smaller so the mass density is bigger due to it's own mass or any materials entering it.
that's why smaller black hole have more gravity, since it has more mass and less radius.
am I right ?
