Originally posted by: L00PY
Originally posted by: Connoisseur
Err.... actually Dr. Pizza believe you are incorrect when you say there's a point in the universe where the net gravity is 0.
I'm with DrPizza. Given a near infinite number of point sources of gravity and an infinite number of intersections of those points, there must be at least one intersection where the net gravity approaches a point indistinguishable from zero.
Since gravity is a curvature of space-time that extends to an infinite distance from any given object, there really is no point that will experience a net 0 gravity. Esentially, no matter where in the universe one is, they will always be accelerated towards a certain point. I only mention this because you used the Newtonian measure of gravity (G*m1*m2/R^2) which, although extremely useful in any practical sense (not having anything to do with relativity), is inherently incorrect. If someone with more physics knowledge than me thinks I am wrong, please feel free to correct me.
I doubt you could find anywhere other than the 'center' of the universe (ie, the point where the big bang seems to have happened) where the net gravitational attraction is truly zero.
I *think* (although I'm also not a physics major) that Newton's equations are correct if you're not accelerating, and your velocity relative to the other objects involved is zero (and even then it's a very, very small divergence unless the velocities are a significant fraction of c). The thing is that the denominator of that expression (R^2) is, once you start talking interstellar distances, ENORMOUS compared to the numerator (G*m1*m2). And G is a pretty small constant to begin with. So if you found a point in the solar system where the gravitational forces from the Sun and planets all balanced out -- yes, you would still feel gravitational attraction from the rest of the matter in the Universe. But since we're talking distances of light-years (and tens of thousands of light-years for more distant objects), the net force exerted on you is, for all practical purposes, zero.
Examples:
Force exerted on you (weight, say, 100kg) by the Sun at an Earth-Moon Lagrange point:
(G * <mass of you> * <mass of the Sun> ) / (distance from Earth to Sun)^2
((6.6742 * 10^-11 Nm^2/kg^2) * (100kg) * (2*10^30 kg)) / (1.496 * 10^11 m)^2
13,348,400,000,000,000,000,000 Nm^2 / 22,380,160,000,000,000,000,000 m^2
0.597 N
Definitely not "zero", but pretty small. But try computing the pull that Alpha Centauri (distance: 3.8*10^16m, mass: together the binary stars are about double the Sun's mass) has on you:
(G * <mass of you> * <2 * mass of the Sun> ) / (distance to Alpha Centauri)^2
(6.6742*10^-11 * 100 * 4*10^30) / (3.8*10^16)^2
26,696,800,000,000,000,000,000 Nm^2 / (1.444 * 10^33 m^2)
1.85 * 10^-11 N
Which is pretty dang close to zero. And the *entire* Andromeda Galaxy (distance: 2.1*10^22 m, mass: 12 x 10^11 the mass of the Sun):
(G * <mass of you> * <12*10^11 * mass of the Sun> ) / (distance to the Andromeda Galaxy) ^ 2
(6.6742*10^-11 * 100 * 12 * 10^11 * 2 * 10^30 ) / (2.1 * 10^22) ^ 2
(1.601808 * 10^37 ) / (4.41 * 10^46)
3.63 * 10^-10 N
So, while this 'background gravity' *is* nonzero, it is very, VERY small, and in fact even smaller in practice because some of the distant objects' gravity gets cancelled out.