The question I want to ask is what point is there in using F=Gm1m2r2
r
.I'm currently not good enough at maths to calculate that myself.
In particular, let's take a vector form for point of mass: →F=Gm1m2|r|2→r|r|
Now we should integrate the vectors over volume V, which is a sphere with center at distance r from the point of our calculations.
How would I go about such calculations?
If the scope of maths involved exceeds what's welcome on physics.se, could you help me rephrase the question for mathematics.se, or point me to resources that would let me solve this?
(assume uniform distribution of mass - asteroids etc.)
Answer
The way you would go about calculating the gravitational forces from a sphere of radius R is to start by looking at a homogeneous ring and calculating its gravitational pull on a fixed point at a certain distance from the circle's center on the rings center axis. Then you look at the gravitational forces from a spherical layer of an infinitesimal thickness, consisting of the rings from before with some infinitesimal width ρdϕ if ρ is the radius of the spherical layer and dϕ is the angular extent of the rings width.
You'll find that the attraction from such a spherical layer with mass M is the same as for a point mass M located at the center of the spherical layer. And since a filled homogeneous sphere is built up from such elementary spherical layers (each with mass dM) the total sphere will have the same property: for gravitational calculations with Newton's law, the sphere could just be replaced by a point mass located at its center.
The whole calculation is a bit long to write out completely here, but if this is too short, I could expand this answer. Also, if the sphere is not homogeneous, corrections need to be made. I'm not entirely sure how that's done though.
EDIT: the link provided by John Rennie explains in (much) more detail what I'm talking about.
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