The Inverse Square Law
Suppose two point masses with masses m and M respectively are
located a distance r apart. Sir Isaac Newton's inverse square law
states that the magnitude | F| of the gravitational force
between the two point masses is
where G is the universal gravitational constant. However, as Newton
realized and struggled with for some time, objects in the real world are not
point-masses and instead, the law (4) might need to be
modified.
In particular, let's suppose that one of the bodies is not a
''point-mass,'' but instead is a sphere of radius R with uniform mass
density m. Suppose that r > R and that the sphere is
centered at ( 0,0, r) . If the other body is a point-mass
''satellite'' of mass m located at the origin, then the gravitational
force is directed along the z-axis.
Suppose now that a small ''piece'' of the sphere is located at a point ( r,f,q) (in spherical coordinates), and suppose
that it has a small mass dM. Then the distance between the small piece and
the origin is r.
so that by (4) the ''small'' magnitude d|F| of the gravitational force between the small ''piece'' and the
satellite is
However, the symmetry of the sphere implies that we need only the gravitational
pull in the vertical direction. The amount of d|F| in the vertical direction is then given by
cos(f) d| F| (see above).
Thus, the total gravitational force in the vertical direction is
|
| F| = |
ó õ
|
|
ó õ
|
|
ó õ
|
S
|
cos( f) d| F| = |
ó õ
|
|
ó õ
|
|
ó õ
|
S
|
|
-Gm cos( f)
r2
|
dM |
|
where S is the sphere corresponding to the ''planet''. If dV denotes the
volume of a small ''piece'' of the sphere, then dM = m
dV, which leads to
|
| F| = -Gmm |
ó õ
|
|
ó õ
|
|
ó õ
|
S
|
|
cos( f)
r2
|
dV |
| (6) |
In Cartesian coordinates, the sphere S is given by
|
x2+y2+( z-r) 2 = R2 or x2+y2+z2-2rz+r2 = R2 |
|
In spherical coordinates this becomes
which by the quadratic formula leads to
Thus, the sphere is contained between
|
r1 = r cosf - |
|
and r2 = r cosf + |
|
|
|
Let us also note that f ranges from 0 to sin-1(R/r) while q ranges over [ 0,2p] .
Evaluating (6) in spherical coordinates leads to
|
|
|
|
-Gmm |
ó õ
|
2p
0
|
|
ó õ
|
sin-1(R/r)
0
|
|
ó õ
|
r2
r1
|
|
cos( f)
r2
|
r2sin( f) drdfdq |
| |
|
|
-Gmm |
ó õ
|
2p
0
|
|
ó õ
|
sin-1( R/r)
0
|
|
ó õ
|
r2
r1
|
cos( f) sin( f) drdfdq |
| |
|
| -Gmm |
ó õ
|
2p
0
|
|
ó õ
|
sin-1( R/r)
0
|
( r2-r1) cos( f) sin( f)drdfdq |
|
|
Since r2-r1 = 2( R2-r2sin2( f)) 1/2, this in turn leads to
|
| F| = -2Gmm |
ó õ
|
2p
0
|
|
ó õ
|
sin-1(R/r)
0
|
( R2-r2sin2( f) )1/2sin( f) cos( f) dfdq |
|
If we let u( f) = R2-r2sin2( f) ,
then the limits of integration become
|
u( 0) = R2 and u |
æ è
|
sin-1 |
æ è
|
|
R
r
|
ö ø
|
ö ø
|
= R2-r2 |
æ è
|
|
R2
r2
|
ö ø
|
= 0 |
|
Moreover, du = -2r22sin( f) cos( f)df, so that
|
|
|
|
|
Gmm
r2
|
|
ó õ
|
2p
0
|
|
ó õ
|
sin-1( R/r)
0
|
( R2-r2sin2( f)) 1/2 ( -2r2sin( f) cos( f) ) dfdq |
| |
|
|
|
Gmm
r2
|
|
ó õ
|
2p
0
|
|
ó õ
|
0
R2
|
u1/2du dq |
| |
|
|
|
Gmm
r2
|
|
ó õ
|
2p
0
|
|
u3/2
3/2
|
ê ê
|
0
R2
|
dq |
| |
|
| |
|
|
|
However, the volume of the sphere is V = 4pR3/3, so that the mass of
the sphere is M = mV = m 4pR3/3. Thus, we have shown that
That is, a uniformly-dense spherical ''planet'' of mass M and a point-mass
of mass M at the center of the sphere have the same gravitational
attraction on a ''satellite'' point mass outside the sphere. Since the
electromagnetic force also satisfies an inverse square law, this result also
says that the electromagnetic force between spheres with uniform charge
density is equivalent to the electromagnetic force between point-charges.