284 Solutions Manual
Problem 2.214
A satellite is moving along the elliptical orbit shown. Using the polar
coordinate system in the figure, the satellite’s orbit is described by
the equation
r.✓/D2b2aCpa2b2cos ✓
a2Cb2.a2b2/cos.2✓/;
which implies the following identity
rr00 2.r0/2r2
r3Da
b2;
where the prime indicates differentiation with respect to
✓
. Using
this identity and knowing that the satellite moves so that
KDr2P
✓
with
K
constant (i.e., according to Kepler’s laws), show that the
radial component of acceleration is proportional to 1=r2, which is
in agreement with Newton’s universal law of gravitation.
Solution
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