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7. At the point where the forces balance
22
12
//
es
GM m r
GM m r
=
, where
M
e
is the mass of
Earth,
M
s
is the mass of the Sun,
m
is the mass of the space probe,
r
1
is the distance from
the center of Earth to the probe, and
r
2
is the distance from the center of the Sun to the
probe. We substitute
r
2
=
d
−
r
1
, where
d
is the distance from the center of Earth to the
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This note was uploaded on 05/17/2011 for the course PHY 2049 taught by Professor Any during the Spring '08 term at University of Florida.
 Spring '08
 Any
 Physics, Force, Mass

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