p14 045

background image

45.

(a) If r is the radius of the orbit then the magnitude of the gravitational force acting on the satellite

is given by GM m/r

2

, where M is the mass of Earth and m is the mass of the satellite. The

magnitude of the acceleration of the satellite is given by v

2

/r, where v is its speed. Newton’s

second law yields GM m/r

2

= mv

2

/r. Since the radius of Earth is 6.37

× 10

6

m the orbit radius is

r = 6.37

× 10

6

m + 160

× 10

3

m = 6.53

× 10

6

m. The solution for v is

v =



GM

r

=



(6.67

× 10

11

m

3

/s

2

·kg)(5.98 × 10

24

kg)

6.53

× 10

6

m

= 7.82

× 10

3

m/s .

(b) Since the circumference of the circular orbit is 2πr, the period is

T =

2πr

v

=

2π(6.53

× 10

6

m)

7.82

× 10

3

m/s

= 5.25

× 10

3

s .

This is equivalent to 87.4 min.


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