P16 072

background image

72. The speed of the submarine going eastward is

v

east

= v

equator

+ v

sub

where v

sub

= 16000/3600 = 4.44 m/s. The term v

equator

is the speed that any point at the equator (at

radius R = 6.37

× 10

6

m) would have in order to keep up with the spinning earth. With T = 1 day =

86400 s, we note that v

equator

= = R2π/T = 463 m/s and is much larger than v

sub

. Similarly, when

it travels westward, its speed is

v

west

= v

equator

− v

sub

.

The effective gravity g

e

(or apparent gravity) combines the gravitational pull of the earth g (which

cancels when we take the difference) and the effect of the centripetal acceleration v

2

/R. Considering the

two motions of the submarine, the difference is therefore

g

e

= g



e

− g

e

=

v

2

east

R

v

2

west

R

=

1

R



(v

equator

+ v

sub

)

2

(v

equator

− v

sub

)

2



=

4v

equator

v

sub

R

=

8πv

sub

T

where in the last step we have used v

equator

= R2π/T . Consequently, we find

g

e

g

=

8πv

sub

gT

=

8π(4.44)

(9.8)(86400)

= 1.3

× 10

4

.

The problem asks for ∆g/g for either travel direction, and since our computation examines eastward
travel as opposed to westward travel, then we infer that either-way travel versus no-travel should be half
of our result. Thus, the answer to the problem is

1
2

(1.3

× 10

4

) = 6.6

× 10

5

.


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