Chapter 7, Problem # 5
Chapter 7, Problem # 6
Chapter 8, Problem # 2
Kepler's third law: a3 = P2 (where a is given in
AU and P is given in years)
rearranging the equation, we get: P = a3/2
plugging in a for the comet yields: P = (105)3/2 =
3.16 × 107 years
So a typical comet from the Oort cloud returns to the inner solar
system about once every 3.16 × 107 years.
Chapter 8, Problem # 6
a) The warning time would be the time it took the asteroid to travel
the 15 million kilometers to the Earth. We assume that the asteroid
is moving at a speed of 15 km/sec.
velocity = distance/time
time = distance/velocity
time = 15,000,000 km / (15 km/sec)
time = 1,000,000 sec × (1 day / 86400 sec)
time = 11.6 days
b) A kilometer-sized asteroid impact is equivalent to the explosion
of a bomb with a yield of hundreds to thousands of megatons (ie.
several extremely large nuclear explosions). Thus the shock wave
from the impact would cause devastation over a large area. Also,
the impact would raise a large dust cloud which could block out
the Sun for weeks or months.
c) If an asteroid (assumed to be traveling at approximately 15 km/sec as
in part a) were discovered when it was 384,000 km from the earth, the warning
time would be (as in part a):
time = distance/velocity
time = 384,000 km / (15 km/sec)
time = 25600 sec × (1 hr / 3600 sec)
time = about 7 hours
d) Assuming that the asteroid is not substantially slowed down by the
earth's atmosphere, we can determine the time it would take the asteroid
to pass through the 100 km thickness of the atmosphere using the same
method as was used in parts a) and c):
time = distance/velocity
time = 100 km / (15 km/sec)
time = 6.7 seconds
Chapter 9, Problem # 3
From this equation, we see than since the mass of Europa is less than the
mass of our Moon, and the radius of Europa is approximately equal to the
radius of our Moon, the force of gravity on Europa would be less than the
force of gravity on our Moon.