2. This problem relates to Kepler's
Third Law. In this problem you will use the power law to determine the
period of revolution about or distance from the sun for all planets given information
about some of the planets. Let d be the mean distance
(x106 km)
from the sun and p be the period of
revolution in days about the sun. You are given the following data [1] concerning
four of the planets:
Planet
|
Distance d
|
Period p
|
Mercury
|
57.9
|
87.96
|
Earth
|
149.6
|
365.25
|
Mars
|
227.9
|
687.0
|
Jupiter
|
778.3
|
4337
|
b. In class, we will show that an
allometric (power law) model has a straight line fitting the
logarithms of data, giving
c. Use the power law found in part a.
to complete the table below:
Planet
|
Distance d
|
Period p
|
Venus
|
108.2
|
|
Saturn
|
|
10,760
|
Uranus
|
2871
|
|
Neptune
|
4497
|
|
Pluto
|
|
90,780
|
[1] Jay M. Pasachof, (1993) Astronomy: From the Earth to the Universe, Fourth Edition, Saunders College Publishing.