Kepler's Third
Law
Background
At
the end of the 16th century, the great astronomer Tycho Brahe spent
decades making the most complete and accurate measurements of the positions and
movements of the planets in the history of the world. His data were as accurate as possible before the invention of the
telescope (which occurred after his death).
Contained within Tycho's data lay the truth of the motions of the
planets. It was Tycho's assistant, the
German mathematician Johannes Kepler, who extracted this truth. Kepler developed a mathematical model for the motion of the planets which fit Tycho's
data.
Kepler
discoveries are now known as Kepler's Laws.
The first and second laws were published in 1609. The first law describes the shape of
planetary orbits:

The orbit of a planet about
the Sun is an ellipse with the Sun at one focus.
The
second law describes how a planet's orbital speed varies as it travels around
the sun. Kepler realized that planets
move more quickly when they are closer to the Sun. His second law makes this precise:
A line joining a planet and the Sun sweeps out equal
areas in equal intervals of time.
Kepler's
first two laws describe the motion of a single planet. His third law compares the motions of different planets. The third law says that the sidereal period
of a planet (the time it takes the planet to travel once around the Sun) is
related to the semimajor axis of the orbit (the average distance of the planet
from the Sun). Your job is to
rediscover Kepler's third law.
Data and Questions
You
will deduce Kepler's third law from the data below (don't cheat and look it
up!). We want to know whether the
relationship between the sidereal period and the semimajor axis is linear,
exponential, logarithmic, a power function, or none of these. We will measure the sidereal period in years
and the semimajor axis in millions of miles.
|
Planet |
Sidereal Period (years) |
Semimajor axis (106 mi) |
|
Mercury |
0.24 |
36.25 |
|
Venus |
0.61 |
66.92 |
|
Earth |
1.00 |
92.96 |
|
Mars |
1.88 |
141.29 |
|
Jupiter |
11.86 |
483.37 |
|
Saturn |
29.46 |
886.80 |
|
Uranus |
84.01 |
1783.83 |
|
Neptune |
164.79 |
2794.26 |
|
Pluto |
248.54 |
3674.55 |
1.
Graph
the data points. Eyeballing the data,
is there a relationship between the two variables? What kind of relationship might it be?
2.
Find
the line which best fits the data (using linear regression). How good a fit is this line?
3.
Graph
the log plots of the data, and use it to find the exponential and logarithmic
functions which best fits the data. How
good are the fits?
4.
Graph
the log-log plot of the data, and use it to find the power function which best
fits the data. How good is the fit?
5.
Graph
the best of your models together with the data. What is Kepler's third law?
Would another choice of units make the law simpler?
(The
background information and data for this project were adapted from Universe, Kauffman and Freedman, 5th
edition.)