Kris Green: Math 223, Section 2
Fall 1998: Due Friday, August 28
The following function shows up in celestial mechanics:

 is a parameter that is fixed.  The physical situation (not
necessary for working the problem) is that a large mass, say the earth, is
located at
 is a parameter that is fixed.  The physical situation (not
necessary for working the problem) is that a large mass, say the earth, is
located at  and a smaller mass, say the moon, at
 and a smaller mass, say the moon, at  .The coordinates are chosen so that the center of mass of the two objects is
at (0,0) and the coordinates rotate around the center of mass at the proper
rate.  The function then gives the set of points where a third mass that is
very small (say a satellite) would have zero orbital velocity.  The
function is used to find stable orbits for various situations.
.The coordinates are chosen so that the center of mass of the two objects is
at (0,0) and the coordinates rotate around the center of mass at the proper
rate.  The function then gives the set of points where a third mass that is
very small (say a satellite) would have zero orbital velocity.  The
function is used to find stable orbits for various situations.
The Problem:  Start with  and choose
and choose  to view the function above in WinPlot.  Note
that this function is way too complicated to visualize without some sort of
help.
 to view the function above in WinPlot.  Note
that this function is way too complicated to visualize without some sort of
help.
 near the
points
 near the
points  and
 and  ?  Why or why not?  [Hint:  look at the
algeraic form of the function.]
?  Why or why not?  [Hint:  look at the
algeraic form of the function.]
 have on the surface?  [For example,
try
 have on the surface?  [For example,
try  or 0.2.]
 or 0.2.]
Getting Help: I will hold my office hours in Math 226 (the open access computer lab) for the rest of the week. This should allow you sufficient time to play with WinPlot and get an idea of what it can do for you.