Kris Green: Math 223, Section 2
Fall 1998: Due Friday, August 28
The following function shows up in celestial mechanics:
where 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 .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 to view the function above in WinPlot. Note that this function is way too complicated to visualize without some sort of help.
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.