This experiment was designed
to plot the light curves of four variable star candidates of an intermediary
magnitude range in order to determine if any were variables, and if so, what
type(s). Research was done using two 24" telescopes, located at Mt. Wilson
and Table Mountain. One star (R. A. 21h
43m 54.205s, Decl.
-00° 13' 40.12" (2000) was found to be variable, and the data indicate it
is a W Ursae Majoris-type eclipsing binary.