A comparative analysis of the special shapes (patterns, profiles) of the eclipses applied for the phenomenological modeling of the light curves of eclipsing binary stars is conducted. Families of functions are considered, generalizing local approximations (Andronov, 2010(Andronov, , 2012 and the functions theoretically unlimited in a width, based on a Gaussian (Mikulášek, 2015). For an analysis, the light curve of the star V0882 Car = 2MASS J11080308 -6145589 of the classic Algolsubtype ( Persei) is used. By analyzing dozens of modified functions with additional parameters, it was chosen the 14 best ones according to the criterion of the least sum of squares of deviations. The best are the functions with an additional parameter, describing profiles, which are limited in phase.