  Two sets of photometric observations of the system AH Tauri have been
analyzed using the latest version of the Wilson-Devinney code. The results show
that AH Tauri may classified as A-type of W-UMa eclipsing binary. The mass
ratio of q = 0.81, an over-contact degree of f = 0.095, and a slightly
temperature difference between the two components have been obtained. The
asymmetry of its light curve explained by the presence of a dark spot on the
massive component. The physical, geometrical, and absolute parameters have been
derived and compared with previous work.
