We report several new reliable times of minimum of the eccentric eclip
sing binary OX Cas (P = 2.48934 days E = 0.04, V = 9.92 mag, B2V + B2V
). The O-C diagram is analyzed found in the literature and improved va
lues for the elements of the apsidal motion and the internal structure
constant are computed. We have found a short period of apsidal motion
U = 37.3 +/- 0.7 yr and the internal structure constant (k) over bar(
2,obs) = 0.0060.