You can use the semi-major axis as R in Kepler's 3rd Law (it is the avg R for an elliptical orbit)
ksunR3 = T2 for all satellites of the sun. If we use earth years and astronomical units, k = 1 (because the earth has an R = 1AU and a period of 1 year)
T = sqrt(R3) in years.
Please consider a tutor.