Take into account that by the Kepler's Third Law, you can use the following formula:
where,
T: period of Mercury
a: average distance from Mercuty to Sun = 0.312AU
k: Kepler's constant = 1.00 AU^3/yr^2
Then, by replacing the previous values of the parameters, you obtain for T:
Hence, the Mercury's orbital period is approximately 0.56 yr