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:
![T=\sqrt[]{(a^3)/(k)}=\sqrt[]{((0.312AU)^3)/(1.00(AU^3)/(yr^2))}\approx0.56yr](https://img.qammunity.org/2023/formulas/physics/college/8ywi2cphqmh11m9mh1dxyhcfc4zrv2f1us.png)
Hence, the Mercury's orbital period is approximately 0.56 yr