By equating the centripetal force and the gravitational pull, we have the equation

where
G=gravitational constant=6.67408*10^(-11) (m^3 kg^-1 s^-2)
m=mass of object
M=mass of sun=1.9885*10^(30) (kg)
v=tangential velocity of object
r=distance from the sun (m)
On simplification, we get the relation

(m/s)
Subtituting constants,including
1 au = 1.49597870700*10^(11) m
and given
r=5 au = 7.47989*10^11 m

m/s
Therefore the orbital period is

s

years

years