From Kepler's 3rd laws of planetary motion we know that
T^2= kR^3
where
K is a constant
T is orbital period = 365 days for earth.
R is semi-major axis of orbit.
Taking the ratio,
(T1/T2)^2 = (R1/R2)^3
Putting, T1 = 365 days, R1=R, R2 =R/2
We get
(365/T2)^2 = (R/(R/2))^3
(365/T2)^2 = 2^3 = 8
T2^2 = 365^2 / 8
T2=129.04
Therefore, Number of days in one year will be about 129 days.