The square of the planets time period is proportional to the cube of the semi-major axis of its orbit. T2∝R3
where R is the distance of earth from the sun.
or (T1T2)2=(R1R2)3
Given, R1=R,R2=4R,T1=T ∴TT2=(RR/4)3/2 =(41)3/2=81
or T2=8T
Hence, the duration of the year will be one-eighth the present year.