According to Kepler's third law (law of periods), T2∝R3
where T is time taken by the planet to go once around the sun R is semimajor axis (distance) of the elliptical orbit. =T2∝kR3
(where k is constant of proportionality)
When R becomes 4 times let time period be T'. =T2=k(4R)3 =T2T2=641
or T′T=81
or T′=8T
So, time period becomes 8 times of previous value.