From Keplers third law of planetary motion. The square of the period of revolution (T) of any planet around the sun is directly proportional to the cube of the semi major axis (X) of its elliptical orbit ie, T2∝R3
Given, Tp=27Te, Tp2Te2=Rp3Re3 (27Te)2Te2=Rp3Re3 ReRp=(27)2/3 ReRp=32Rp=9Re