Lets consider a distance of dr at a distance of r from center of earth.
now, dt=dr−v [since the velocity is towards the center of earth]
Energy is conserved , Initial = final energy
So, −GMmR+2mGM2=mv22+−GMm2R3(3R2−r2)
solving this, we get v=(GM(3R2−r2)R3)0.5
dt=dr−(GM(3R2−r2)R3)0.5
Integrating on both sides with limits from 0 to R
T=sin−1(130.5)(R3GM)0.5=sin−1(130.5)(Rg)0.5
So, x=3