The formula for gravitational acceleration
g = M*G/r2
where M is the mass of the planet, r is the radius of the planet, and G is the universal gravitational constant (G = 6.673×10-11 N.m2/Kg2, but you'll see that we won't need that value to answer the question).
so if we double the mass and triple the radius, our equation turns into
g_new = (2M)*G/(3r)2 = (2M)*G/(9r2)
note, all we did was replace the M by 2*M and the r by 3*r (which, was squared in the parenthesis). If we want to see the factor by which the acceleration due to gravity changes, we can simply divide
g_new/g = 2MG/(9r2) ÷ MG/r2 = 2MG/(9r2) × r2/(MG) = 2MGr2 / (9r2 MG) = 2/9 (G, M, and r2 all cancel out)
The new planet has an acceleration due to gravity that's 2/9 the strength of gravity of the original planet. If the planet was earth, our acceleration would change from 9.81 m/s2 —> 2.18 m/s2