The formula for escape velocity ($v_e$) is $v_e = \sqrt{\frac{2GM}{R}}$, with G representing the gravitational constant, M the planet's mass, and R its radius.
For a new planet, its mass is $M' = 9M$ and its radius is $R' = 16R$.
Consequently, the new escape velocity is $v_e' = \sqrt{\frac{2G(9M)}{16R}} = \frac{3}{4}\sqrt{\frac{2GM}{R}} = \frac{3}{4}v_e$.