C) 4
The terminal velocity is given by v, where v \(\propto\) r2 (r = radius of the sphere).
The mass of the sphere can be given by
\(m\) = \(\frac{4}{3}\pi r^3\rho,\) Thus \(m\propto r^3\)
\(\frac{m_1}{m_2}\) = \(\frac{1}{8}\) =(\(\frac{r_1}{r^2}^3\)) \(\Rightarrow\frac{r_1}{r_2}\)= \(\frac{1}{2}\)
and since, \(\frac{v_1}{v_2}\)= (\(\frac{r_1}{r_2}\))2 = \(\frac{1}{4}\)
\(\Rightarrow \frac{v}{nv} = \frac{1}{4}\)
\(\Rightarrow n=4\)