(d) $\frac{\Delta\lambda}{\lambda} = \frac{v}{c}$, Now $\Delta\lambda = \frac{0.5}{100}\lambda \Rightarrow \frac{\Delta\lambda}{\lambda} = \frac{0.5}{100}$
$\therefore v = \frac{0.5}{100} \times c = \frac{0.5}{100} \times 3 \times 10^{8} = 1.5 \times 10^{6}m/s$
Increase in $\lambda$ indicates that the star is receding