(c) From Hubble ‘s law
$\ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ Z\ \propto r$
Where $Z \rightarrow$ red shift, $r \rightarrow$distance of the galaxy
Also, $\ \ \ \ \ \ \ \ Z = \frac{d\lambda}{\lambda}$ $=$ $\frac{v}{c}\ =$ $\frac{speed\ of\ galaxy}{speed\ of\ light}$
Given $d\lambda$ $= \ 401.8\ - 393.3 = 8.5\ nm,$
$\ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \lambda = 393.3\ nm$,
$\ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ Z\ = \frac{8.5}{393.3}$ $= 0.0216$
Also$\ \ \ \ \ \ \ \ v = cZ$
$\ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ = 3\ \times \ 10^{8} \times 0.0216$
$\ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ = 64.8\ \times \ 10^{5}{ms}^{- 1}\ $
Since$\ \ \ 1km\ = \ 10^{3}m\ ,\ therefore$
$\ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ v = 6480\ {kms}^{- 1}$