For a specific wavelength \( 670 \, \text{nm} \) of light coming from a galaxy moving with velocity \( v \), the observed wavelength is \( 670.7 \, \text{nm} \). The value of \( v \) is:
\( 3 \times 10^{8} \, \text{ms}^{-1} \)
\( 3 \times 10^{10} \, \text{ms}^{-1} \)
\( 3.13 \times 10^{5} \, \text{ms}^{-1} \)
\( 4.48 \times 10^{5} \, \text{ms}^{-1} \)