The speed of light is 3.00 × 108 m/s.

At Earth, the wavelength of a spectral line detected from the distant galaxy G\mathbf{G}G is different from the wavelength emitted in a stationary laboratory.
The difference in wavelength (wavelength shift) is 12 nm12\text{ nm}12 nm.
The rest wavelength that the source emits is 600 nm600\text{ nm}600 nm.
Calculate the recessional velocity of galaxy G\mathbf{G}G.
Use the equation:
velocity of galaxy G=speed of light×wavelength shiftrest wavelength emitted \text{velocity of galaxy } \mathbf{G} = \frac{\text{speed of light} \times \text{wavelength shift}}{\text{rest wavelength emitted}} velocity of galaxy G=rest wavelength emittedspeed of light×wavelength shiftGive your answer in standard form.