The Doppler shift formula for the wavelength change when the source is moving away from the observer is: \[ \frac{\Delta \lambda}{\lambda} = \frac{v}{c} \] where: - \( \Delta \lambda = \lambda' - \lambda \) is the change in wavelength, - \( v \) is the velocity of the galaxy relative to Earth, - \( c \) is the speed of light. Substituting the values: \[ \frac{601 - 600}{600} = \frac{v}{3 \times 10^8} \] \[ \frac{1}{600} = \frac{v}{3 \times 10^8} \] Solving for \( v \): \[ v = \frac{3 \times 10^8}{600} = 500 \, \text{km/s} \]
The speed of the galaxy with respect to Earth is \( {500 \, \text{km/s}} \), so the correct answer is (A).
List- I (Layer of atmosphere) | List- II (Approximate height over earth's surface) | ||
A. | F1-Layer | I. | 10 km |
B. | D-Layer | II. | 170-190 km |
C. | Troposphere | III. | 100 km |
D. | E-layer | IV. | 65-75 km |