Calculating the velocity of a moving source in the context of the Doppler effect involves determining the speed at which the source is approaching or receding from the observer. This is done using the relativistic Doppler effect formula.
The formula relates the observed frequency \( f' \) to the rest frequency \( f \), using the equation \( f' = f \sqrt{\frac{1 + \beta}{1 - \beta}} \), where \( \beta = \frac{v}{c} \). Here, \( v \) is the velocity of the source and \( c \) is the speed of light.
To find the velocity \( v \), we first solve for \( \beta \). This process involves:
- Substituting the known values into the formula.
- Rearranging and solving the equation for \( \beta \).
- Multiplying \( \beta \) by the speed of light \( c \) to find \( v \).
In our solution, we found \( \beta \) to be approximately 0.2196, indicating that the source is moving at 21.96% the speed of light toward the observer.