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The spectral line for a given element in...

The spectral line for a given element in the light received from a distant star is shifted towards longer wavelength side by `0.025%`. Calculate the velocity of star in the line of sight.

A

`7.5xx10^(4)ms^(-1)`

B

`-7.5xx10^(4)ms^(-1)`

C

`3.7xx10^(4)ms^(-1)`

D

`-3.7xx10^(4)ms^(-1)`

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The correct Answer is:
To solve the problem of determining the velocity of the star in the line of sight based on the redshift of a spectral line, we can follow these steps: ### Step-by-Step Solution: 1. **Understanding Redshift**: The problem states that the spectral line is shifted towards longer wavelengths by 0.025%. A shift towards longer wavelengths indicates a redshift, which means the star is moving away from us. 2. **Expressing the Redshift**: The redshift \( z \) can be expressed in terms of the change in wavelength \( \Delta \lambda \) and the original wavelength \( \lambda \): \[ z = \frac{\Delta \lambda}{\lambda} \] Given that the shift is 0.025%, we can express this as: \[ z = \frac{0.025}{100} = 0.00025 \] 3. **Relating Redshift to Velocity**: The velocity \( V \) of the star can be calculated using the formula: \[ V = z \cdot c \] where \( c \) is the speed of light, approximately \( 3 \times 10^8 \) m/s. 4. **Calculating the Velocity**: Substituting the value of \( z \) into the equation: \[ V = 0.00025 \cdot (3 \times 10^8 \text{ m/s}) \] 5. **Performing the Calculation**: \[ V = 0.00025 \times 3 \times 10^8 = 0.00075 \times 10^8 = 7.5 \times 10^4 \text{ m/s} \] 6. **Interpreting the Result**: Since this is a redshift, the velocity will be negative, indicating that the star is moving away from us: \[ V = -7.5 \times 10^4 \text{ m/s} \] ### Final Answer: The velocity of the star in the line of sight is approximately \( -7.5 \times 10^4 \) m/s. ---

To solve the problem of determining the velocity of the star in the line of sight based on the redshift of a spectral line, we can follow these steps: ### Step-by-Step Solution: 1. **Understanding Redshift**: The problem states that the spectral line is shifted towards longer wavelengths by 0.025%. A shift towards longer wavelengths indicates a redshift, which means the star is moving away from us. 2. **Expressing the Redshift**: The redshift \( z \) can be expressed in terms of the change in wavelength \( \Delta \lambda \) and the original wavelength \( \lambda \): \[ ...
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