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The wavelength of light received from a ...

The wavelength of light received from a galaxy is 10% greater than that received from identical source on the earth. The velocity of the galaxy relative to the earth is

A

A) `3xx 10^(8) ms^(-1)`

B

B) `3xx 10^(7) ms^(-1)`

C

C) `3xx 10^(6) ms^(-1)`

D

D) `3xx 10^(5) ms^(-1)`

Text Solution

AI Generated Solution

The correct Answer is:
To solve the problem, we need to find the velocity of the galaxy relative to the Earth based on the change in wavelength of light received from it. Here’s a step-by-step solution: ### Step 1: Understand the Given Information We are given that the wavelength of light received from a galaxy is 10% greater than that received from an identical source on Earth. This means: - If the original wavelength (λ) is received from Earth, the wavelength from the galaxy (λ') can be expressed as: \[ \lambda' = \lambda + 0.1\lambda = 1.1\lambda \] ### Step 2: Calculate the Change in Wavelength The change in wavelength (Δλ) is given by: \[ \Delta \lambda = \lambda' - \lambda = 1.1\lambda - \lambda = 0.1\lambda \] ### Step 3: Use the Formula for Velocity We can relate the change in wavelength to the velocity of the galaxy using the formula: \[ V = \frac{\Delta \lambda}{\lambda} \cdot c \] where: - \( V \) is the velocity of the galaxy relative to Earth, - \( c \) is the speed of light (approximately \( 3 \times 10^8 \) m/s). ### Step 4: Substitute the Values From the previous steps, we have: \[ \frac{\Delta \lambda}{\lambda} = 0.1 \] Substituting this into the velocity formula gives: \[ V = 0.1 \cdot c = 0.1 \cdot (3 \times 10^8 \text{ m/s}) \] ### Step 5: Calculate the Velocity Now, calculate the velocity: \[ V = 0.1 \cdot 3 \times 10^8 = 3 \times 10^7 \text{ m/s} \] ### Step 6: Identify the Correct Option The calculated velocity \( V = 3 \times 10^7 \text{ m/s} \) corresponds to option B. ### Final Answer The velocity of the galaxy relative to the Earth is: \[ \boxed{3 \times 10^7 \text{ m/s}} \] ---
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Knowledge Check

  • The escape velocity from the surface of the earth is (where R_(E) is the radius of the earth )

    A
    `sqrt(2gR_(E))`
    B
    `sqrt(gR_(E))`
    C
    `2sqrt(gR_(E))`
    D
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  • The wavelength of spectral line coming from a distant star shifts from 600 nm to 600.1 nm. The velocity of the star relative to earth is

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    B
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    C
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    D
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  • Light from the sun reaches the earth approximately in

    A
    5s
    B
    50s
    C
    500s
    D
    0.5s
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