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Two slits are separated by a distance of...

Two slits are separated by a distance of `0.5mm` and illuminated with light of `lambda=6000Å`. If the screen is placed `2.5m` from the slits. The distance of the third bright image from the centre will be

A

1.5 mm

B

3mm

C

6 mm

D

9 mm

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The correct Answer is:
To find the distance of the third bright fringe from the center in a double-slit interference pattern, we can use the formula for the position of the bright fringes: \[ y_n = \frac{n \lambda D}{d} \] Where: - \( y_n \) = distance of the nth bright fringe from the center - \( n \) = order of the bright fringe (in this case, \( n = 3 \)) - \( \lambda \) = wavelength of the light (in meters) - \( D \) = distance from the slits to the screen (in meters) - \( d \) = distance between the slits (in meters) ### Step-by-Step Solution: 1. **Convert the given values to appropriate units:** - Wavelength \( \lambda = 6000 \, \text{Å} = 6000 \times 10^{-10} \, \text{m} = 6 \times 10^{-7} \, \text{m} \) - Distance between the slits \( d = 0.5 \, \text{mm} = 0.5 \times 10^{-3} \, \text{m} = 5 \times 10^{-4} \, \text{m} \) - Distance from the slits to the screen \( D = 2.5 \, \text{m} \) 2. **Substitute the values into the formula for the third bright fringe (n = 3):** \[ y_3 = \frac{3 \cdot \lambda \cdot D}{d} \] 3. **Plug in the values:** \[ y_3 = \frac{3 \cdot (6 \times 10^{-7} \, \text{m}) \cdot (2.5 \, \text{m})}{5 \times 10^{-4} \, \text{m}} \] 4. **Calculate the numerator:** \[ 3 \cdot (6 \times 10^{-7}) \cdot (2.5) = 4.5 \times 10^{-6} \, \text{m} \] 5. **Now divide by \( d \):** \[ y_3 = \frac{4.5 \times 10^{-6} \, \text{m}}{5 \times 10^{-4} \, \text{m}} = 9 \times 10^{-3} \, \text{m} \] 6. **Convert the result to micrometers:** \[ 9 \times 10^{-3} \, \text{m} = 9 \, \text{mm} \] ### Final Answer: The distance of the third bright image from the center is \( 9 \, \text{mm} \).

To find the distance of the third bright fringe from the center in a double-slit interference pattern, we can use the formula for the position of the bright fringes: \[ y_n = \frac{n \lambda D}{d} \] Where: - \( y_n \) = distance of the nth bright fringe from the center - \( n \) = order of the bright fringe (in this case, \( n = 3 \)) - \( \lambda \) = wavelength of the light (in meters) ...
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