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The sun subtends asn angle of (1//2)^(@)...

The sun subtends asn angle of `(1//2)^(@)` on earth. The image of sun is obtained on the screen with the help of a convex lens of focal length 100 cm the diameter of the image obtained on the screen will be

A

`18 cm`

B

`1mm`

C

`50 cm`

D

`8.73 mm`

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The correct Answer is:
To solve the problem, we need to find the diameter of the image of the sun formed by a convex lens with a given focal length when the sun subtends an angle of \( \frac{1}{2}^\circ \) at the earth. ### Step-by-Step Solution: 1. **Understanding the Geometry**: The sun subtends an angle \( \theta = \frac{1}{2}^\circ \) at the earth. This angle can be used to find the size of the image formed by the lens. 2. **Convert the Angle to Radians**: To use the angle in calculations, we need to convert degrees to radians. The conversion formula is: \[ \text{radians} = \text{degrees} \times \frac{\pi}{180} \] Therefore, \[ \theta = \frac{1}{2} \times \frac{\pi}{180} = \frac{\pi}{360} \text{ radians} \] 3. **Using the Lens Formula**: When the object (the sun) is at a very large distance (effectively at infinity), the image is formed at the focal point of the lens. The diameter of the image can be calculated using the formula: \[ x = f \cdot \theta \] where \( f \) is the focal length of the lens. 4. **Substituting the Values**: Given that the focal length \( f = 100 \) cm, we can substitute the values: \[ x = 100 \cdot \frac{\pi}{360} \] 5. **Calculating the Diameter**: Now, we compute \( x \): \[ x = 100 \cdot \frac{3.14}{360} \approx 8.73 \text{ cm} \] Since the question asks for the diameter, we can directly use this value. 6. **Converting to Millimeters**: To express the diameter in millimeters, we convert centimeters to millimeters: \[ 8.73 \text{ cm} = 8.73 \times 10 = 87.3 \text{ mm} \] ### Final Answer: The diameter of the image obtained on the screen is approximately **8.73 mm**.

To solve the problem, we need to find the diameter of the image of the sun formed by a convex lens with a given focal length when the sun subtends an angle of \( \frac{1}{2}^\circ \) at the earth. ### Step-by-Step Solution: 1. **Understanding the Geometry**: The sun subtends an angle \( \theta = \frac{1}{2}^\circ \) at the earth. This angle can be used to find the size of the image formed by the lens. 2. **Convert the Angle to Radians**: ...
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