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Question

In an experiment with a convex lens, the length of an image is 1 cm, and the object length is 5 cm. If the object is placed at a distance of 40 cm from the lens, then the focal length of the lens is

The correct answer is
6.67 cm

Convex Lens Focal Length Calculation

This problem involves calculating the focal length of a convex lens using information about the object and its image formed during an experiment. We will use the concepts of linear magnification and the lens formula.

Given Data Analysis

The following information is provided:

  • Image length ($L_i$): 1 cm
  • Object length ($L_o$): 5 cm
  • Object distance ($u$): 40 cm

Magnification Calculation Explained

Linear magnification ($m$) is defined as the ratio of the size of the image to the size of the object. It also relates the image distance ($v$) to the object distance ($u$).

The formula for magnification based on lengths is:

$ m = \frac{L_i}{L_o} $

Substituting the given values:

$ m = \frac{1 \text{ cm}}{5 \text{ cm}} = \frac{1}{5} $ $ m = 0.2 $

Since the image length is smaller than the object length, the magnification is less than 1, indicating that the image is diminished.

Lens Formula and Sign Convention

To find the focal length, we use the lens formula:

$ \frac{1}{f} = \frac{1}{v} - \frac{1}{u} $

We need to apply the standard sign conventions:

  • Object distance ($u$) is measured from the optical center. Since the object is placed in front of the lens, it is taken as negative: $u = -40$ cm.
  • For a convex lens forming a diminished image, it's usually a real image formed on the opposite side, meaning the image distance ($v$) is positive.
  • Magnification ($m$) is negative for real, inverted images. Thus, $m = -0.2$.

Image Distance Determination

We use the magnification formula relating distances:

$ m = \frac{v}{u} $

Substitute the known values of $m$ and $u$:

$ -0.2 = \frac{v}{-40 \text{ cm}} $

Solve for $v$:

$ v = (-0.2) \times (-40 \text{ cm}) $ $ v = 8 \text{ cm} $

The positive value for $v$ confirms that the image formed is real.

Focal Length Calculation

Now, substitute the values of $u$ and $v$ into the lens formula:

$ \frac{1}{f} = \frac{1}{v} - \frac{1}{u} $ $ \frac{1}{f} = \frac{1}{8 \text{ cm}} - \frac{1}{-40 \text{ cm}} $ $ \frac{1}{f} = \frac{1}{8 \text{ cm}} + \frac{1}{40 \text{ cm}} $

To add the fractions, find a common denominator, which is 40:

$ \frac{1}{f} = \frac{5}{40 \text{ cm}} + \frac{1}{40 \text{ cm}} $ $ \frac{1}{f} = \frac{6}{40 \text{ cm}} $

Simplify the fraction:

$ \frac{1}{f} = \frac{3}{20 \text{ cm}} $

Calculate the focal length ($f$) by taking the reciprocal:

$ f = \frac{20}{3} \text{ cm} $ $ f \approx 6.67 \text{ cm} $

The calculated focal length is positive, which is characteristic of a convex lens.

Conclusion

The focal length of the convex lens is calculated to be approximately 6.67 cm.

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Important Questions from Ray Optics and Optical Instruments

  1. A Convex mirror produces the magnification 1/3 and 1/4 when the object is placed at the points P and Q in front of the mirror.

  2. Which of the following statements are correct?

    • A. The saturation current is constant with collector plate potential for different frequencies of incident radiation.
    • B. The saturation current is different with collector plate potential for different frequencies of incident radiation.
    • C. The saturation current is different with collector plate potential for different intensity of incident radiation.
    • D. The saturation current is constant with collector plate potential for different intensity of incident radiation.
    • E. Below threshold frequency, no photoelectrons are emitted.

    Choose the correct answer from the options given below:

  3. For insulators and semiconductors, the resistance decreases with an increase in temperature because:

  4. A ray of light passes through four transparent media with refractive index μ1, μ2, μ3, and μ4 as shown in the figure. The surfaces of all media are parallel. If BC and DE are parallel, we must have:

  5. Light of uniform intensity shines perpendicularly on a totally absorbing surface, fully illuminating the surface. If the area of the surface is decreased, what is the effect on radiation pressure?

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