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Q.Write the lens maker's formula. Why is this formula useful? Double-convex lenses are to be manufactured from a glass of refractive index 1.55 with both faces of the same radius of curvature. What is the radius of curvature required if the focal length is to be 20 cm?

(OR)
Define the magnifying power of an optical instrument. Draw a ray diagram for an astronomical telescope when the final image is formed at infinity, and write the formula for its magnifying power.
Uttarakhand UbseUttarakhand Board Intermediate (Class 12) 2024Subjective· 4mImportance★★★★★
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Figure — The OR alternative instructs 'Draw a ray diagram for an astronomical telescope when the final image is formed
Figure — The OR alternative instructs 'Draw a ray diagram for an astronomical telescope when the final image is formed

Lens maker's formula relates ff to the material's refractive index and the two surface curvatures; for an equi-curved biconvex lens it simplifies neatly.

Lens maker's formula:

1f=(μ−1)(1R1−1R2)\frac{1}{f}=(\mu-1)\left(\frac{1}{R_1}-\frac{1}{R_2}\right)

where ff is the focal length, μ\mu the refractive index of the lens material relative to the surrounding medium, and R1,R2R_1,R_2 the radii of curvature of its two surfaces (with the usual sign convention).

Why it is useful: it lets an optician/lens manufacturer calculate the focal length a lens will have, given only the refractive index of the glass used and the curvatures ground onto its two faces — or, conversely, work out what curvatures are needed to manufacture a lens of a desired focal length from a given glass, without having to measure the focal length experimentally each time.

Numerical part. For a double-convex (biconvex) lens with both faces of equal radius of curvature magnitude RR: by the sign convention, the first (convex towards the incoming light) surface has R1=+RR_1=+R and the second (also convex, curving away) has R2=−RR_2=-R. So:

1f=(μ−1)(1R−1−R)=(μ−1)2R\frac{1}{f}=(\mu-1)\left(\frac{1}{R}-\frac{1}{-R}\right)=(\mu-1)\frac{2}{R}

Given μ=1.55\mu=1.55 and f=20 cmf=20\ \text{cm}:

120=(1.55−1)×2R=0.55×2R=1.1R\frac{1}{20}=(1.55-1)\times\frac{2}{R}=0.55\times\frac{2}{R}=\frac{1.1}{R}

R=1.1×20=22 cmR=1.1\times20=22\ \text{cm}


OR — Astronomical telescope.

Magnifying power of an optical instrument is defined as the ratio of the angle subtended at the eye by the final (virtual) image formed by the instrument, to the angle subtended at the (unaided) eye by the object when viewed directly:

m=βαm=\frac{\beta}{\alpha}

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