Lens maker’s formula
It is given by
\(\frac{1}{f} = (\mu - 1)(\frac{1}{R_1} -\frac{1}{R_2})\)
This formula relates the focal length of the lens of the radii of curvature of the surfaces and the refractive index of the material of the lens.
Why is it called lens maker’s formula?
It is so called because this formula is used by the manufacturers to prepare lenses of desired focal lengths.
Sign conventions
- All the distances are measured from the optical centre of lens.
- Distance measured in the direction of incident light is taken +ve.
- Distance measured in the direction opposite to the direction of incident light is taken -ve.
Assumptions
- Object is a point object.
- Lens is thin so that distances are measured from the poles of its surfaces.
- The aperture of the lens is small.
- Angles of incidence and refraction are small.
Let C1 and C2 be centres of curvature of two spherical surfaces XP1Y and XP2Y with optical centre C. Let µ2 be the refractive index of the material of the lens and µ1 that of the medium surrounding the lens where µ2 > µ1.
Refraction at surface XP1Y
Let a ray OA starts from the point object O which is placed on the principal axis of the convex lens and it refracts into the denser medium at point A. The refracted ray AB goes undeviated to meet at point I1, if the lens material were continued. Then I1 would be the real image of point object O.
From Snell’s law for small i1 and r1, we have
\(\frac{sin\ i}{\sin r_1} = \frac{i_1}{r_1} = \frac{\mu_2}{\mu_1}\)
or µ1 i1 = µ2 r1 ..........(1)
In ∆ AOC1,
i1 = α1 + γ1
In ∆ AI1C1,
γ1 = ß1 + r1
or r1 = γ1 - ß1
Putting the values of i1 and r1 in Eq.(1), we get
µ1 (α1 + γ1) = µ2 (γ1 - ß1)
or µ1α1 + µ1γ1 = µ2γ1 - µ2ß1
or µ1α1 + µ2ß1 = (µ2 - µ1) γ1
Since α1, ß1 and γ1 are small, so they can be replaced by their tangents.
∴ µ1 tan α1 + µ2 tan ß1 = (µ2 - µ1) tan γ1
Refraction at surface XP2Y
Actually the lens is not continuous and the ray AB suffer refraction at B and finally meet at I. So I is the real image of the virtual object I1 (placed in the material of the lens).
From Snell’s law for small i2 and r2, we have
\(\frac{sin\ i_2}{\sin r_2} = \frac{i_2}{r_2} = \frac{\mu_1}{\mu_2}\)
or µ1r2 = µ1i2 ..........(3)
In ∆ BC2I1,
i2 = ß1 + γ2
In ∆ BC2I, r2 = ß2 + γ2
Putting the value of i2 and r2 in Eq. (3), we get
µ1 (ß2 + γ2) = µ2 (ß1 + γ2)
or µ1ß2 + µ1γ2 = µ2ß1 + µ2γ2
or µ1ß2 - µ2ß1 = (µ2 - µ1) γ2
Since ß2, ß1 and γ2 are small, so they can be replaced by their tangents, so
µ1 tan ß2 - µ2 tan ß1 = (µ2 - µ1) tan γ2