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Class XII/Chapter 9: Ray Optics and Optical Instruments/Thin Lens Formula and Magnification

Thin Lens Formula and Magnification

For a thin lens of focal length ff in air, the object and image distances satisfy the lens equation.

Concept

Thin lens formula:

1v1u=1f\frac{1}{v} - \frac{1}{u} = \frac{1}{f}

Linear magnification:

m=hh=vum = \frac{h'}{h} = \frac{v}{u}

(Both uu and vv are measured with the Cartesian sign convention; signs of hh and hh' follow.)

  • A converging lens has f>0f > 0.
  • A diverging lens has f<0f < 0.
  • For a real object (u<0u < 0) in a converging lens, the image is real and inverted when u>f|u| > f; virtual and erect when u<f|u| < f.

Derivation

The lens formula follows directly from the lens-maker's derivation: adding the two single-surface relations gave

1v1u=(n1)(1R11R2)=1f\frac{1}{v} - \frac{1}{u} = (n - 1)\left(\frac{1}{R_1} - \frac{1}{R_2}\right) = \frac{1}{f}

For the magnification, two rays construct the image: one parallel to the axis bending through FF, and one through the optical centre going undeviated. Similar triangles (object and image heights with uu and vv) give

hh=vu\frac{h'}{h} = \frac{v}{u}

with the appropriate signs absorbed.

Two lenses in contact (focal lengths f1,f2f_1, f_2):

1F=1f1+1f2\frac{1}{F} = \frac{1}{f_1} + \frac{1}{f_2}

equivalently P=P1+P2P = P_1 + P_2.

Worked Example

Object 30 cm in front of converging lens of f=20f = 20 cm. Find image position and magnification.

u=30u = -30 cm, f=+20f = +20 cm.

1v=1f+1u=120+130=3260=160\frac{1}{v} = \frac{1}{f} + \frac{1}{u} = \frac{1}{20} + \frac{1}{-30} = \frac{3 - 2}{60} = \frac{1}{60}

v=+60v = +60 cm (real image, on the opposite side of the lens).

m=vu=6030=2m = \frac{v}{u} = \frac{60}{-30} = -2

Image is real, inverted, twice the object size.

Common Confusions

  • For mirrors m=v/um = -v/u, for lenses m=+v/um = +v/u. The signs come from the geometry of how rays go through versus reflect.
  • The lens formula here uses the convention 1/v1/u=1/f1/v - 1/u = 1/f (with signed quantities); some textbooks write the unsigned version 1/v+1/u=1/f1/v + 1/u = 1/f for a real object — both are equivalent if used consistently.
  • The optical centre is the point where a ray passes undeviated. For a thin symmetric lens it coincides with the geometric centre.

Key Takeaways

  • 1v1u=1f\frac{1}{v} - \frac{1}{u} = \frac{1}{f} for a thin lens.
  • Magnification m=v/um = v/u (signed).
  • Converging lens: f>0f > 0; diverging lens: f<0f < 0.
  • Lenses in contact add powers: P=P1+P2P = P_1 + P_2.

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