One Curved Interface, One Master Formula

Let light cross a single spherical surface of radius R from a medium of index n1n_1 into n2n_2 (object O on the axis, image I). For paraxial rays, the small-angle geometry plus Snell's law (n1i=n2rn_1 i = n_2 r for small angles) gives, after applying the Cartesian convention (OM =u= -u, MI =+v= +v, MC =+R= +R):

n2vn1u=n2n1R\boxed{\frac{n_2}{v} - \frac{n_1}{u} = \frac{n_2 - n_1}{R}}

Reading the formula:

  • It connects object and image across one refracting surface — the atomic unit from which the lens formulas are assembled (Section 6 applies it twice).
  • R carries a sign: convex towards the incident light (centre beyond the surface) means R>0R > 0.
  • Set RR \to \infty (flat interface) and it reduces to n2v=n1u\frac{n_2}{v} = \frac{n_1}{u} — the apparent-depth result in disguise.

Refraction at a single spherical surface with object and image positions

The Template Problem

Light from a point source in air falls on a glass surface (n = 1.5, R = 20 cm) from 100 cm away. Where is the image?

Setup: n1=1n_1 = 1, n2=1.5n_2 = 1.5, u=100u = -100 cm, R=+20R = +20 cm.

1.5v=1.5120+1100=0.0250.010=0.015    v=+100 cm\frac{1.5}{v} = \frac{1.5 - 1}{20} + \frac{1}{-100} = 0.025 - 0.010 = 0.015 \;\Rightarrow\; v = +100\text{ cm}

The image forms 100 cm inside the glass, in the direction of the incident light.

Problem-solving drill:

  1. Identify n1n_1 (where light starts) and n2n_2 (where it goes) — the formula is direction-sensitive!
  2. Sign u (almost always negative), sign R by where C lies.
  3. Solve for v; positive v = image downstream (real, inside medium 2 here).

[JEE Tip] Curved-interface problems love two disguises: a fish under a curved bowl wall, and an air bubble inside a glass sphere (light then travels glass-to-air: n1=1.5n_1 = 1.5, n2=1n_2 = 1 — swap roles!). Direction of travel decides which index is which.

Solved Examples

Example 1: The NCERT template (Example 9.5)

A point source in air sits 100 cm from a convex glass surface (n = 1.5, R = 20 cm). Locate the image.

Solution:

  1. 1.5v1100=0.520\frac{1.5}{v} - \frac{1}{-100} = \frac{0.5}{20}.
  2. 1.5v=0.0250.01=0.015\frac{1.5}{v} = 0.025 - 0.01 = 0.015.
  3. v=+100v = +100 cm — a real image 100 cm beyond the surface, inside the glass.

Example 2: Same surface, nearer object [JEE Numerical]

Move the source to 25 cm from the same surface. Now where is the image?

Solution:

  1. 1.5v=0.520+125=0.0250.04=0.015\frac{1.5}{v} = \frac{0.5}{20} + \frac{1}{-25} = 0.025 - 0.04 = -0.015.
  2. v=100v = -100 cm.
  3. Negative v: a virtual image 100 cm on the incident side — close objects beat the surface's converging power.

Example 3: Flat-interface limit [NEET Numerical]

Use the master formula with RR \to \infty for a fish 90 cm under water (n = 4/3), viewed from straight above. Where does it appear?

Solution:

  1. n2v=n1u\frac{n_2}{v} = \frac{n_1}{u} with n1=4/3n_1 = 4/3 (water, where light starts), n2=1n_2 = 1, u=90u = -90.
  2. 1v=4/39011v=67.5\frac{1}{v} = \frac{4/3}{-90}\cdot\frac{1}{1} \Rightarrow v = -67.5 cm.
  3. The fish appears 67.5 cm deep =90/(4/3)= 90/(4/3) — the apparent-depth rule, straight from the master formula.

Example 4: Glass-to-air crossing [JEE Numerical]

An object inside glass (n = 1.5) sits 30 cm from a surface separating glass from air; the surface is concave as seen from inside the glass, with signed radius R = -10 cm. Find the image. (Light goes glass to air: n1=1.5n_1 = 1.5, n2=1n_2 = 1.)

Solution:

  1. 1v1.530=11.510=0.05\frac{1}{v} - \frac{1.5}{-30} = \frac{1 - 1.5}{-10} = 0.05.
  2. 1v=0.050.05=0\frac{1}{v} = 0.05 - 0.05 = 0.
  3. vv \to \infty: the rays emerge parallel — this object happens to sit at the surface's first focus.

Example 5: Sign the radius [NEET pattern]

State the sign of R when light strikes (a) a surface bulging towards it (convex), (b) a surface curving away (concave).

Solution:

  1. R runs from the surface's pole to its centre of curvature C, signed along the incident light.
  2. (a) Convex towards the light: C lies downstream — R>0R > 0.
  3. (b) Concave towards the light: C lies upstream — R<0R < 0.

Example 6: The formula's direction-sensitivity

Why must n1n_1 always be the medium the light comes FROM?

Solution:

  1. The derivation applies Snell's law at the crossingn1sini=n2sinrn_1\sin i = n_2\sin r with i in the first medium.
  2. Swapping the labels flips the sign of (n2n1)(n_2 - n_1) and misplaces the image.
  3. In bubble-in-glass problems light starts in glass: n1=1.5n_1 = 1.5, n2=1n_2 = 1. Read the ray, then label.

Example 7: Landing on the second focus [JEE Numerical]

For the air-glass surface (n = 1.5, R = +20 cm), find the object distance for which the image forms at v=+60v = +60 cm.

Solution:

  1. 1.5601u=0.520=0.025\frac{1.5}{60} - \frac{1}{u} = \frac{0.5}{20} = 0.025.
  2. But 1.560=0.025\frac{1.5}{60} = 0.025 exactly, so 1u=0\frac{1}{u} = 0, i.e. uu \to \infty.
  3. A parallel beam (object at infinity) focuses at 60 cm — incidentally the surface's second focal distance: f2=n2Rn2n1=1.5×200.5=60f_2 = \frac{n_2 R}{n_2 - n_1} = \frac{1.5 \times 20}{0.5} = 60 cm.

Example 8: First and second foci of one surface [JEE Numerical]

For the same surface, find the first focal distance (object position giving parallel emergent rays).

Solution:

  1. Set vv \to \infty: n1u=n2n1R-\frac{n_1}{u} = \frac{n_2 - n_1}{R}.
  2. u=n1Rn2n1=1×200.5=40u = -\frac{n_1 R}{n_2 - n_1} = -\frac{1 \times 20}{0.5} = -40 cm.
  3. Note f1f2|f_1| \ne |f_2| (40 vs 60 cm) — single surfaces have unequal foci, in the ratio n1:n2n_1 : n_2.

Example 9: A drop as a surface [NEET Numerical]

A tiny insect sits at the centre of curvature of a hemispherical dew drop (n = 4/3, R = 3 mm) and is viewed from above through the curved surface. Where does it appear?

Solution:

  1. An object at the centre of curvature sends every ray along a radius — each meets the surface normally and passes undeviated.
  2. The formula agrees: with the signed radius R-R (C lies on the incident side) and u=Ru = -R: n2v=n2n1R+n1R=n2R\frac{n_2}{v} = \frac{n_2-n_1}{-R} + \frac{n_1}{-R} = \frac{n_2}{-R}, so v=Rv = -R.
  3. The insect appears exactly where it is — rays through C never bend. A favourite shortcut.

Example 10: Building towards the lens

How does this section's formula become a lens formula?

Solution:

  1. A thin lens is two spherical surfaces back-to-back.
  2. Apply n2vn1u=n2n1R\frac{n_2}{v} - \frac{n_1}{u} = \frac{n_2-n_1}{R} at the first surface; its image becomes the object for the second application.
  3. Add the two equations, let the thickness vanish — out drops the lens maker's formula (Section 6). One brick, used twice.