Skip to content

Physics · Ch 9 — Ray Optics and Optical Instruments

Refraction at a Spherical Surface

9.5.1

Refraction at a Spherical Surface

Refraction at a Spherical Surface

When light travels from one transparent medium to another across a curved spherical surface, the path of the rays bends. The geometry of this bending is governed by Snell’s law and the curvature of the surface. For a small aperture (the surface’s lateral size is small compared to other distances), we can use small-angle approximations.

Consider a spherical surface with centre of curvature CC and radius of curvature RR. An object OO lies on the principal axis. Rays from OO are incident from a medium of refractive index n1n_1 into another medium of refractive index n2n_2. The image II is formed on the principal axis.

Derivation of the Formula
  1. Small-angle approximations: For small angles, the perpendicular from point NN on the surface to the principal axis is approximately equal to MNMN. The tangents of the relevant angles are:

    • tan⁡∠NOM=MNOM\tan \angle NOM = \frac{MN}{OM}
    • tan⁡∠NCM=MNMC\tan \angle NCM = \frac{MN}{MC}
    • tan⁡∠NIM=MNMI\tan \angle NIM = \frac{MN}{MI}
  2. Angle of incidence (ii): In triangle NOCNOC, the exterior angle ii equals the sum of the two opposite interior angles:

i=∠NOM+∠NCM=MNOM+MNMCi = \angle NOM + \angle NCM = \frac{MN}{OM} + \frac{MN}{MC}

  1. Angle of refraction (rr): In triangle NICNIC, the angle rr is the difference between two angles:

r=∠NCM−∠NIM=MNMC−MNMIr = \angle NCM - \angle NIM = \frac{MN}{MC} - \frac{MN}{MI}

  1. Applying Snell’s law: For small angles, sin⁡i≈i\sin i \approx i and sin⁡r≈r\sin r \approx r. Snell’s law n1sin⁡i=n2sin⁡rn_1 \sin i = n_2 \sin r becomes:

n1i=n2rn_1 i = n_2 r

  1. Substituting ii and rr: Substitute the expressions for ii and rr into the simplified Snell’s law:

n1(MNOM+MNMC)=n2(MNMC−MNMI)n_1 \left( \frac{MN}{OM} + \frac{MN}{MC} \right) = n_2 \left( \frac{MN}{MC} - \frac{MN}{MI} \right)

Cancelling $MN$ (which is non-zero) gives:

n1OM+n1MC=n2MC−n2MI\frac{n_1}{OM} + \frac{n_1}{MC} = \frac{n_2}{MC} - \frac{n_2}{MI}

Rearranging:

n1OM+n2MI=n2−n1MC\frac{n_1}{OM} + \frac{n_2}{MI} = \frac{n_2 - n_1}{MC}

  1. Applying the Cartesian sign convention: The distances OMOM, MIMI, and MCMC are magnitudes. Using the sign convention:
    • Object distance: OM=−uOM = -u (object is to the left of the surface) …
Figure 9.15Refraction at a spherical surface separating two media.
Fig. 9.15 — Refraction at a spherical surface separating two media.

Drawn by us to help you understand the concept clearly, and verified to make sure it's accurate. For exams, practice from your textbook's own diagram.

What the Figure Shows

The figure depicts a convex spherical refracting surface — a single curved arc — that separates two transparent media. The medium to the left has refractive index n1n_1 (optically rarer), and the medium to the right has refractive index n2n_2 (optically denser, n2>n1n_2 > n_1). The principal axis is a horizontal straight line passing through the centre of curvature CC and the pole MM of the spherical surface. The radius of curvature RR is the distance MCMC along the axis.

A point object OO is placed on the principal axis in medium 11. One ray from OO travels along the axis (the axial ray) and strikes the surface normally at MM, continuing undeviated. Another ray from OO strikes the surface at point NN (not at the pole). At NN, the ray refracts and bends toward the normal (since n2>n1n_2 > n_1), and after refraction it meets the axial ray at point II on the principal axis in medium 22. Thus II is the real image of OO formed by the spherical surface.

Key Geometrical Elements and Labels

  • OO: object point on the principal axis in medium n1n_1.
  • II: image point on the principal axis in medium n2n_2.
  • CC: centre of curvature of the spherical surface, on the principal axis.
  • MM: pole of the spherical surface (the point where the principal axis meets the surface).
  • NN: point of incidence of the non-axial ray on the spherical surface.
  • RR: radius of curvature, R=MCR = MC.
  • n1n_1, n2n_2: refractive indices of the two media.
  • Angles marked: ∠NOM\angle NOM, ∠NCM\angle NCM, ∠NIM\angle NIM — these are the angles that the incident ray, the radius, and the refracted ray make with the principal axis, respectively. The angle of incidence ii is the exterior angle of triangle NOCNOC, and the angle of refraction rr is the difference ∠NCM−∠NIM\angle NCM - \angle NIM.

Physical Idea Taught

The figure illustrates how a single spherical surface can form an image by refraction. The derivation uses the small-angle approximation (aperture of the surface is small compared to distances OMOM, MIMI, MCMC), so that the perpendicular NMNM is nearly equal to the arc length, and tan⁡θ≈θ\tan \theta \approx \theta. By applying Snell's law (n1sin⁡i=n2sin⁡rn_1 \sin i = n_2 \sin r) in the small-angle limit (n1i=n2rn_1 i = n_2 r), and expressing ii and rr in terms of the distances OMOM, MIMI, MCMC, the textbook arrives at the fundamental relation for refraction at a spherical surface.

Key Formula Derived

The final result, after applying the Cartesian sign convention, is:

n2v−n1u=n2−n1R\frac{n_2}{v} - \frac{n_1}{u} = \frac{n_2 - n_1}{R}

where: …