Q.What is the shape of the wavefront in each of the following cases:
The shape of a wavefront is determined by the geometry of the source and the optical path. For a point source, it is spherical; for light emerging from a convex lens with the source at its focus, it is planar; and for light from a distant star intercepted by Earth, it is effectively planar.
The key idea here is frequency invariance — the frequency of light does not change when it travels through different media or optical systems, but the wavefront shape changes based on how the light propagates. A wavefront is a surface of constant phase; its shape tells you how the light is spreading or converging.
Let’s break it down case by case.
1. Light diverging from a point source
A point source emits light equally in all directions. Imagine a tiny bulb at the centre of a dark room — the light spreads out as concentric spheres. At any given instant, all points on a sphere centred at the source have travelled the same distance from the source, so they are at the same phase. That surface of constant phase is a sphere.
Think of a pebble dropped in still water — the ripples are circles (2D). In 3D, a point source gives spherical wavefronts. The radius of each sphere increases with time.
So the wavefront is spherical, with the source at the centre.
2. Light emerging from a convex lens when a point source is placed at its focus
Place a point source exactly at the focus of a convex lens. Light rays from the source strike the lens and are refracted. Because the source is at the focus, the lens bends the rays so they emerge parallel to the principal axis. Parallel rays mean the wavefront is a plane — all points on a plane perpendicular to the rays have the same phase.
Why? The lens introduces a path difference that exactly cancels the spherical curvature of the incoming wave. The emerging wavefront is flat.
A common mistake is to think the wavefront remains spherical after the lens. But the lens is designed to convert a spherical wave from the focus into a plane wave. If the source is exactly at the focus, the output is collimated — planar wavefront.
So the wavefront is planar (a plane wave).
3. The portion of the wavefront of light from a distant star intercepted by the Earth
A star is so far away that the light reaching Earth has travelled an enormous distance — effectively infinite compared to Earth’s size. The spherical wavefront from the star has a radius of many light-years. Over the small patch intercepted by Earth (a few thousand kilometres across), the curvature is negligible. A tiny arc of a huge sphere looks flat.
For a sphere of radius , the sagitta (deviation from flatness) over a chord of length is approximately . For m (a light-year) and m (Earth’s diameter), the sagitta is about m — a centimetre over thousands of kilometres. That’s effectively flat.
So the intercepted wavefront is planar (a plane wave).
- Spherical wavefront,
- Planar wavefront,
- Planar wavefront.
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