Partial Mirror Obstruction — Why the Formula Holds
Let's build this from first principles. The core idea is: what happens when a mirror is partially blocked, and how does that affect the image?
1. The Fundamental Principle
A plane mirror forms an image because each point on the object sends rays in all directions. The mirror reflects these rays according to the law of reflection:
Angle of incidence = Angle of reflection
The image appears where the extensions of the reflected rays meet behind the mirror.
2. What "Partial Obstruction" Actually Means
When part of a mirror is covered (say, by a cloth or tape), only the uncovered portion can reflect light. The key question: Does the image shrink, disappear partially, or remain full but dimmer?
The surprising result (derived below):
The full image remains visible, but its brightness decreases proportionally to the uncovered area.
3. Derivation — Step by Step
Step 1: Consider a single point on the object
Take a point P on the object. Light from P spreads out in all directions. Some rays hit the mirror, some miss it entirely.
Step 2: Which rays matter?
Only the rays that:
- Strike the uncovered part of the mirror
- Then reflect into the observer's eye
Step 3: The cone of rays
From point P, the set of rays that can reach the observer after reflection forms a cone. The mirror's uncovered area acts like an aperture — it lets through only those rays that hit it.
Step 4: The image location is unchanged
The image of P is located behind the mirror at the same perpendicular distance as P is in front. This location depends only on geometry, not on which part of the mirror is used.
Why? Because the law of reflection is local — any small patch of mirror still reflects rays from P to the same virtual image point P′.
Step 5: Brightness reduction
The number of rays reaching the eye from P is proportional to the area of the mirror that is uncovered. If:
- Atotal = total mirror area
- Auncovered = area not blocked
Then the intensity (brightness) of the image scales as:
I∝AtotalAuncovered
4. The Key Formula(e)
For a single point object:
Image brightness∝Total mirror areaUncovered mirror area
For an extended object:
The entire image remains visible (same size, same location), but dimmer:
Relative brightness=AtotalAuncovered …