Key ideas needed
- Light travels in straight lines, and an opaque object casts a shadow only where its dark region actually reaches a screen (here, the ground).
- The Sun is huge but very far away, so it acts as an extended source of light, not a point source.
- The shadow of any object in sunlight has two parts:
- Umbra – the region where light from no part of the Sun reaches; it is completely dark.
- Penumbra – the region where light from some (but not all) of the Sun reaches; it is only partially dark and looks very faint.
Step 1 – Picture the shadow of the bird
Draw rays from the two opposite edges of the Sun’s disc that just graze the bird’s body. Behind the bird these rays cross over to form a narrow cone. Inside the cone is the umbra (fully dark); outside it, but still partially blocked, is the penumbra.
(Sketch: Sun at the top, bird below it, two grazing rays tangent to the bird crossing behind it to form a narrow umbral cone that tapers to a point; ground at the bottom.)
Step 2 – How long is the bird’s umbra?
The Sun’s angular diameter in our sky is about $$0.53^\circ$$, so its angular radius is
\[
\alpha \;\approx\; 0.265^\circ \;=\; 0.0046\ \text{rad}.
\]
By simple geometry, the length $$L$$ of the umbral cone behind a small object of size $$d$$ is approximately
\[
L \;\approx\; \frac{d}{\alpha}.
\]
Taking a bird about $$d \approx 0.2\ \text{m}$$ across,
\[
L \;\approx\; \frac{0.2}{0.0046} \;\approx\; 43\ \text{m}.
\]
So the bird’s umbral cone is only a few tens of metres long – certainly nothing like the hundreds of metres at which a bird usually flies.
Step 3 – Why we do not see a shadow when the bird is high
- If the bird’s height $$h$$ is much greater than $$L$$ (about $$40$$–$$50\ \text{m}$$), the umbral cone tapers to a point in mid-air before it can reach the ground.
- Only the very faint penumbra reaches the ground, and it is spread over such a large area that it is far too dim for our eyes to notice.
Step 4 – Why we do see a shadow when the bird swoops low
- When the bird flies low enough that $$h < L$$, the umbra actually reaches the ground.
- A small, distinct dark patch (the umbra) now appears on the ground, surrounded by a thin lighter region (the penumbra), and we clearly see it as the bird’s shadow.
Conclusion
Because the Sun is an extended source, the bird’s umbra is only a few tens of metres long. When the bird is high in the sky, the umbra ends in the air, so only an extremely faint penumbra falls on the ground and no shadow is seen. When the bird swoops near the ground, the umbra finally touches the ground and a clear dark shadow becomes visible.