Light travels in a straight line, and that is why shadows exist
We only see an object when light coming from it reaches our eye. Some objects, which we call primary sources, make their own light (the Sun, a light bulb, a candle), while secondary sources only reflect the light they receive (the Moon, this page, you).
Light passes through a transparent medium (air, clear glass) in an orderly way. A translucent medium (frosted glass, tracing paper) also lets it through, though scattered, and an opaque one (wood, a wall) does not let it pass at all.
In a uniform medium light travels in a straight line, so an opaque object in its way blocks the rays and a shadow appears behind it. With a point source the edge of the shadow is sharp. An extended source also produces a penumbra, a region that receives light from only part of the source. Eclipses are exactly this on an astronomical scale.
In a pinhole camera, each point of the object sends one ray through the tiny hole, and because the rays cross there the image comes out upside down, with a size we can find by similar triangles.
Let's discuss
- Click 'Point source' and check whether there is a penumbra, then slowly increase the size of the source and watch the edge of the shadow.
- Move the object closer to the source. Does the shadow get bigger or smaller, and what happens to the penumbra?
- Click 'Annular eclipse', where the source is bigger than the object, and look for the shadow. Where did it go?
- In the pinhole camera, move the candle farther away and see what happens to the size of the image, then check \(o/i = p/p^{\prime}\) with the numbers in the readouts.
- Why does the image in the pinhole camera come out upside down? Following a single ray from the top of the candle may help.