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F-number, light, and diffraction

A smaller F-number buys photons and spends depth of field.
12 September 2026 by

F-number is the lens opening as a ratio of focal length to entrance pupil. Smaller number, more light, shallower depth of field, more demand on the glass in the corners. It is not a quality grade. F/1.2 is not "better" than F/2.8. It is a different trade.

Workbench with small parts in shallow focus
A fast lens gathers light and throws away depth. That is useful on a workbench and fatal if you needed the back row of a rack.

In one sentence. F-number is how wide the pupil is. It buys photons and spends depth of field and edge sharpness.

What you gain when you open up

Each full stop doubles the light. F/1.4 to F/2.8 is two stops, a factor of four. That can be the difference between a usable warehouse aisle and a noisy guess. It also means a thinner slice of the world is in focus, and the edge of a wide M12 often falls apart.

What you gain when you stop down

More depth of field. Cleaner corners, up to a point. Then diffraction: the airy disk grows, and your expensive 1.4 µm pixel is smeared by physics, not by a cheap lens. Tiny pixels and tiny F-numbers do not automatically like each other, and neither do tiny pixels and very large F-numbers.

The reading-glasses test

In a dim restaurant you open your eyes wide and the menu is readable, but the candle behind it is a blur. In noon sun you squint and everything from the plate to the street is sharp, and you needed less "ISO." That is F-number, done with meat instead of glass.

How to read Camemaker

The lens library filters F-number as a range. Pick the slowest lens the scene can live with if you need depth (a dock, a shelf, a corridor). Pick a faster one if the light is poor and the subject sits in a known plane (a barcode at a fixed distance). Then check whether that fast glass still covers the format and still has MTF in the corner.

Colour filter arrays: RGB, mono, and the rest
Colour is a filter on a grey well. Mono is the well without the tax.