Why do f-stops change by square roots instead of a linear scale?
Asked 5/31/2014
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I understand that each full stop changes exposure by a factor of two, but the f-number sequence goes 1.4, 2, 2.8, 4, 5.6, 8, etc. Why is aperture expressed this way instead of with a simple linear scale? For example, why not use numbers where f/6 would admit half as much light as f/3? Is the current system just historical, or is there a physical reason for the square-root progression?
Originally by Photography Stack Exchange contributor. Source · Licensed CC BY-SA 4.0
Photography Stack Exchange contributor
12y ago
2 Answers
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It's not linear because it's based on area rather than lines.
Or, to put it another way, the scale isn't based on square roots. It's based on the actual math that represents the physical properties of the system, and it happens that exposure doubles when aperture size opens by a factor of the square root of 2.
If you remember back to your elementary-school math, the area of a circle is πr². For a given aperture area A, how do we change r to get it to double? Well, we need to increase that r by a number which, when squared, is 2 — there's our √2.
We could certainly renumber those stops to give a linear scale, but since that would be an extra layer of abstraction from the physical system, that actually makes it more complicated rather than easier. This is more than theoretical, as the numbers are used in other places like flash guide numbers.
It's not really hard to understand and memorize the basic scale (since the practical range is only a handful of numbers anyway). In the 19th century, there were a number of competing systems using linear numbering, but by the beginning of the last century, the f-number system had won out.
Originally by user1943. Source · Licensed CC BY-SA 4.0
user1943
12y ago
0
Generated from our catalog & community — verify before relying on it.
F-stops aren’t arbitrary numbers; they come from lens geometry. The f-number is the ratio of focal length to the diameter of the entrance pupil. The amount of light admitted depends on the aperture’s area, and area of a circular opening scales with the square of its diameter.
So if you want each full stop to represent a doubling or halving of light, you must change the aperture diameter by the square root of 2, because area is proportional to diameter squared. That’s why the familiar sequence is f/1.4, f/2, f/2.8, f/4, f/5.6, f/8, etc.
A linear numbering system could be invented, but it would be less directly tied to the physical lens. The current system is useful because the same f-number represents the same light-gathering geometry regardless of focal length, making apertures comparable across lenses.
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