*********************************************************************** How large should the hole for a pinhole camera be, and why? by Dick Koolish *********************************************************************** In terms of sharpness, the pinhole should be the same size as the diffraction disk it produces. A larger pinhole has a larger geometrical spot while a smaller pinhole has a larger diffraction spot. The linear diameter of the diffraction spot (Airy disk) produced by a pinhole of a given diameter is: spot = (2.44 * wavelength * focal_length) / diameter For example, a .5 mm pinhole at 100 mm focal length at 550 nm wavelength would produce a diffraction disk of: spot = (2.44 * .000550 * 100) / .5 = .268 mm So you see that the pinhole is too big in this case because .5 is larger than .268. The optimal size is where spot = diameter, so: diameter * diameter = (2.44 * wavelength * focal_length) diameter = sqrt (2.44 * wavelength * focal_length) At 100 mm focal distance and 550 nm wavelength, the optimal pinhole size is: diameter = sqrt (2.44 * .000550 * 100) = sqrt (.01342) = .366 mm Sharpness of an image can be improved by using a shorter focal length rather than a longer focal length for a given film size. This allows you to use a smaller pinhole. Also, if you use orthochromatic (blue sensitive) film, you can use a smaller pinhole by eliminating the longer wavelengths. If you have a choice, use the largest film size you can, rather than a smaller film size and enlarging. For a given sized final print, the optimal size pinhole increases slower than the enlarging factor. I have actually done some tests with various size pinholes at 100mm focal length and you can see how too large or too small pinholes degrade the image. By the way, the resolution of pinholes is nowhere near that of a real lens. At 100mm focal length, the optimum pinhole might resolve 5 lines/mm while a good lens will resolve 80-100 lines/mm. Table of pinhole sizes for 550 nm wavelength. Distance Diameter Diameter f number mm mm in 10 0.116 0.005 86.3 20 0.164 0.006 122.1 30 0.201 0.008 149.5 40 0.232 0.009 172.6 50 0.259 0.010 193.0 60 0.284 0.011 211.4 70 0.306 0.012 228.4 80 0.328 0.013 244.2 90 0.348 0.014 259.0 100 0.366 0.014 273.0 200 0.518 0.020 386.0 300 0.635 0.025 472.8 400 0.733 0.029 546.0 500 0.819 0.032 610.4 600 0.897 0.035 668.7 700 0.969 0.038 722.2 800 1.036 0.041 772.1 900 1.099 0.043 818.9 1000 1.158 0.046 863.2 2000 1.638 0.064 1220.8 3000 2.006 0.079 1495.1 4000 2.317 0.091 1726.4 5000 2.590 0.102 1930.2 6000 2.838 0.112 2114.5 7000 3.065 0.121 2283.9 8000 3.277 0.129 2441.6 9000 3.475 0.137 2589.7 10000 3.663 0.144 2729.8 Trial exposures can be determined from the "sunny 16 rule". For example, for ISO 100 speed film, the bright sunlight exposure is f/16 at 1/100 sec. If we use common shutter speeds, we get: f/16 1/125 seconds f/22 1/60 f/32 1/30 f/45 1/15 f/64 1/8 f/90 1/4 f/128 1/2 f/180 1 second f/256 2 f/360 4 f/512 8