Dawes' limit
Dawes' limit is a formula to express the maximum resolving power of a microscope or telescope.[1] It is so named after its discoverer, William Rutter Dawes ,[2] although it is also credited to Lord Rayleigh.
diffraction pattern matching Dawes' limit
The formula takes different forms depending on the units.
| R = 4.56/D | D in inches, R in arcseconds |
| R = 11.6/D | D in centimeters, R in arcseconds |
| where | D is the diameter of the main lens (aperture) |
| R is the resolving power of the instrument |
This formula agrees with the usual at a wavelength of about 460nm, somewhat bluer than the peak sensitivity of rod cells at c. 498nm.
See also
References
-
Bob King (2017-03-01). "Pushing Limits: A Spring Sky Double Star Romp". Sky and Telescope magazine. Retrieved 2020-02-12.
The most stringent test of telescopic resolution uses the criteria of Dawes' limit given by the equation R = 4.56/D, where R is the resolution in arcseconds and D is the telescope's aperture in inches.
- Dawes, W.R., Catalogue of Micrometrical Measurements of Double Stars. In: Memoirs of the Royal Astronomical Society, Vol. 35, p.137 1867, Bibcode:1867MmRAS..35..137D
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