Web Reference: Resolution is another vital telescope function. Simply put, telescope resolution limit determines how small a detail can be resolved in the image it forms. In the absence of aberrations, what determines limit to resolution is the effect of diffraction. Dec 20, 2019 · Resolving power (or resolution) of an optical telescope is the ability to see small details in the image. It is an angular distance between two stars that are barely visible as two separate images – it is usually expressed in units of arc-seconds. El Límite de Dawes es una fórmula para expresar la máxima resolución óptica de un microscopio o de un telescopio. Lleva el nombre de su descubridor, el astrónomo británico W. R. Dawes (1799-1868), a pesar de que también es acreditado en ocasiones John Rayleigh como su descubridor.
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