Rayleigh Limit

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Instrumentation And Observational Techniques, Astronomical Instrumentation

Scientific paper

The theoretical resolving power of a telescope according to a criterion devised by Lord Rayleigh (1842-1919). Because of the phenomenon of diffraction the image of a point source of light (such as a star) produced even by a perfect optical instrument consists of a central bright spot (the Airy disk) surrounded by concentric dark and light rings. If two point sources are very close together, the r...

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