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Telescope Resolving Power Calculator

0.77Dawes limit (arcsec)
0.92"Rayleigh limit
5.9"Aperture (inches)
225xPower to split

Resolving power is the smallest angle a telescope can separate, which decides whether a tight double star shows as two points or one blurred blob. It depends almost entirely on aperture: bigger mirrors and lenses resolve finer detail. This calculator gives two classic figures in arcseconds. The Dawes limit, 116 divided by the aperture in millimeters, is an empirical rule for splitting equal magnitude double stars. The Rayleigh limit, 138 divided by the aperture in millimeters, is the stricter physical diffraction criterion. Enter your aperture to see both, along with the useful magnification you need to actually perceive that separation. All math runs locally in your browser with nothing uploaded.

Frequently asked questions

What is Telescope Resolving Power Calculator?

Resolving power is the smallest angle a telescope can separate, which decides whether a tight double star shows as two points or one blurred blob. It depends almost entirely on aperture: bigger mirrors and lenses resolve finer detail.

Is Telescope Resolving Power Calculator free to use?

Yes. Telescope Resolving Power Calculator is completely free, with no sign-up and no usage limits.

Does Telescope Resolving Power Calculator work in a web browser?

Yes. Telescope Resolving Power Calculator runs in any modern web browser. There is nothing to download or install.

Is my data private with Telescope Resolving Power Calculator?

Yes. Telescope Resolving Power Calculator runs entirely on your device in your browser, so nothing you enter is uploaded to a server.