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.
Both give the finest angle in arcseconds a scope can separate, but Dawes is the empirical tighter split for equal stars while Rayleigh is the slightly larger theoretical diffraction limit.
Resolution improves as aperture grows; the Dawes limit is about 116 divided by aperture in millimeters, so a bigger scope splits closer double stars.
No; the theoretical limit is fixed by aperture and the light wavelength, though you still need enough magnification and steady seeing to actually see the 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.
Yes. Telescope Resolving Power Calculator is completely free, with no sign-up and no usage limits.
Yes. Telescope Resolving Power Calculator runs in any modern web browser. There is nothing to download or install.
Yes. Telescope Resolving Power Calculator runs entirely on your device in your browser, so nothing you enter is uploaded to a server.
Link this tool from a README, doc or site. The badge links back to this page.
[](https://yourhack.ai/telescope-resolving-power-calculator)