Telescope Resolving Power Calculator

Enter your telescope's aperture in millimeters.

How to use

  1. Enter your values in the fields above.
  2. Press Calculate to see your result instantly.
  3. Use the Share button to copy a link to your result.

About this calculator

A telescope's resolving power is the smallest angular separation at which it can still distinguish two close objects, such as a tight double star. The Rayleigh criterion (θ = 1.22·λ/D) gives the diffraction-limited theoretical minimum, while the empirical Dawes limit (116/D, with D in mm, giving arcseconds) is a slightly tighter rule of thumb derived from real observations of equal-brightness double stars.

Both scale inversely with aperture D — bigger apertures resolve finer detail. Amateur and professional astronomers use this calculator to compare telescopes and predict what detail — lunar craters, planetary cloud bands, close binary star pairs — a given aperture can actually reveal before buying or setting up equipment.

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