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Resolving Power of a Telescope

Last modified by
on
Nov 7, 2024, 4:11:56 PM
Created by
on
May 20, 2017, 6:29:17 PM
α=2.06×105(λD)
(λ)Wavelength
(D)Diameter
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The Resolving Power of a Telescope calculator computes the angular distance between two stars on the limit of visibility for a telescope.

INSTRUCTIONS: Choose units and enter the following:

Resolving Power (α): The calculator returns the Resolving Power in  arc seconds.  

The Math / Science

The resolving power of a telescope is the angular distance between two stars that are just barely visible through the telescope as separate images. The resolving power α in arc seconds of a telescope with diameter D in meters that is collecting light of wavelength λ in nanometers equals is given by this formula.  The formula for the resolving power of a telescope is:

     α=2.06x105(λD)

where:


Astronomy Calculators

Kepler's 3rd Law           T² = (4π • R³)/(G • M)

Flux and Magnitude

Small Angle Formula         α = S / D

Telescope formulas

Luminosity

Mass formulas

Other Formulas

Relative Size Formulas

Wavelength Formulas


This equation, Resolving Power of a Telescope, is used in 2 pages
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