Table of contentsWhat does angular resolution measure?Angular resolution formulaWhat is the angular resolution of the human eye?
This angular resolution calculator will assist you in determining the angular resolution of a lens – the ability of an instrument to distinguish small details of an object. Keep reading if you wish to learn the answers to questions such as:
- What does the angular resolution measure?
- What is resolution in microscopy?
Read on to find answers to these questions and learn about the angular resolution formula.
What does angular resolution measure?
Angular resolution is the capacity of an optical instrument to separate two objects that are located at a small angular distance. In other words, with this physical quantity, you can check if you can:
- Resolve two small points that are very close to each other; or
- Distinguish between very distant objects that seem close to each other.
The smaller the angular resolution is, the more details you can see. It is essential when designing microscopes, telescopes, or cameras. Even the human eye has its angular resolution!
If you are interested in learning about telescope magnification, check our telescope magnification calculator.
Angular resolution formula
Angular resolution is sometimes called the Rayleigh criterion. The famous physicist, Lord Rayleigh, has proposed an empirical angular resolution formula:
θ = 1.22 × λ / d
θ– Angular resolution (expressed in radians);
λ– Wavelength of the light; and
d– Diameter of the lens aperture.
The above formula was derived for diffraction grating, but it can also be used for other purposes. Lord Rayleigh stated that two light sources are regarded as resolved when the principal diffraction maximum of one image coincides with the first minimum of the other.
If you are interested in learning more about diffraction grating, see our diffraction grating calculator.
What is the angular resolution of the human eye?
The diameter of an eye pupil (our natural lens) changes during the day and night, but it is approximately
2 mm on sunny days and
8 mm at night. Let's assume that we will try to resolve points that are green; the wavelength of green light is equal to
λ ≈ 550 nm. With the Angular resolution calculator, we compute that the angular resolution during the day is
θ ≈ 0.02°.
We can compare this result with the Hubble space telescope, which has a mirror of diameter
2.4 m (it collects light just like the eye pupil). The estimated angular resolution equals
θ ≈ 0.000016° – it is 125 times better than our eye!
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