Sky science
Diffraction Limit
Direct answer
Diffraction Limit: The Diffraction Limit is the finest ideal angular detail possible for an aperture at a given wavelength.
It is the wave-optics floor for image resolution.
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At a glance
- Found in
- Astronomy & Skywatching
- Related
- Angular Resolution, Resolving Power, Rayleigh Criterion, Telescope Aperture
It is the wave-optics floor for image resolution.
A scientific orientation to scale, light, or motion; the article supplies the precise definition.
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The story behind Diffraction Limit
Wave optics replaced purely ray-based expectations of perfect imaging.
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Why Diffraction Limit matters
Diffraction Limit explains why larger apertures and shorter wavelengths can show finer detail.
Diffraction Limit in practice: an example
Doubling aperture halves the characteristic diffraction angle at one wavelength.
Where readings of Diffraction Limit go wrong
A diffraction-limited specification does not guarantee good contrast or sampling.
Sources and editorial method
Research references used for this entry include:
- European Southern Observatory: Technology for Telescopes - Observatory reference for aperture, angular resolution, atmospheric seeing, mirrors, and telescope technology.
- NASA Science: Universe Glossary - NASA definitions for common stellar, galactic, orbital, and high-energy astronomy terms.
- Source
- The Great Almanac Dictionary
- Category
- Astronomy & Skywatching
- Last updated
- 2026-09-26
See how aperture limits detail
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Common questions
What is the Diffraction Limit?
The Diffraction Limit is the finest ideal angular detail possible for an aperture at a given wavelength.
What do people get wrong about the Diffraction Limit?
A diffraction-limited specification does not guarantee good contrast or sampling.
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