
The ability of an imaging system to distinguish closely spaced details.Resolution is the ability of an imaging system to distinguish between two closely spaced objects or details. In physics and engineering, it is a fundamental limit that determines how fine a structure can be observed, whether in a microscope, telescope, camera, or medical scanner. Higher resolution means finer details can be seen, which is crucial for fields ranging from astronomy to materials science.
The concept of resolution limits was formalized by Lord Rayleigh in the 19th century, who defined a criterion for when two point sources are just barely distinguishable. This Rayleigh criterion remains a standard reference.
Resolution is limited by the wavelength of the radiation used and the numerical aperture of the optical system. For conventional optics, the diffraction limit sets a minimum angular separation below which two points blur into one. Techniques like using shorter wavelengths (e.g., X-rays instead of visible light) or computational methods (e.g., super-resolution) can push beyond this limit. In digital imaging, resolution also depends on pixel size and sampling density.
Resolution is critical in X-ray microscopy, medical imaging (CT, MRI), satellite photography, and optical lithography for microchip manufacturing.
The Hubble Space Telescope, with a mirror of 2.4 meters, can resolve details as small as about 0.05 arcseconds — equivalent to reading a newspaper from about a kilometer away.



