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The minimum angular separation of two points which can just be resolved by an optical instrument is given by min = 1.22 /D, where D is the diameter of the aperture of the instrument.
= wavelength. U = angle of the cone of light coming from object. U' = angle of cone of light forming image. N = refraction index of object. M = magnification. NA = numerical aperture. D = distance between two points in the image. D = 0.61 / (m tank') (1)* **
The diffraction limit of the eye can be calculated using Rayleigh's criterion: angular resolution = (1.22)(lambda)/D, where lambda is the wavelength of light (on the average, about 550 nm) and D is the diameter of the eye's pupil, which is about 5 mm indoors.
Resolving power is defined as the ability of a microscope or telescope to distinguish two close together images as being separate. An example of resolving power is how well a telescope can show two stars as being separate stars.
2:23 5:30 Suggested clip Physics — Optics: Diffraction Grating (6 of 7) Resolving Power=? Of YouTubeStart of suggested client of suggested clip Physics — Optics: Diffraction Grating (6 of 7) Resolving Power=? Of
Resolving Power. The resolving power of an objective lens is measured by its ability to differentiate two lines or points in an object. The greater the resolving power, the smaller the minimum distance between two lines or points that can still be distinguished.
Resolving power is defined as the ability of a microscope or telescope to distinguish two close together images as being separate. An example of resolving power is how well a telescope can show two stars as being separate stars.
For telescope: Resolving power = D/1.22, here D is diameter of aperture, and lambda is the wavelength of light used. For microscope: Resolving power = 2usin@ / 1.22, here u = refractive index, @ = angle subtended by object on objective, lambda is wavelength.
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