Resolving Power


Ask a Question, Get an Answer!
Hundreds of tutors are online and ready to help you right now!
The ability of the instrument to resolve the images of two point objects lying close to each other. Due to the wave nature of light each point object produces its own diffraction pattern, which overlap, and the image can no longer be identified.

Resolving power of a microscope is the reciprocal of the minimum distance (d) between two point objects, which can just be seen through the microscope as separate.

resolving power of a microscope

To increase the resolving power, m, q should be large and l should be decreased where

l = the wavelength of the light used to illuminate the object.

q = half angle of the cone of light from the point object kept under objective lens.

m = refractive index of the medium between the object and objective lens.

Resolving power of a telescope is the reciprocal of the small angular separation dq between two distant objects whose images are just seen in the telescope as separate.

where l is the wavelength of light, d is aperture of the objective

Resolving power of a telescope

To obtain a higher value of resolving power d the aperture should have a larger value and l small value.


Ask a Question? Get an Answer!

connect to a tutor


Related Searches

resolving power

;,  

objective power

,  

wave power

,  

power of a lens

,  

diffraction pattern aperture

,  

wavelength of light

,  

diffraction of light

,  
objective lens
,  
diffraction pattern
,  
objective lenses
,  
double value
,  
diffraction pattern wavelength
,  
telescope animation
,  
objective friction
,  
microscope objective
...more