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Define the resolving power of microscopes. Write its formula. How will it vary, when
(a) wavelength of incident light is decreased.
(b) the aperture of the objective lens is decreased.

Answer
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Hint: Microscopes are used to see objects which are too small for naked eye. We use circular openings like lenses to magnify the object. Whenever we use a circular opening like a lens or iris of our eye. A circular diffraction pattern is formed. We need to differentiate between two such diffraction patterns which are very close to each other. The resolving power of a microscope gives us that limit.


Complete step by step solution:
Resolving power of microscopes is given by the inverse of the distance between two lines or points that can be resolved clearly using the microscope.

Let’s understand why we need this quantity. When we see an object through a circular opening it creates a diffraction pattern as shown in the following figure. The concentric rings are called Airy’s rings.

seo images



When two objects are very close to each other, we need to make sure that these rings do not overlap with each other and create a blurry image of the two objects. This gave rise to the Rayleigh criterion.
We can use this criterion to find the resolving power of microscopes. It is given by the inverse of the distance between two objects that can be resolved. Hence, we can write the Abbe’s criterion as,
Resolving power = 1Δd=2nsinθλ

Where,
1Δd is the resolving power of the microscope
n is the refractive index separating the object and aperture.
λis the wavelength of the light used for observation.

The termnsinθ is also called Numerical Aperture (N.A.) of the microscope. Hence, we can write,
Resolving power = 1Δd=2N.A.λ.................(1)

(a) From equation (1) we can say that the resolving power of the microscope will increase if the wavelength of incident light is decreased.

(b) From equation (1) we can again say that the resolving power of the microscope will decrease if we decrease the aperture of the objective lens.


Note: Rayleigh’s criterion is given by,
θ=1.22λd

Where,
θ is the half angle subtended by the first minimum at the source
λ is the wavelength of light that is being used for measurement
d is the distance between the two objects

This is an important criterion to observe two fully resolved objects using telescopes or microscopes.
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