Resolving power helps us understand how well an optical instrument, like a grating, microscope, telescope, or even the human eye, can distinguish between two close objects or details. A higher resolving power means the instrument can see finer details more clearly. In this article, we will study about resolving power and learn more about resolving the power of Telescope and Microscope. We will study the resolving power of Grating, limit of resolution and resolving power of human Eye. In the last we will see the difference between telescope and microscope .
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Resolving Power is the ability of an optical instrument (like a microscope or telescope) to clearly show two close objects as separate.
The resolving power of a microscope is its ability to distinguish two very close points on a small object as separate. It depends on the wavelength of light ( $\lambda$ ) and the numerical aperture (NA) of the microscope lens.
$
\text { Resolving Power of Microscope }=\frac{1}{d}=\frac{2 n \sin \theta}{\lambda}
$
Here,
The resolving power of a telescope is its ability to distinguish two distant stars (or objects) that appear very close together in the sky.
$
\text { Resolving Power of Telescope }=\frac{1}{\theta}=\frac{D}{1.22 \lambda}
$
Here,
A microscope is an optical instrument used to see tiny objects that cannot be seen clearly with the naked eye. It works by magnifying the image of small objects, such as cells, bacteria, or fine details of materials. A microscope uses one or more lenses to bend (refract) light and enlarge the image. The most common types are the simple microscope (one lens) and the compound microscope (two or more lenses).
Example: Used in laboratories to study microorganisms, tissues, and cells.
A telescope is an optical instrument used to see distant objects by collecting and focusing light or other forms of electromagnetic radiation. It helps us observe stars, planets, and galaxies that are far away from Earth. Telescopes can be refracting (use lenses) or reflecting (use mirrors).
Example: Used in astronomy to study celestial bodies like the Moon and planets.
The resolving power of a diffraction grating is its ability to separate two very close wavelengths of light. It depends on the number of lines ( N ) and the order of diffraction ( n ).
$
R=n N
$
A grating with more lines gives better separation of light, which means higher resolving power.
The limit of resolution is the smallest distance between two points or objects that can still be seen as separate. If the objects are closer than this limit, they appear as one. It depends on the wavelength of light and the aperture of the instrument.
The resolving power of the human eye is the ability to distinguish two close objects as separate. Under normal conditions, the minimum angle the eye can resolve is about 1 minute of $\operatorname{arc}\left(1 / 60^{\circ}\right)$. This is why we can see distant objects clearly but cannot separate very tiny details without instruments.
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NCERT Physics Notes:
Frequently Asked Questions (FAQs)
The resolving power of a telescope depends on the wavelength of light (
Resolving Power of Telescope =D/1.22 λ
It is defined as the reciprocal of the smallest angular separation between two distant objects that can just be distinguished by the telescope.
The resolving power of a microscope or telescope is its ability to show two close objects as separate. A higher resolving power means the instrument can show finer details clearly.
From a distant ,we can’t able to judge the separation between the source point but as the object comes closer ,we can barely resolve and tell the difference between the two images .Hence angular resolution depends upon the distance (L)
L: distance of image from Eye. It is always in radian
Microscope | Telescope |
This optical instrument is used to see very small objects like cells ,study of diseases | This optical instrument is used to see very large object like Celestial body ,study of solar system |
The aperture of the object is small | The aperture of the object is large |
In this , Eye piece is greater than focal length | In this optical instrument focal length is greater than Eyepiece. |
Wavelength of light and numerical aperture of the lens.
Because, the wavelength of visible light is greater than the wavelength of electrons.