In this chapter, 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 and study further in details about resolution limit, types of microscope and unit of numerical aperture.
JEE Main 2025: Physics Formula | Study Materials | High Scoring Topics | Preparation Guide
JEE Main 2025: Syllabus | Sample Papers | Mock Tests | PYQs | Study Plan 100 Days
NEET 2025: Syllabus | High Scoring Topics | PYQs
The Rayleigh criterion for the minimum resolvable angle is
θmin = 1.22 λ/D
Where, D is the diameter of the aperture of the instrument
Also read -
Resolving Power of Grating
It is the capacity of an aperture to separate two different diffraction maxima formed by two different wavelengths which are very close to each other.
Resolving Power and its SI unit
Resolving Power of optical instruments is defined as the capacity of its to distinguish between smaller details .
For the objects to be distinguished kept at a smaller distance , resolving power should be higher.
SI unit of Resolving Power
Resolving power is dimensionless quantity and thus it has no SI unit
Note: Resolving Power is the ratio between mean wavelength of different spectral lines and difference of wavelength between them and as there is the same quantity having the same unit thus there is no SI unit.
Related Topics Link, |
Types of Microscope
Resolution of Electron Microscope
As we know Resolution depends upon wavelength and wavelength of electrons is much smaller than other particles so theoretically resolution of electron microscope comes to be unlimited.
Resolution of Compound Microscope
Restraints of resolution of simple Microscope can be removed by using Compound Microscope as it has two lens arrays namely objective lens and Eyepiece. The combination of these lens arrays results in formation of an enlarged virtual image.
Numerical Aperture Derivation
NA= √( Ƞ1^2- Ƞ2^2)
Where, Ƞ1 is refractive index of core
Ƞ2 is refractive index of cladding.
Also Read:
Types of telescope
On the basis of wavelength Telescope is distinguished as:
Optical Telescope
X-Ray Telescope
Ultraviolet Telescope
Telescope Resolution
It is an ability of a telescope to distinguish two point source objects into different images.
Principles of Telescope
We try to understand this by an example:
Let's say on a hazy night we were driving through the forest and were experiencing a lot of obstacles to see through the foggy light . We saw a beam of light coming towards us and we were unable to study the origin of point source or unable to distinguish the point source but as the object came closer by, we found it was a four wheeler instead of motorbike as we could easily see different point sources of light.
Same principle is followed by Telescope
Telescope Power
In simple term , Telescope power is its ability to enlarge its object size
Resolving power of Telescope formula is given by:
Resolving Power =D/d= a / 1.22 λ
Where D= distance of object from the lens of telescope
a= Resolution of two slit
How can we change Resolving Power
As we can see Resolving Power of a telescope depends on the resolution of two slits, so by increasing the value of (a) we can increase the power value.
Resolving Power of an Eye
Like telescopes or other optical instruments our Eyes also have resolving power. It depends on size of pupils ,as compared to diameter of aperture of other optical instruments our pupils size is comparatively very small hence it is obvious that resolving power of our Eyes is lower than all other optical instruments.
Also check-
NCERT Physics Notes:
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.
30 Nov'24 01:19 PM
29 Nov'24 05:26 PM
29 Nov'24 02:40 PM
29 Nov'24 01:21 PM
28 Nov'24 04:42 PM
28 Nov'24 01:26 PM
28 Nov'24 01:21 PM
26 Nov'24 03:50 PM
22 Nov'24 01:31 PM
17 Nov'24 09:51 AM