If aperture diameter of the lens of a telescope is 1.25 m and wavelength of light used is 5000 Å, its resolving power is
A
`2.05xx10^(6)`
B
`2.5xx10^(5)`
C
`4.1xx10^(5)`
D
`4.1xx10^(6)`
Text Solution
AI Generated Solution
The correct Answer is:
To find the resolving power of the telescope, we can use the formula for the resolving power (RP) of a telescope, which is given by:
\[
RP = \frac{d}{1.22 \lambda}
\]
where:
- \( d \) is the diameter of the telescope's aperture,
- \( \lambda \) is the wavelength of light used.
### Step 1: Identify the given values
- Diameter of the lens \( d = 1.25 \, \text{m} \)
- Wavelength of light \( \lambda = 5000 \, \text{Å} \)
### Step 2: Convert the wavelength from angstroms to meters
1 angstrom (Å) = \( 10^{-10} \) meters, so:
\[
\lambda = 5000 \, \text{Å} = 5000 \times 10^{-10} \, \text{m} = 5 \times 10^{-7} \, \text{m}
\]
### Step 3: Substitute the values into the formula
Now substitute \( d \) and \( \lambda \) into the resolving power formula:
\[
RP = \frac{1.25 \, \text{m}}{1.22 \times 5 \times 10^{-7} \, \text{m}}
\]
### Step 4: Calculate the denominator
First, calculate \( 1.22 \times 5 \):
\[
1.22 \times 5 = 6.1
\]
Now, multiply by \( 10^{-7} \):
\[
6.1 \times 10^{-7} \, \text{m}
\]
### Step 5: Calculate the resolving power
Now substitute back into the equation:
\[
RP = \frac{1.25}{6.1 \times 10^{-7}} \approx 2.049 \times 10^{6}
\]
### Step 6: Round the result
Rounding \( 2.049 \times 10^{6} \) gives:
\[
RP \approx 2.05 \times 10^{6}
\]
### Conclusion
The resolving power of the telescope is approximately \( 2.05 \times 10^{6} \) (unitless).
Topper's Solved these Questions
JEE MAINS
JEE MAINS PREVIOUS YEAR ENGLISH|Exercise Chemistry|1 Videos
JEE MAIN
JEE MAINS PREVIOUS YEAR ENGLISH|Exercise All Questions|452 Videos
JEE MAINS 2020
JEE MAINS PREVIOUS YEAR ENGLISH|Exercise PHYSICS|250 Videos
Similar Questions
Explore conceptually related problems
The diameter of the lens of a telescope is 0.61 m and the wavelength of light used is 5000 Å. The resolution power of the telescope is
The diameter of the objective of the telescope is 0.1 metre and wavelength of light is 6000 Å . Its resolving power would be approximately
The diameter of the objective lens of a telescope is 5.0m and wavelength of light is 6000 Å . The limit of resolution of this telescope will be
The wavelength of light is 5000 Å , express it in m .
The wavelength of light is 5000 Å , express it in nm .
Two stars distant two light years are just resolved by a telescope. The diameter of the telescope lens is 0.25 m . If the wavelength of light used is 5000 A^(0) , then the minimum distance between the stars is
The numerical aperture of an objective of a microscope is 0.5 and the wavelength of light used is 5000 A^(0) . Its limit of resolution will be
In Young's double slit experiment, the distnace between two sources is 0.1//pimm . The distance of the screen from the source is 25 cm. Wavelength of light used is 5000Å Then what is the angular position of the first dark fringe.?
A : The resolving power of both miroscope and telescope depends on the wavelength of the light used. R : The resolving power of a lens is the ability to resolve the two images so that they are distinctly identified.
Fraunhoffer diffraction pattern of a single slit is obtained in the focal plane of lens of focal length 1m . If third minimum is formed at a distance of 5mm from the central maximum and wavelength of light used is 5000Å , then width of the slit will be –
JEE MAINS PREVIOUS YEAR ENGLISH-JEE MAINS-Chemistry