MCQ
The resolving power of a telescope depends on:
- ALength of telescope
- BFocal length of objective
- ✓Diameter of the objective
- DFocal length of eyepiece
Resolving power of telescope $\text{R}=\frac{1}{\Delta\theta}=\frac{\text{a}}{1.22\lambda}$
where, $\Delta\theta$ is angular separation between two objects.
a is the diameter of the objective.
$\lambda$ is wavelength of light.
So, clearly resolving power of a telescope depends on diameter of the objective.
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($1$) The value of $R$ is. . . . meter.
($2$) The value of $b$ is. . . . . .meter.
| $(I)$ Presbiopia | $(A)$ Sphero-cylindrical lens |
| $(II)$ Hypermetropia | $(B)$ Convex lens of proper power may be used close to the eye |
| $(III)$ Astigmatism | $(C)$ Concave lens of suitable focal length |
| $(IV)$ Myopia | $(D)$ Bifocal lens of suitable focal length |