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Question: An astronomical telescope has objective and eyepiece focal lengths \(40cm\) and \(4cm\) respectively...

An astronomical telescope has objective and eyepiece focal lengths 40cm40cm and 4cm4cm respectively. To view an object 200cm200cm away from the objective, the lenses must be separated by a distance:
A) 54.0cmA)\text{ }54.0cm
B) 37.3cmB)\text{ 37}.3cm
C) 46.0cmC)\text{ 46}.0cm
D) 50.0cmD)\text{ }50.0cm

Explanation

Solution

The total tube length will be the distance between the two lenses. It will be the sum of the image distance of the image formed by the objective and the focal length of the eyepiece. This is because, for the final image to be formed at infinity, the object for the eyepiece (which is the image formed by the objective) must be situated at its focus.

Formula used:
1f=1v1u\dfrac{1}{f}=\dfrac{1}{v}-\dfrac{1}{u}

Complete step by step answer:
The final image formed is at infinity for which the object for the eyepiece must be situated at its focus. Now, the object for the eyepiece is nothing but the image formed by the objective. Therefore, it can be said that the distance between the lenses will be the sum of the image distance of the image formed by the objective and the focal length of the eyepiece.
Now, the focal length ff, image distance vv and object distance uu for a lens is given by
1f=1v1u\dfrac{1}{f}=\dfrac{1}{v}-\dfrac{1}{u} --(1) [Lens formula]
Now, let us analyze the question.
Let the separation between the lenses, that is, the tube length of the telescope be LL.
Let the image distance of the image formed by the objective be v0{{v}_{0}}.
The focal length of the objective is f0=40cm{{f}_{0}}=40cm.
The focal length of the eyepiece is fe=4cm{{f}_{e}}=4cm.
The object distance for the objective is u0=200cm{{u}_{0}}=-200cm.
(The negative sign is due to sign convention).
Now, as explained above, the tube length will be the sum of the image distance of the image formed by the objective and the focal length of the eyepiece.
L=v0+fe\therefore L={{v}_{0}}+{{f}_{e}} --(2)
Now, using (2), we get
1fo=1vo1uo\dfrac{1}{{{f}_{o}}}=\dfrac{1}{{{v}_{o}}}-\dfrac{1}{{{u}_{o}}}
1vo=1fo+1uo\therefore \dfrac{1}{{{v}_{o}}}=\dfrac{1}{{{f}_{o}}}+\dfrac{1}{{{u}_{o}}}
Putting the values of the variables in the above equation, we get
1vo=140+1200=1401200=51200=4200=150\dfrac{1}{{{v}_{o}}}=\dfrac{1}{40}+\dfrac{1}{-200}=\dfrac{1}{40}-\dfrac{1}{200}=\dfrac{5-1}{200}=\dfrac{4}{200}=\dfrac{1}{50}
vo=50cm\therefore {{v}_{o}}=50cm --(3)
Now, using (2) and (3), we get
L=50+4=54.0cmL=50+4=54.0cm
Hence, the required separation between the lenses in the telescope is 54.0cm54.0cm.

So, the correct answer is “Option A”.

Note:
Students may make the mistake of thinking that the tube length of the telescope will be the sum of the focal length of the objective and the eyepiece. However, they must understand that this is valid only in cases of special astronomical telescopes where the object is at infinity and the image is also produced at infinity. In the general case, the tube length of the telescope is the sum of the image distance of the objective and the object distance of the eyepiece.