All of the following statements are correct except:

  • A
    The total length of an astronomical telescope is the sum of the focal lengths of its two lenses.
  • B
    The image formed by the astronomical telescope is always erect because the effect of the combination of the two lenses is divergent.
  • C
    The magnification of an astronomical telescope can be increased by decreasing the focal length of the eye-piece.
  • D
    The magnifying power of the refracting type of astronomical telescope is the ratio of the focal length of the objective to that of the eye-piece.

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Similar Questions

Diameter of the moon is $3.5 \times 10^3 \, km$ and its distance from earth is $3.8 \times 10^5 \, km$. It is seen by a telescope whose objective and eyepiece have focal lengths $4 \, m$ and $10 \, cm$ respectively. What will be the angular diameter of the image of the moon in degrees?

The objective lens of a telescope has a focal length of $100 \, cm$. When the final image is formed at the least distance of distinct vision,the distance between the lenses is $105 \, cm$. Calculate the focal length of the eyepiece in $cm$.

The magnifying power of a telescope can be increased by

$A$ telescope has an objective lens of focal length $150\,cm$ and an eyepiece of focal length $5\,cm$. If a $50\,m$ tall tower at a distance of $1\,km$ is observed through this telescope in normal setting,the angle formed by the image of the tower is $\theta$,then $\theta$ is close to.....$^o$

In an astronomical telescope,the focal lengths of the objective lens and the eyepiece are $150 \, cm$ and $6 \, cm$ respectively. In the case where the final image is formed at the least distance of distinct vision,the magnifying power is:

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