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Draw a Labeled Ray Diagram to Obtain the Real Image Formed by an Astronomical Telescope in Normal Adjustment Position. Define Its Magnifying Power - Physics

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प्रश्न

Draw a labeled ray diagram to obtain the real image formed by an astronomical telescope in normal adjustment position. Define its magnifying power.

उत्तर

 
 

In normal adjustment, the final image is formed at infinity.

Magnifying power or angular magnification of astronomical telescope: It is defined as the ratio of the angle subtended at the eye by the final image to the angle subtended at the eye, by the object directly, when the final image and the object, both are at infinity.

Angular magnification,`M=beta/alpha`

β and α are very small.

`:.beta~~tan beta`

`alpha~~tanalpha`

`=>M=tanbeta/tanalpha`

I is the image formed by the objective. f0 and fe are the focal lengths of the objective and eyepiece, respectively.

Here,

`tanalpha=I/f_0`

`tan beta=I/-f_e`

(Distance of the image from the eyepiece is taken as negative.)

`:.M=((-I)/f_e)/(I/f_0)`

`M=(-f_0)/f_e`



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Optical Instruments: Telescope
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2015-2016 (March) All India Set 2 C

संबंधित प्रश्न

A small telescope has an objective lens of focal length 140 cm and an eyepiece of focal length 5.0 cm. What is the magnifying power of the telescope for viewing distant objects when

  1. the telescope is in normal adjustment (i.e., when the final image is at infinity)?
  2. the final image is formed at the least distance of distinct vision (25 cm)?

  1. For the telescope is in normal adjustment (i.e., when the final image is at infinity)? what is the separation between the objective lens and the eyepiece?
  2. If this telescope is used to view a 100 m tall tower 3 km away, what is the height of the image of the tower formed by the objective lens?
  3. What is the height of the final image of the tower if it is formed at 25 cm?

Write two important limitations of a refracting telescope over a reflecting-type telescope.


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Read the following paragraph and answer the questions.

A number of optical devices and instruments have been designed and developed such as periscope, binoculars, microscopes and telescopes utilising the reflecting and refracting properties of mirrors, lenses and prisms. Most of them are in common use. Our knowledge about the formation of images by the mirrors and lenses is the basic requirement for understanding the working of these devices.
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