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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 - Physics

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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)?
संख्यात्मक

उत्तर

Focal length of the objective lens, fo = 140 cm

Focal length of the eyepiece, fe = 5 cm

Least distance of distinct vision, d = 25 cm

(a) When the telescope is in normal adjustment, its magnifying power is given as:

`"m" = "f"_"o"/"f"_"e"`

= `140/5`

= 28

(b) When the final image is formed at d, the magnifying power of the telescope is given as:

`"f"_"o"/"f"_"e"  [1 + "f"_"e"/"d"]`

= `140/5 [1 + 5/25]`

= 28[1 + 0.2]

= 28 × 1.2

= 33.6

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Optical Instruments: Telescope
  क्या इस प्रश्न या उत्तर में कोई त्रुटि है?
अध्याय 9: Ray Optics and Optical Instruments - Exercise [पृष्ठ ३४७]

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एनसीईआरटी Physics [English] Class 12
अध्याय 9 Ray Optics and Optical Instruments
Exercise | Q 9.28 | पृष्ठ ३४७
एनसीईआरटी Physics [English] Class 12
अध्याय 9 Ray Optics and Optical Instruments
Exercise | Q 34 | पृष्ठ ३४९

संबंधित प्रश्न

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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.


  1. A giant refracting telescope at an observatory has an objective lens of focal length 15 m. If an eyepiece of focal length 1.0 cm is used, what is the angular magnification of the telescope?
  2. If this telescope is used to view the moon, what is the diameter of the image of the moon formed by the objective lens? The diameter of the moon is 3.48 × 106 m, and the radius of lunar orbit is 3.8 × 108 m.

You are given the following three lenses. Which two lenses will you use as an eyepiece and as an objective to construct an astronomical telescope ? Give reason

Lenses Power (D) Aperture (cm)
L1 3 8
L2 6 1
L3 10 1

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Write the two important factors considered to increase the magnifying power?


"A telescope resolves whereas a microscope magnifies." Justify this statement ?


Draw a labelled ray diagram of an astronomical telescope to show the image formation of a distant object. Write the main considerations required in selecting the objective and eyepiece lenses in order to have large magnifying power and high resolution of the telescope.


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


A small telescope has an objective lens of focal length 150 cm and an eye piece of focal length 5 cm. If this telescope is used to view a 100 m high tower 3 km away, find the height of the final image when it is formed 25 cm away from the eye piece.


(i) What is meant by resolving power of a telescope?
(ii) State any one method of increasing the resolving power of an astronomical telescope.


Draw a labelled ray diagram of an astronomical telescope in the near point adjustment position. A giant refracting telescope at an observatory has an objective lens of focal length 15 m and an eyepiece of focal length 1.0 cm. If this telescope is used to view the Moon, find the diameter of the image of the Moon formed by the objective lens. The diameter of the Moon is `3.48 xx 10^6`m, and the radius of the lunar orbit is `3.48 xx 10^8`m.


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

  1. the telescope is in normal adjustment,
  2. the final image is formed at the least distance of distinct vision.

Draw a ray diagram for the formation of image of an object by an astronomical telescope, in normal adjustment. Obtain the expression for its magnifying power.


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Assertion: An astronomical telescope has an objective lens having large focal length.

Reason: Magnifying power of an astronomical telescope varies directly with focal length of the objective lens.


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