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ASTRONOMICAL TELESCOPE

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ASTRONOMICAL TELESCOPE
Shared by: Ali Raza
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11/6/2011
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ASTRONOMICAL TELESCOPE

Introduction

It is an optical instrument used to view heavenly bodies such as moon,stars,

planets and distant object.

Construction

Astronomical telescope consists of two convex lenses:

Objective

Eye piece

Objective

The objective is a convex lens of large focal length and large aperture. It usually

made of two convex lenses in contact with each other to reduce the chromatic and

spherical aberrations.

Eye piece



The eye piece is also a convex lens .Its focal length is smaller than that of

objective. It is also a combination of two lenses. The objective is mounted on a

wide metallic tube while the eye piece is mounted on a small tube .The distance

b/w the eye piece and the objective can be changed by moving tubes.









WORKING

The rays coming from a distant object falls on objective as parallel beam at some

angle say "" and these rays after refraction and passing through the objective

converge at its focus and make an inverted & real image AB. This image acts as

an object for the eye piece. The distance of the eye piece is so adjusted that the

image AB lies within the focal length of the eye piece. The eye piece forms the final

image .The final image is magnified ,virtual and inverted with respect to object.

The final image is formed at infinity.

MAGNIFYING POWER



The magnifying power (M) of astronomical telescope is given by:









It is because the object is at infinite distance and hence the angle subtended by

the object at eye may be taken as the angle subtended by the object at objective.

M = 

since  and are small angles, therefore we can take:

 = tan ...................

and.....................

 = tan 



................

In right angled triangles AOB & AEB









...................

This expression shows that in order to obtain high magnification, focal length of

object must be large and that of eye piece is small.

LENGTH OF TELESCOPE

The distance b/w objective lens and the eye piece is equal to the length of the

telescope.

From figure:

OE = length of telescope =L

But

OE = OB + BE

OB = Fo & BE = Fe

OR



OR

L = focal length of objective + focal length of eye piece


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