A telescope is an optical instrument used to see distant objects clearly and magnified. The telescope was invented in 1608 by a Dutch optician Hans Lippershey. In 1609, the Italian astronomer Galileo made his first telescope and observed the rings of Saturn and Jupiter’s moons. Today there are three main kinds of telescopes: refracting telescopes, reflecting telescopes and radio telescopes.

Refracting Telescopes: A refracting telescope makes use of two lenses fitted at the end of a tube. An astronomical telescope consists of one larger size convex objective lens and a convex eyepiece while a Galilean telescope makes use of a convex objective lens and a concave eyepiece. Modern refracting telescopes usually contain complicated lens systems to correct chromatic aberrations.

Reflecting Telescope: A reflecting telescope is made of a concave mirror that gathers and focuses light waves. Another mirror near the point where waves come together reflects light into the eyepiece.

            A Newtonian telescope uses a mirror set at a 45° angle to reflect the light into the eyepiece. A Casegranian telescope has convex mirror which reflects light through a tiny hole in the centre of the objective mirror. The light passes through to the eyepiece, which makes the image larger.

           The largest reflecting telescope in the world is at the Yerkes observatory in Wisconsin. Its objective lens has a 102cm diameter. The Palomar observatory in California has a reflecting mirror with a diameter of 508cm.

Radio Telescopes: A radio telescope has a huge reflector shaped like a bowl which reflects radio waves to a detector. Radio telescopes are used in astronomy. These telescopes can be used under all weather conditions.