Astronomical telescope
Astronomical Telescope
The astronomical telescope is an optical instrument used to observe celestial bodies such as stars, planets, galaxies, and other astronomical objects. The telescope is a key tool in astronomy, a science dedicated to the study of celestial objects, the physics, chemistry, and evolution of such objects, and phenomena that occur outside the Earth's atmosphere.
History[edit | edit source]
The first known practical telescopes were invented in the Netherlands at the beginning of the 17th century, by using glass lenses. They found use in both terrestrial applications and astronomy. The first recorded astronomical telescope was a refracting telescope, which was invented by Galileo Galilei in 1609.
Types of Astronomical Telescopes[edit | edit source]
There are three main types of astronomical telescopes: refracting, reflecting, and catadioptric.
Refracting Telescopes[edit | edit source]
Refracting telescopes use lenses to gather and focus light. They are the oldest type of telescope and have been around since the invention of the telescope.
Reflecting Telescopes[edit | edit source]
Reflecting telescopes use mirrors to gather and focus light. They were invented as a solution to the chromatic aberration seen in refracting telescopes.
Catadioptric Telescopes[edit | edit source]
Catadioptric telescopes use a combination of mirrors and lenses to gather and focus light. They are designed to bring the benefits of both refracting and reflecting telescopes.
See Also[edit | edit source]
References[edit | edit source]
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Contributors: Prab R. Tumpati, MD