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observatory

A Dictionary of Architecture and Landscape Architecture | 2000 | | © A Dictionary of Architecture and Landscape Architecture 2000, originally published by Oxford University Press 2000. (Hide copyright information) Copyright

observatory.
1. Building used for observing natural phenomena, usually astronomical, meteorological, etc., using special instruments, telescopes, etc.

2. Building commanding an extensive view, e.g. a belvedere or gazebo.

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JAMES STEVENS CURL. "observatory." A Dictionary of Architecture and Landscape Architecture. Oxford University Press. 2000. Encyclopedia.com. 10 Jul. 2009 <http://www.encyclopedia.com>.

JAMES STEVENS CURL. "observatory." A Dictionary of Architecture and Landscape Architecture. Oxford University Press. 2000. Encyclopedia.com. (July 10, 2009). http://www.encyclopedia.com/doc/1O1-observatory.html

JAMES STEVENS CURL. "observatory." A Dictionary of Architecture and Landscape Architecture. Oxford University Press. 2000. Retrieved July 10, 2009 from Encyclopedia.com: http://www.encyclopedia.com/doc/1O1-observatory.html

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observatory

World Encyclopedia | 2005 | © World Encyclopedia 2005, originally published by Oxford University Press 2005. (Hide copyright information) Copyright

observatory Location of telescopes and other equipment for astronomical observations. Large optical telescopes are housed in domed buildings, usually sited well away from the smoke of cities. Radio observatories are open sites containing one or more large radio telescopes. The largest radio-telescope dishes have been built in natural mountain hollows: the Arecibo Observatory in Puerto Rico is 300m (975ft) across.

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observatory

A Dictionary of Astronomy | 1997 | © A Dictionary of Astronomy 1997, originally published by Oxford University Press 1997. (Hide copyright information) Copyright

observatory A place from which astronomical observations are made; sometimes the name is also used for an administration building completely separate from the observing site. An observatory contains instruments for detecting electromagnetic radiation from celestial objects at various wavelengths. Before the invention of the telescope, observatories such as those of Ulugh Beg and TychoBrahe had only simple equipment for naked-eye sightings of positions. The development of optical telescopes in the 17th century led to the need for a permanent protective building, usually with a dome that could be opened to view the sky. To ensure the best possible observing conditions, astronomers began in the late 19th century to site their telescopes on high mountains, above the densest parts of the atmosphere. This trend has continued by placing telescopes in orbit, where they can also observe wavelengths such as X-rays, ultraviolet, and infrared that do not penetrate the atmosphere. Radio telescopes, developed after World War II, are not usually housed in observatory buildings, because they are too large and also because they do not need as much protection from the elements as optical telescopes.

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