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Celestial cartography
Celestial cartography, uranography or star cartography is the fringe of astronomy and branch of cartography concerned with mapping stars, galaxies, and other astronomical objects on the celestial sphere. Measuring the position and light of charted objects requires a variety of instruments and techniques. These techniques have developed from angle measurements with quadrants and the unaided eye, through sextants combined with lenses for light magnification, up to current methods which include computer automated space telescopes. Uranographers have historically produced planetary position tables, star tables and star maps for use by both amateur and professional astronomers. More recently computerized star maps have been compiled, and automated positioning of telescopes is accomplished using databases of stars and other astronomical objects.
==Etymology==
The word "uranography" derived from the Greek "ουρανογραφια" (Koine Greek ''ουρανος'' "sky, heaven" + ''γραφειν'' "to write") through the Latin ''"uranographia"''. In Renaissance times, ''Uranographia'' was used as the book title of various celestial atlases.〔1690: Hevelius J., ''Firmamentum Sobiescianum sive Uranographia''.〕〔c. 1750: Bevis J., ''Uranographia Britannica''.〕〔1801: Bode. J. E., ''Uranographia sive Astrorum Descriptio''.〕 During the 19th century, "uranography" was defined as the "description of the heavens". Elijah H. Burritt re-defined it as the "geography of the heavens".〔Burritt, E. H., ''The Geography of the Heavens'', 1833.〕 The German word for uranography is "''Uranographie''", the French is "''uranographie''" and the Italian is "''uranografia''".
抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』
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