Equatorial Telescope Mounts![]() As a result of the Earth's rotation, the right ascension coordinate drifts across the sky along a path parallel to the celestial equator. Once the telescope is adjusted to point at an object's sky coordinates (right ascension and declination), it is simply a matter of driving the right ascension axis with a motor to keep up with the object as it moves. ![]() "Equatorial Telescope Mounts" from The Wolfram Demonstrations Project http://demonstrations.wolfram.com/EquatorialTelescopeMounts/ Contributed by: Jeff Bryant |
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