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  2. GoTo (telescopes) - Wikipedia

    en.wikipedia.org/wiki/GoTo_(telescopes)

    For an equatorial GoTo telescope mount, the user must align the mount by hand with either the north celestial pole or the south celestial pole. Assuming the user is accurate in the alignment, the mount points the telescope to a bright star, asking the user to center it in the eyepiece.

  3. Equatorial mount - Wikipedia

    en.wikipedia.org/wiki/Equatorial_mount

    A large German equatorial mount on the Forststernwarte Jena 50cm Cassegrain reflector telescope. An equatorial mount is a mount for instruments that compensates for Earth's rotation by having one rotational axis, called polar axis, parallel to the Earth's axis of rotation. [1] [2] This type of mount is used for astronomical telescopes and cameras.

  4. Equatorial platform - Wikipedia

    en.wikipedia.org/wiki/Equatorial_platform

    A large portable Newtonian telescope on an altazimuth mount with a third equatorial axis platform mount consisting of a pivot and radius bearing surfaces.. An equatorial platform or equatorial table is an equatorial telescope mount in the form of a specially designed platform that allows any device sitting on it to track astronomical objects in the sky on an equatorial axis. [1]

  5. Meade LX200 - Wikipedia

    en.wikipedia.org/wiki/Meade_LX200

    The Meade LX200 is a family of commercial telescopes produced by Meade Instruments launched in 1992 with 8" (20.32 cm) and a 10" (25.4 cm) Schmidt–Cassegrain models on computerized altazimuth mounts. [1] [2] Two larger models, a 12" (30.48 cm) and a 16" (40.64 cm), quickly followed.

  6. Meade Instruments - Wikipedia

    en.wikipedia.org/wiki/Meade_Instruments

    Many Meade telescope lines are classified by the self aiming computerized alt-azimuth and equatorial mounts they come on, a technology commonly called a "GoTo" mount. Models. LXD75, including Newtonian, Schmidt-Newtonian, Advanced Coma-Free, and achromatic refractor telescopes

  7. GOTO (telescope array) - Wikipedia

    en.wikipedia.org/wiki/GOTO_(telescope_array)

    The Gravitational-wave Optical Transient Observer (GOTO) is an array of robotic optical telescopes optimized for the discovery of optical counterparts to gravitational wave events [1] and other multi-messenger signals. The array consists of a network of telescope systems, with each system consisting of eight 0.4m telescopes on a single mounting ...