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The Meade Instruments (also shortened to Meade) was an American multinational company headquartered in Watsonville, California, that manufactured, imported and distributed telescopes, binoculars, spotting scopes, microscopes, CCD cameras, and telescope accessories for the consumer market. [2]
The observatory includes a 20.5 foot ASH dome housing a 16" LX200GPS SCT Meade telescope. Four smaller 12" LX200GPS Meade telescopes are used on two observation decks. (See Meade LX200 )
Meade ETX telescope; Meade LX90; Meade LX200; MySky This page was last edited on 24 December 2019, at 07:48 (UTC). Text is available under the Creative Commons ...
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.
The Meade LX90 is a Schmidt-Cassegrain design of telescope made by Meade Instruments for the mid-priced (2000 USD circa 2008) commercial telescope market. [1] [2] It uses a similar optical system to the bigger and more expensive Meade LX200 [2] —although it lacks some useful functions like primary mirror locking.
The ETX started out as a 90 mm (3-1/2") Maksutov Cassegrain telescope (first produced in 1996) and took advantage of high volume mass production and simplified optical and parts construction to open a new market for a cheap alternative to the very expensive Questar 3-1/2 Maksutov Cassegrain [1] [2] The ETX "line" has been expanded to 105 mm, and 125 mm Maksutov Cassegrains and achromatic ...
Meade Instruments would eventually become the world's largest telescope manufacturer for amateur astronomy, with distribution in over thirty countries. Diebel received the Franklin Institute's Bower Award for Business Leadership in 1998 [ 1 ] and retired from Meade Instruments in 2003.
A weather station was also in operation since March 2008. Finally, a 400mm MEADE telescope with an SBIG spectrograph was used to obtain spectral measurements of the sky background. [3] In parallel, a study on cloud cover was commissioned using high-resolution satellite images of the Pico del Buitre area for the years 2005 and 2006.
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