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"NODO" redirects here. For other uses, see Nodo.
Observatory
The NASA-LMT was a 3 m (9.8 ft) apertureliquid-mirror telescope located in NODO's main dome. It consisted of a 3 m diameter parabolic dish that held 4 U.S. gallons (15 L) of a highly reflective liquid metal, mercury, spinning at a rate of 10 rpm, with sensors mounted above on a fixed structure. Due to the primary mirror's material, the NASA-LMT was configured as a zenith telescope. Using 20 narrowband filters, it cataloged space debris in Earth's orbit. The telescope was initially completed in 1994 at NASA's Johnson Space Center, and moved to Cloudcroft the following year, where it operated routinely until June 2002. The LMT was also used for the UBC-NASA Multi-Narrowband survey, which examined galaxies at moderate redshifts. When it was retired, some of the components were used in the 6 m (20 ft) Large Zenith Telescope in British Columbia.
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