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Radio Astronomy Laboratory SETI Institute Altitude: 986 m (3,235 ft) Wavelength: 60, 2.7 cm (500, 11,100 MHz) Telescope style: Gregorian telescope radio interferometer Number of telescopes: 42 Diameter: 6.1 m (20 ft 0 in) Secondary diameter: 2.4 m (7 ft 10 in) Collecting area: 1,227 m 2 (13,210 sq ft) Website: www.seti.org /ata
From 1995 through March 2004, Phoenix conducted observations at the 64-meter (210 ft) Parkes radio telescope in Australia, the 140-foot (43 m) radio telescope of the National Radio Astronomy Observatory in Green Bank, West Virginia, and the 1,000-foot (300 m) radio telescope at the Arecibo Observatory in Puerto Rico. The project observed the ...
SETI@home ("SETI at home") is a project of the Berkeley SETI Research Center to analyze radio signals with the aim of searching for signs of extraterrestrial intelligence. Until March 2020, it was run as an Internet-based public volunteer computing project that employed the BOINC software platform.
Primary lens: The objective of a refracting telescope. Primary mirror: The objective of a reflecting telescope. Corrector plate: A full aperture negative lens placed before a primary mirror designed to correct the optical aberrations of the mirror. Schmidt corrector plate: An aspheric-shaped corrector plate used in the Schmidt telescope.
Hat Creek Radio Observatory is located approximately 467 km (290 mi) northeast of San Francisco, California at an elevation of 986 m (3235 ft) above Sea Level in Hat Creek, California (in Shasta County). Latitude: 40° 49' 03" N; longitude: 121° 28' 24" W.
The Berkeley SETI Research Center also hosts the Breakthrough Listen program, [4] [5] [6] which is a ten-year initiative with $100 million funding begun in July 2015 to actively search for intelligent extraterrestrial communications in the universe, in a substantially expanded way, using resources that had not previously been extensively used for the purpose.
The search was publicized in articles in the popular media of the time, such as Time magazine and was described as the first modern SETI experiment. [2] Drake used a radio telescope with a diameter of 85 feet (26 m) to examine the stars Tau Ceti and Epsilon Eridani near the 1,420 MHz marker frequency, the equivalent of wavelength of 21 ...
32m RT-32 radio telescope, operating range 1.4–22 GHz. [permanent dead link ] Svetloe Radio Astronomical Observatory Svetloe, Karelia, Russia 1.4–22 GHz 32m RT-32 radio telescope, operating range 1.4–22 GHz. [34] RT-7.5 (Bauman's radio telescope) Moscow Oblast, Russia Two 7.75-meter diameter antennas (only one is working at the moment ...