Constructed in 1958 this telescope was the first radio telescope located at the National Radio Astronomy Observatory in Green Bank, West Virginia. Astronomers used this telescope to examine large radio objects in space, including other solar systems. Following the construction of two of 85-foot radio telescopes at the observatory, the Tatel telescope would become a part of the Green Bank Interferometer, from 1978 to 2000. Despite the Tatel Telescope only expected to function for 20 years it remained active for over 40 years. Operations by the Tatel telescope stopped on October 6, 2000, while the other two 85-foot telescopes continued their contracted work on different projects.
National Radio Astronomy Observatory established a site at Green Bank, West
Virginia without a radio telescope. The kit needed to construct their first
radio telescope arrived in summer of 1958 and finished construction in early
1959. Named after Howard Tatel, who worked for the Carnegie Institute
Department of Terrestrial Magnetism, creating the initial design of the
telescope, making it both more precise and cheaper to build. Tatel did not see
the finished telescope because of his death in 1957, while the first telescope
was still under construction. Green Bank’s 85-1 telescope would be named in his
memory on October 16, 1958, during its dedication. The Tatel Telescope gave
astronomer brighter and more accurate information on radio objects in space
previously available. Including objects located within the solar system, such
as the surface temperature of the moon and studies of Jupiter’s radiation belt.
The telescope was only expected to work for twenty years, despite this, the
telescope continued to function and remained in use until October 2000.
13, 1959, the Tatel Telescope began its 24-hour examination of the universe,
examining the brightest known radio objects, including supernovas and galaxies.
Astronomer Frank Drank used this telescope to create a detailed map of the Milky
Way galaxy. Discovering a never seen complexity of radio waves coming from the
galaxy’s core. In 1960 for two months Drake turned the telescope towards two
nearby sun-like stars, Tau Ceti and Epsilon Eridani, searching for possible
signals from an alien civilization. The project used a 21-cm line of hydrogen,
“the most common radio signal in the universe” to search for radio
transmissions with minimal interference. They did not find any evidence of
alien life near either star, but during research, they received a false signal
caused by airplanes. After the construction of two additional 85-foot
telescopes using the same design as the Tatel Telescope, these three telescopes
combined to become the Green Bank Interferometer, using multiple telescopes to
gain a better perception of the target. From 1978 to 1996 the GBI was used to
study the Earth’s rotation and a variety of radio signals. Then from 1996 to
2000, its focus shifted to studying gamma and x-rays of stars with partial
funding from NASA. The GBI would continue its work until October 6, 2000, but
the individual telescopes remained in operation focusing on other projects they
were contracted to perform.