CETI from Copernicus

Details CETI from Copernicus CETI from Copernicus

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975spfl...17..328l&link_type=abstract

Spaceflight, vol. 17, Aug.-Sept. 1975, p. 328-330.

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Applications

Extraterrestrial Life, Interstellar Communication, Laser Applications, Oao 3, Satellite Observation, Spaceborne Astronomy, Space Shuttles, Spacelab, Ultraviolet Radiation, Wideband Communication

Scientific paper

Copernicus is now scanning three solar class stars, Epsilon Eridani, Tau Ceti, and Epsilon Indi for signs of laser emission, particularly ultra-violet wavelengths between 930 and 3,000 A. The paper discusses the basis of the experiments, speculates on methods of generating the particular signals involved and gives the names and characteristics of other possible nearby CETI candidates. Copernicus apparatus will not be able to decode any intelligent signal if received. Sophisticated receiving and decoding gear (local oscillator laser, and a suitable wide-band radio amplifier and detector system) are suggested for the Space Shuttle and Spacelab programs.

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