Search for Extraterrestrial
Intelligence (SETI)
SETI projects aim to detect signals from advanced civilizations elsewhere
in our galaxy. This usually involves searching for radio signals, but other
approaches, such as searching for signals in the form of light pulses (optical
SETI) are also possible.
The Southern SERENDIP Project is a SETI project using the Parkes radio
telescope in New South Wales. The SETI project operates in a piggyback
mode on the 21cm Multibeam Survey, a radio survey of the southern sky.
The SERENDIP instrument can scan 58 million spectral channels simultaneously,
in a range of wavelengths around the neutral hydrogen line at 1420MHz.
Southern SERENDIP is operated by the SETI Australia Centre at the University
of Western Sydney.
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Parkes Radio Telescope
©Australia Telescope National Facility |
Multibeam Receiver used
for Southern SERENDIP |
Southern SERENDIP is one of a number of SETI projects operating
around the world. The SERENDIP project of the University of California
at Berkeley is a similar piggyback survey using the 1000 foot radio
telescope at Arecibo in Pueto Rico. Project Phoenix is a targeted
search looking for signals from planets orbiting nearby stars. In
1995 Project Phoenix made observations in the southern hemisphere
using the Parkes radio telescope, but is now searching the northern
sky using the Green Bank observatory in the USA. It is run by the
SETI Institute in California.
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