CURRENT STATUS OF RESEARCH AND FUTURE PROSPECTS
Clearly the SETI project has no obvious hunting ground or no clear route to
discovery. In 40 years of data collection, actual experimental evidence has
been missing. We still have not detected any undebatable signals from the
extra terrestrial intelligence that we presume is somewhere out there.
With 400 billion stars in the Milky Way itself, the search is analogous to
seeking a needle in a haystack. Also the astronomical distances that
signals need to cover before they reach earth causes them to diminish in
intensity.
At present Project Phoenix uses the Arecibo Telescope to examine nearby,
Sun-like stars for narrow band microwave signals. Other SETI searches
also sweep wide areas of the sky in the hunt for such signals.
Over the years of observation we have found evidence that planets are
abundant, but we still do not know about the existence of life-supporting
conditions on them. Also over the decades we have developed powerful
lasers and supercomputers.
Today research involves studying both radio and optical signals for extraterrestrial
signals. Recent developments include an improved detector for
targeted optical SETI that reduces the number of false alarms from
typically once a night to once a year! Radio SETI searches too benefit from
the technology leaps.
The ideal SETI radio telescope would monitor every point on the sky, in
every radio channel from one end of the microwave window of the earth
to the other all the time. This projects called the Omnidirectional Search
System, or OSS.
The Moore's Law in computing predicts a thousandfold improvement in
computational power in 15 years. If this happens then OSS can be a reality
at the end of that time period.
Presently the most sensitive project is Phoenix. But the Phoenix is not
sensitive enough to even pick up leakage satellite and television signals
from the earth at a distance equal to that of the Alpha Centaur (the
nearest star to earth.) For sheer sensitivity, SETI's dream instrument is the
proposed Square Kilometer Array, or SKA. This grand radio telescopes
would be a mammoth device with a total collecting area of one square
kilometer.
No one can predict the ultimate outcome the search. However the
powerful next generation instruments will surely raise the probability of a
finding if such extra-terrestrial intelligence actually exists.
ACKNOWLEDGEMENTS
We would like to thank Prof. V. M. Gadre for the wonderful opportunity he
provided us to explore this fascinating subject through the assignment.
REFERENCES
The SETI Institute.
SETI@Home Project
Princeton OSETI Center
SERENDIP Project
Sky and Telescope Magazine
Discrete Fourier Transform – David Gilliam (Texas Tech Univ.)
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