If SETI@home is now a respectable 10 years old, Project SERENDIP's roots go back much further. The first SERENDIP was built at U.C. Berkeley in 1979, and collected data from the radio telescope at the Hat creek Observatory in California. Since then the project's hardware has been upgraded repeatedly: In 1992 SERENDIP's 3d generation was installed at the Arecibo radio telescope, the largest and most sensitive in the world. Five years later, with help from The Planetary Society, this system was replaced at Arecibo by SERENDIP IV, which continued in operation for the next 8 years. And now SERENDIP V is set to take over and continue a long and persistent search that began three decades ago. As
SERENDIP was upgraded repeatedly over the years, each new generation
represented a quantum leap over the capabilities of its predecessor.
SERENDIP I, for example, could look at 100 channels at a time, which
seemed pretty impressive back in 1979. But its successor, which began
operations in 1986, could look at 65,000 channels at a time, and with
SERENDIP IV the number was up to 168 million! Such exponential growth
is unheard of in most scientific fields, but is not unusual in SETI,
which is always on the lookout for new cutting-edge technologies for
scanning the skies.
(Read more about this project here) |
