EXTRATERRESTRIAL LIFE

Introduction
There is no evidence of extraterrestrial life now, but astronomers valiantly continue the search.
This quest is called SETI, for Search for Extra Terrestrial Intelligence. Most SETI projects use radio telescopes to listen for radio signals from planets in distant star systems.
The Arecibo telescope in Puerto Rico is the largest radio telescope in the world. It has a hemisphere shape with a diameter of 305 meters (1000 feet) at its brim. It focuses incoming electromagnetic waves onto a feed arm.

Proponents
Noted author Carl Sagan (1934 - 1996) was one of the leading proponents of SETI.
Astronaut Buzz Aldrin is also a proponent. He proposed building a radio telescope on the dark side of the Moon. Such a telescope would be shielded from Earth's radio signals.
Project OZMA
Radioastronomer Frank D. Drake carried out the first attempt to detect interstellar radio transmissions, in 1960. He performed this at the National Radio Astronomy Observatory (NRAO) in Green Bank, West Virginia,
Project Ozma was named after the queen of L. Frank Baum's imaginary land of Oz -- a place "very far away, difficult to reach, and populated by strange and exotic beings." The stars chosen by Drake for the first SETI search were Tau Ceti in the Constellation Cetus (the Whale) and Epsilon Eridani in the Constellation Eridanus (the River), some eleven light years (66 trillion miles) away. Both stars are about the same age as our sun.
Project HRMS
As of 1992, NASA was conducting a SETI project called HRMS, for High Resolution Microwave Survey. This was one of several NASA SETI projects. Congress terminated SETI funding in 1993 due to budget pressures, however.
Project Phoenix
Another SETI project is called Project Phoenix. This is a privately funded continuation of the NASA HRMS project. This project will use the Arecibo radio telescope along with others throughout the world. Its strategy is to carefully examine the regions around 1,000 nearby Sun-like stars.

Project Phoenix began its serach using the Parkes 210 foot radio telescope in New South Wales, Australia. This is the largest radio telescope in the Southern Hemisphere. Project Phoenix also uses the Arecibo telescope.
Project Beta
BETA, for Billion-channel Extra-Terrestrial Assay, is another SETI project. This search is performed using the Harvard-Smithsonian radio telescope outside of Boston. Incoming radio waves are fed into a super computer for analysis.
Project SERENDIP
The University of California at Berkeley SETI program, named SERENDIP, was begun in the late 1970's. This project is aimed at detecting narrow band radio signals from extraterrestrial civilizations. It collects data using the Arecibo telescope.
Seti@Home
SETI@home is a scientific experiment that harnesses the power of hundreds of thousands of Internet-connected computers in the search for extraterrestrial intelligence. The data is collected from the Arecibo Radio Telescope in Puerto Rico.

This project is being conducted by the SETI Institute in Mountain View, California.

People interested in participating can download software at:
http://setiathome.ssl.berkeley.edu/
Optical SETI
Some astronomer believe that extraterrestrial worlds might try to communicate with bursts of laser light.

Stuart Kingsley, an amateur astronomer, has an observatory in Columbus, Ohio dedicated to the search for optical signals.

Astronomer Dan Werthimer of the University of California at Berkeley is involved in a similar search using the Leuschner Observatory.

Paul Horowitz, a Harvard astronomer, is also searching for optical signals.
Planets outside of Our Solar System
A number of planets outside our solar system have recently been discovered.
Astronomers Michel Mayor and Didier Queloz of the Geneva Observatory discovered a planet orbiting the star 51 Pegasi, which is in the constellation Pegasus. This star is 42 light-years from the Earth. The discovery was announced in October 1995.
In addition, San Francisco State University astronomers Geoffrey Marcy and Paul Butler have discovered a planet orbiting the star 47 Ursae Majoris. This star is in the Big Dipper and is 34 light-years away from the Earth. The discovery was made on December 30, 1995.
Marcy and Butler have also discovered a planet orbiting the star 70 Virgins, which in the constellation Virgo. This star is also 34 light-years away from the Earth. Note that some astronomers consider that this new "planet" is really a brown dwarf star.
As new planets are discovered, astronomers will investigate the temperature and chemical composition of each. These parameters will help determine whether the new planets are capable of sustaining life. The various SETI projects can then choose whether to focus their radio telescopes on these new planets.
References
1. Michael Milstein, Signs of Light, Smithsonian Air & Space Magazine, September 1999.
2. SETI web site: http://www.seti-inst.edu/seti-info.html


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Please send comments and questions to Tom Irvine at: tomirvine@aol.com

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