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New Alien-Life Search Aims to Eavesdrop on ETs

John Roach
for National Geographic News
January 11, 2007
 
Do extraterrestrials sweep their skies with radar to scan for incoming missiles?

If so, Avi Loeb of the Harvard-Smithsonian Center for Astrophysics in Cambridge, Massachusetts, thinks he can find the radio signals leaked from warring alien civilizations.

He might also be able to catch their version of reality TV and talk radio.

The concept is different than other radio programs in the search for extraterrestrial intelligence (SETI) that look for high-frequency signals deliberately beamed across space to make contact with distant civilizations.

Extraterrestrials may not emit such beacons, Loeb theorizes.

"However, our own civilization is transmitting power unintentionally through radio and TV broadcasting and military radars," he said in a videotaped presentation played Wednesday to reporters at a meeting of the American Astronomical Society in Seattle, Washington.

"An interesting question is whether we can eavesdrop on another civilization at the frequencies that we are ourselves transmitting in," he said.

(See related story: "Are Neighborhood Aliens Listening to Earth Radio?" [September 7, 2006].)

Piggyback Search

Loeb believes he can detect the leaked signals by piggybacking his search on a new generation of radio telescopes designed to study low-frequency radio emissions in the distant, infant universe.

He and his colleagues hope to test the theory with the Mileura Wild-Field Array currently under construction in Australia and is slated to start operations in 2008.

In its current configuration, the array will be sensitive to any Earth-like civilizations that may exist on a planet orbiting one of about a thousand stars up to 30 light-years away, Loeb said.

Future observatories, such as the Square Kilometer Array proposed for development in Australia or southern Africa, could detect Earth-like planets ten times farther away, which would encompass 100 million stars.

If radio emissions were detected from a distant planet, additional observations could tell astronomers about the host star's mass, the orbit of the planet, and the distance between the two, Loeb noted.

"That by itself would allow us to decide whether there could be liquid water on the surface of the planet and whether that can support life as we know it," he said.

(See a gallery of what life on other planets might look like.)

High Frequency

Peter Backus is the observing programs manager at the SETI Institute in Mountain View, California. He said the institute's radio telescope under construction in northern California is also exploring new regions of the frequency spectrum.

"Just as [Loeb]'s paper talks about the low-frequency end, we're expanding up to higher frequencies that really haven't been searched at all," he said at the briefing.

Previous searches looked at the frequency range between 1,200 and 3,000 megahertz.

The new telescope, named the Allen Telescope Array after its primary donor, Microsoft cofounder Paul Allen, will go up to 11,200 megahertz, Backus said.

Preliminary tests reveal that nearly 90 percent of that band is available to detect extraterrestrial transmissions.

The array configuration will also allow simultaneous examinations of several patches of the sky.

"That gives us a lot of flexibility in what we can do and how much we can do at one time," Backus said.

Ultimately the array will consist of 350 20-foot (6-meter) dishes spread out over 2,300 feet (700 meters). Currently 36 of the antennas are online with 42 expected to boot up this summer.

Though originally conceived as a telescope primarily for SETI, Backus said radio astronomy projects will direct where the array points. Within the field of view are bound to be several of the million or so SETI candidate stars.

"Although a certain fraction of the time we'll have to point the array to follow up on result candidates," he noted.

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