I had dinner with Gregory Benford last weekend, and he raised a provocative point. So far, radio searches for extraterrestrial life have only seen puzzling brief signals - not long transmissions.
But what if this is precisely what we should expect?A provocative example is Sullivan, et al. (1997). This survey lasted about 2.5 hours, with 190 1.2 minute integrations. With many repeat observations, they saw nothing that did not seem manmade. However, they “recorded intriguing, non-repeatable, narrowband signals, apparently not of manmade origin and with some degree of concentration toward the galactic plane…” Similar searches also saw one-time signals, not repeated (Shostak & Tarter, 1985; Gray & Marvel, Gray, 1994; 199 Tarter, 2001). These searches had slow times to revisit or reconfirm, often days (Tarter, 2001). Overall, few searches lasted more than hour, with lagging confirmation checks (Horowitz & Sagan, 1993). Another striking example is the “WOW” signal seen at the Ohio SETI site...That's a quote from this paper:
• Gregory Benford, James Benford, and Dominic Benford, Searching for cost optimized interstellar beacons,
#spnetwork #mustread #SETI arXiv:0810.3966.
They claim the cheapest way a civilization could communicate to lots of planets is a pulsed, broadband, narrowly focused microwave beam that scans the sky. So, for anyone receiving this signal, there would be a lot of time between pulses. That might explain some of the above mysteries, or this:
As an example of using cost optimized beacon analysis for SETI purposes, consider in detail the puzzling transient bursting radio source, GCRT J17445-3009, which has extremely unusual properties. It was discovered in 2002 in the direction of the Galactic Center (1.25° south of GC) at 330 MHz in a VLA observation and subsequently re-observed in 2003 and 2004 in GMRT observations (Hyman, 2005, 2006, 2007). It is a pulsed coherent source, with the ‘burst’ lasting as much as 10 minutes, with 77-minute period. Averaged over all observations, Hyman et al. give a duty cycle of 7% (1/14), although since some observations may have missed part of bursts, the duty cycle might be as high as 13%.Even if these are red herrings, it seems very smart to figure out the cheapest ways to
transmit signals and use that to
guess what signals we should look for.
The cost analysis is here:
• James Benford, Gregory Benford, Dominic Benford, Messaging with cost optimized interstellar beacons,
#spnetwork #mustread #SETI arXiv:0810.3964.
and you can see a summary in this talk by James Benford, who works on high-power microwave technologies.