|
Fall 2005 Issue |
|
|
DR. SETI’s STARSHIP Shouting in the Jungle By Dr. H. Paul Shuch,* N6TX |
|
|
Nearly half a century of SETI science, and still not a single confirmed transmission from “Be- yond.” What kind of DXpedition is this? When Frank Drake conducted the world’s first SETI experiment in 1960, he was just days into the project when he heard a loud, periodic signal from Up There. “My God,” he thought, “could it really be this easy?” The signal was, of course, RFI, a phenomenon with which every subsequent effort to detect evidence of extraterrestrial intelligence has been plagued. No, it wasn’t that easy, then or now. The bands, it seems, are dead. After a while, when the band seems dead, any sensible ham will want to stir the pot. So why aren’t we calling CQ? The whole question of transmitting from Earth is fraught with controversy. Every ham knows that if everyone is listening and no one is transmitting, no one is going to know when a band opening occurs. That’s one of the reasons why we put propagation beacons on the air from exotic locations. Early on, SETIzens thought that advanced extraterrestrial civilizations would accommodate us immature Earthlings by providing just such beacons, to draw us into membership in the Galactic Club. Thus, the early SETI experiments, beginning with Drake’s, concentrated on searching nearby sun-like stars for just such strong and steady beacons. If they are abundant, you’d think we would have heard one by now.
We haven’t, though, and not necessarily
because the bands are dead. Maxwell’s laws quantify propagation, and they
suggest that even a modest beacon, properly aimed, will easily be
detectable by Earth’s receive technology, across the interstellar gulf.
Maybe, then, it’s time to rethink our assumptions. Advanced civilizations,
if indeed they exist, apparently don’t announce their presence using radio
waves. Do they perhaps know something we don’t? |
![]() The San Marino Scale is an ordinal scale between one and ten used to quantify the relative risk of a given electromagnetic transmis-sion from Earth. Each numeric San Marino Scale value correlates to a subjective measure of risk, from Insignificant to Extraordinary. |
|
Click here to return to Fall 2005 highlights Click here to subscribe to VHF _________________ © Copyright 2005, CQ Communications, Inc. All rights reserved. This material may not be reproduced or republished, including posting to a website, in part or in whole, by any means, without the express written permission of the publisher, CQ Communications, Inc. Hyperlinks to this page are permitted.
|
|