Space Topics: Search for Extraterrestrial Intelligence
The Search for Extraterrestrial Intelligence: A Short History
by Amir Alexander
Part 2: The Founding Moment of SETI
It is, of course, very difficult to pinpoint an exact birth-date for SETI.
Fascination with other worlds and their inhabitants has a long history, dating
back to antiquity. Even the search for radio signals from space stretches
back to experiments by the leading radio pioneers in the earliest days of
radio. But the history of modern SETI does have a clear beginning. In 1959
Philip Morrison and Giuseppe Cocconi were young physicists at Cornell University
interested in gamma rays. "One spring day in 1959," recalls Morrison, "my
ingenious friend Giuseppe Cocconi came into my office and posed an unlikely
question: would not gamma rays, he asked, be the very medium of communication
between the stars?" Morrison agreed that gamma rays would work, but suggested
they should consider the entire electromagnetic spectrum for its possibilities.
The result of this brainstorming was a short two-page article, which was
published in Nature magazine on September 19, 1959. Entitled "Searching for Interstellar
Communications," it is rightly considered the founding document of modern
SETI.
In the article Morrison and Cocconi freely admit that it is impossible to
estimate the probability of the existence of alien civilizations on planets
orbiting distant stars. But based on the only example available - that of
humans on Earth - they argue that one cannot rule out that there may be very
many alien technological societies out there. Many of them, they argue, may
be much older than human societies and far more technologically advanced.
The aliens, furthermore, would in all likelihood consider our Sun to be a
likely candidate for the formation of a technologically advanced civilization,
and would seek to make contact with it. The main question, according to Morrison
and Cocconi, is what means would they choose?
Electromagnetic waves (radio waves, light waves, etc.) they argue are the
obvious choice. Only these, traveling at the speed of light, can cross the
fantastic distances involved without dispersing and in anything resembling
a practical amount of time. This leads to the next crucial question: at what
frequency will the aliens transmit their signal?
The most rational frequencies for communication between the stars, Morrison
and Cocconi argued, were between 1 and 10,000 MHz. Those are the frequencies
in which the planetary atmosphere interferes the least with electromagnetic
signals, and where radiation noise from our galaxy is also at a minimum. Several
years later it was discovered that those were also frequencies in which there
was little interference from Cosmic Background Radiation, but this was not
known in 1959.
SETI - the founding article
The first page of Cocconi and Morrison's classical article in Nature, September 19, 1959.
Credit: Nature Magazine
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A range of frequencies of 10,000 MHz is still far too wide for conducting
a systematic search. Morrison and Cocconi therefore hazarded a guess that
has shaped the course of SETI research to this day: The aliens, they argued,
are most likely to be broadcasting at a frequency of 1420 MHz (wavelength
of 21 cm). That is the emission frequency of the atom of the most common element
in the universe - hydrogen. This frequency would suggest itself because it
would be known to any observer in the universe. Any systematic search should
begin here.
The authors then made another observation, which has had a profound impact
on the way SETI searches are conducted: any signal sent from a the aliens'
orbiting planet to our orbiting planet would necessarily drift away from its
original frequency. This is the result of the Doppler shift, familiar to anybody
who has heard the change of pitch of a train's whistle as it passes by. Because
the speed at which the planets are moving relative to each other constantly
changes, the frequency of the transmission will inevitably drift over time.
A search for an alien signal would have to take this drift into account, and
search for a transmission whose frequency slowly changes.
Morrison and Cocconi concluded their article with a challenge to skeptical
readers. Many, they admitted, would argue that this kind of speculation belongs
in science fiction rather than science. This is not so: their argument, they
claimed, shows that the presence of an alien signal is consistent with all
that is presently known. They concluded with a challenge that has become the
rallying cry for all SETI enthusiasts since: "The probability of success
is difficult to estimate; but if we never search, the probability of success
is zero."
--Amir Alexander
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