Copy Link
Add to Bookmark
Report
Info-ParaNet Newsletters Volume 1 Number 596
Info-ParaNet Newsletters Volume I Number 596
Thursday, October 8th 1992
(C) Copyright 1992 Paranet Information Service. All Rights Reserved.
Today's Topics:
another gratuitous UFO reference
Micro-citation on Aurora
SETI and October 12th
Nasa To Begin Search For Inhabited Planets
SETI - Part 1
SETI - Part 2
SETI - Conclusion
-------------------------------------------------------------------------------
From: cbmvax.cbm.commodore.com!vanth!jms
Subject: another gratuitous UFO reference
Date: 2 Oct 92 07:26:14 GMT
From: vanth!jms@cbmvax.cbm.commodore.com (Jim Shaffer)
Heard on 'Cheers' tonight, when Norm and Cliff have just walked into a bar
with a lot of neon lights:
Norm: 'Wow, this looks like the inside of a UFO.'
Cliff: 'No, actually that's much different.'
--
* From the disk of: | jms@vanth.uucp | 'there's a hell of
Jim Shaffer, Jr. | uunet!cbmvax!vanth!jms | a good universe
37 Brook Street | jms%vanth@cbmvax.commodore.com | next door; let's go'
Montgomery, PA 17752 | 72750.2335@compuserve.com | (e.e. cummings)
--------------------------------------------------------------------
From: sdsu.edu!infinity%mintaka
Subject: Micro-citation on Aurora
Date: 2 Oct 92 21:34:04 GMT
From: infinity%mintaka@sdsu.edu (David E. Coleman)
Just for someone's canonical Aurora bibliography:
Land Investment News (Sherman Oaks, CA), Summer '91 (23:3), p. 5 'Coffee Break.'
.......
What goes on in Lockheed's Skunk Works in Palmdale is a well-kept
secret. However, there are rumors that the firm is working on a project
code-named 'Aurora' that may have something to do with Stealth aircraft
technology.
Well, that's all; sorry; just thought it couldn't hurt to note that people
are becoming aware of Aurora.
Land Investment News is dedicated solely to real estate goings-on
in the high desert North of Los Angeles.
More galactic thoughts from:
Amicitia Subjugat Omnia Hweohthte... (Hwe-oath-T)
---- ---- ---- ---- ---- ---- ---- ---- ---- ---- ---- ---- ---- ---- ----
David E. Coleman infinity@wam.umd.edu
8125 48th Ave, Apt. 612
College Park, MD 20740 1-(301)-474-7424
---- ---- ---- ---- ---- ---- ---- ---- ---- ---- ---- ---- ---- ---- ----
--------------------------------------------------------------------
From: Michael.Corbin@p0.f428.n104.z1.FIDONET.ORG (Michael Corbin)
Subject: SETI and October 12th
Date: 5 Oct 92 07:02:01 GMT
As many of you know, October 12th will mark the beginning of the Search for
Extraterrestrial Intelligence by NASA. I am following this message with some
information that pertains to this endeavor and what NASA plans to do if
discovery is made that there are intelligently-coded signals coming to Earth.
One of our NASA insiders has told us that NASA may use this opportunity to
introduce a confirmation that there is indeed intelligent life out there which
may be able to get the government off the hook with the saucer business
without getting into too much hot water with the public over the secrecy and
knowledge that someone may have been coming here for years. Whatever the
outcome, it is interesting to note what procedures will be used to bring it
out.
Finally, we have received information that Budd Hopkins, Stan Friedman, Linda
Howe and John Scheussler attended a UN meeting last Friday. At this time, we
do now know what the deal is, but we will have some answers tomorrow.
Mike
--
Michael Corbin - via ParaNet node 1:104/422
UUCP: !scicom!paranet!User_Name
INTERNET: Michael.Corbin@p0.f428.n104.z1.FIDONET.ORG
--------------------------------------------------------------------
From: Michael.Corbin@p0.f428.n104.z1.FIDONET.ORG (Michael Corbin)
Subject: Nasa To Begin Search For Inhabited Planets
Date: 5 Oct 92 07:02:02 GMT
* Forwarded from "Alt.Alien.Visitors"
* Originally from Anna Anderson
* Originally dated 10-04-92 12:08
From: anna@moxie.hou.tx.us (Anna Anderson)
Date: 4 Oct 92 13:29:53 GMT
Organization: University of Houston
Message-ID: <1992Oct4.132953.22159@moxie.hou.tx.us>
Newsgroups: alt.alien.visitors
> From: baalke@kelvin.jpl.nasa.gov (Ron Baalke)
> Subject: HRMS Press Kit
> Newsgroups: sci.space,sci.astro
> Organization: Jet Propulsion Laboratory
> Date: Sat, 3 Oct 1992 00:57:16 GMT
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
HIGH RESOLUTION MICROWAVE SURVEY (HRMS)
PRESS KIT
OCTOBER 1992
PUBLIC AFFAIRS CONTACTS
NASA HEADQUARTERS, WASHINGTON, D.C.
Office of Space Science and Applications
Michael Braukus
(Phone: 202/358-1547)
Ames Research Center, Mountain View, Calif.
Michael Mewhinney
(Phone: 415/604-9000)
Jet Propulsion Laboratory, Pasadena, Calif.
Mary Hardin
(Phone: 818/354-5011)
CONTENTS
General
Release 1
Media Services Information 3
Quick-Look Facts. 4
Project History 5
Project Objectives 6
Targeted Search 7
Sky Survey 9
Signal Detection Plans 10
Project Management. 11
RELEASE: 92-161
NASA TO BEGIN SEARCH FOR INHABITED PLANETS
On Oct. 12, NASA will begin the most comprehensive search
ever conducted for evidence of intelligent life elsewhere in the
universe.
The search will use telescopes and antennas to detect radio
transmissions from other planetary systems. The search will
commence 500 years after Columbus landed in North America.
"In the first few minutes, more searching will be
accomplished than in all previous searches combined," according
to Dr. John Billingham of NASA's Ames Research Center, Mountain
View, Calif.
"Over the past few decades, " Billingham added, "scientific
opinion has increasingly supported the theory that complex life
may have evolved on planets orbiting other stars in the galaxy
and the universe. In some cases, further evolution may have led to
the emergence of intelligence, culture and technology."
Billingham, the program chief at Ames, said the High
Resolution Microwave Survey (HRMS) consists of two parts -- a
Targeted Search and a Sky Survey.
The Targeted Search will use the largest available radio
telescopes around the world to search the frequency range from
1,000 to 3,000 megahertz, seeking a variety of patterns that may
indicate the presence of an artificially generated signal. A
megahertz is a unit of frequency equal to one million cycles per
second.
The Targeted Search will perform the most sensitive search
ever conducted of solar-type stars less than 100 light-years
distant. The Targeted Search begins from the world's largest
radio telescope at the National Astronomy and Ionosphere Center's
Arecibo Observatory in Puerto Rico. It is operated for the
National Science Foundation by Cornell University.
The Sky Survey will use the 34-meter antennas at NASA's Deep
Space Network sites in the northern and southern hemispheres to
scan the entire sky over the frequency range from 1,000 to 10,000
megahertz. The Sky Survey begins at the Goldstone, Calif., site.
"Because of the large increase in the area of sky and
frequencies covered, a signal will have to be stronger to be
detected by the Sky Survey," Billingham said. "But it could
detect signals emitted in distant regions from directions that
would be overlooked if the search were limited to nearby solar-
type stars," he added.
Both elements of the HRMS are using specially developed
digital signal processing systems capable of simultaneously
analyzing tens of millions of radio frequency channels.
The HRMS is managed by NASA's Ames Research Center, which
also is responsible for the Targeted Search project. The Jet
Propulsion Laboratory, Pasadena, Calif., is responsible for the
Sky Survey.
The HRMS is part of NASA's Toward Other Planetary Systems
program in the Solar System Exploration Division, Office of Space
Science and Applications at NASA Headquarters, Washington, D.C.
- end -
MEDIA SERVICES INFORMATION
NASA Select Television Transmissint on Oct. 12, 1992. Video footage of
the HRMS deployment will be taken for documentary and archival purposes.
Media Coverage
Those interested in attending the initial deployment at
Arecibo on Oct. 12, contact Michael Mewhinney at NASA Ames
Research Center by calling 415/604-9000. Those wishing to attend
the initial deployment at Goldstone, Calif., contact Mary Hardin
at the Jet Propulsion Laboratory by calling 818/354-5011.
Because of limited parking, use of private vehicles at both sites will be
restricted. Buses will be available at both locations to
transport reporters. Reportt the press desks
at either the Holiday Inn, Barstow, Calif., or the Hyatt Dorado
Beach Hotel, Dorado, Puerto Rico, for transportation and
admissionhis telescope is operated for the National
Science Foundation by Cornell University. The new 34-meter (112-
foot diameter) antenna at NASA's Goldstone Deep Space
Communications Complex near Barstow, Calif., will be used for the
Sky Survey.
Time of Deployment: Targeted Search at 3 p.m. EDT, Arecibo,
Puerto Rico; Sky Survey at noon PDT, Goldstone, Calif.
Project Duration: Expected to last until about 2001.
PROJECT HISTORY
The Earth is the only location known to harbor life. But as
knowledge of the nature of lhere may, in the long run, be one of
science's most important and most profound contributions to
mankind and to our civilization." Also in 1972, NASA published
its first report describing how NASA-developed technology could
make such a search possible.
In the years between 1972 and 1988, NASA maintained a low-
level research and development activity that resulted in the
initiation of the Search for Extraterrestrial Intelligence
Microwave Observing Project (MOP) in FY 1989.
In 1992, NASA established the High Resolution Microwave
Survey (HRMS) as part of the Toward Other Planetary Systems
(TOPS) program within NASA's Solar System Exploration Division.
The Sky Survey (scanning the entire sky for strong signals
coming from any direction) will begin observations at noon PDT
using a 34-meter antenna at NASA's Goldstone Deep Space
Communications Complex near Barstow, Calif.
PROJECT OBJECTIVES
The detection and characterization of planetary systems
around other stars is the goal of NASA's Toward Other Planetary
Systems (TOPS) program. Earth's solar system is still the only
known example of a planetary system, and Earth is the only known
planet that sustains life. Recent astrophysical observations
suggest the existence of other planetary systems around distant
stars. The existence of these systems could support the
hypothesis that lifts TOPS program to include a new
project called the High Resolution Microwave Survey (HRMS). The
project will observe the microwave region of the electromagnetic
spectrum in a manner that can detect signals produced by a
distant technology.
Potentially, there are billions of solar systems in the
Milky Way galaxy at tremendous distances from Ear provide for an expanded
comparative study of the universe.
TARGETED SEARCH
Scientists at NASA's Ames Research Center will conduct the
Targeted Search portion of the HRMS.
The Targeted Search will examine 1,000 nearby solar-type
stars within 100 light years distance from Earth (one light year
is approximately 5.9 trillion miles). The objective is to test
the hypothesis that extraterrestrial technologies are
transmitting radio signals whose characteristics are greatly different
from natural sources of radio emissile sensitivity, the largest
available radio telescopes will be used to conduct the Targeted
Search. The number of targets covered will be much larger than
previous searches, and the range of frequencies covered will be
thousands of times greater than all previous searches combined.
To accomplish this, specialized digital signal processing
equipment has been constructed to listen for microwave radio
transmissions reaching the Earth from distant planetary systems.
The specialized digital signal processing equipment will
simultaneously study the radio spectrum over tens of millions of
individual frequency channels, at spectral resolutions ranging
from 1, 2, 4, 7, 14 and 28 helses, a likely form of interstellar
transmission. An automatic data analysis subsystem will be used
to detect the presence of fixed frequency or drifting continuous
wave (CW) signals or sequences of regularly spaced pulses.
The Targeted Search will use the National Science
Foundation's National Astronomy and Ionosphere Center's 305-meter
(1,000-ft) diameter radio telescope located at the Arecibo
Observatory near Arecibo, Puerto Rico, for the initial deployment
of the HRMS on Oct. 12, 1992. Theng very large observations of each
target at each frequency. It will serve as the logistical hub of
the HRMS Targeted Search. Over the next 3 years, three more such
systems will be built and packaged into two mobile research
facility trailers for air transport to the observation sites.
SKY SURVEY
The NASA Jet Propulsion Laboratory, Pasadena, Calif., will
conduct the Sky Survey portion of NASA's HRMS to search for radio
signals from other planetary systems. The Sky Survey will scan
all directions of the sky to cover a wide range of frequencies
from 1,000 to 10,000 megahertz.
NASA's HRMS will conduct a comprehensive, systematic search
of a portion of the microwave radio spectrum to detect evidence
of radio transmissions from other planetary systems. An
intentionally transmitted signal is easiest to detect in a
frequency band where the background radio noise or static is
minimal. One of the quietest frequency bands is the "microwave
window," which lies between 1,000 and 10,000 megahertz. Since
thstic of microwave ally mapping small areas of the sky, called sky
frames. As the observations are completed, over the entire sky.
For each of 31 frequency bands, the sky is divided into sevplex of
NASA's Deep Space Network in California's Mojave Desert. Toward
the latter part of the survey, the search will move to a
The prototype receiver, spectrum analyzer and signal processor
will break up incomiwith 40 megahertz total bandwidth or a
dual polarization mode with 20 megahertz total bandwidth.
Specially designed digital hardware, operating at supercomputer
speeds, will simultaneously process the 2 million channels to
identify and separate intersterch organizations.
After the discovery has been verified, national and
international authorities are to be informed. News of the
confirmed discovery then will be disseminated promptly, openly
and widely through scientific channels and the news media. All data
necessary for the confirmation of the detection will be made
available to the international scientific community through
publications, meetings, conferences and other appropriate means.
No response to any confirmed signal will be sent from Earth
until appropriate international consultations have occurred.
PROJECT MANAGEMENT
NASA Headquarters, Washington, D.C.
Dr. Wesley Huntress Director, Solar System Exploration Division
Dr. Nicholas Renzetti Manager, Telecommunications and Data Acquisition
Science Complex
Goldstone Deep Space Communications Complex
Dr. Michael J. Klein JPL SETI Project Manager and HRMS Sky Survey Manager
Dr. Samuel Gulkis HRMS Deputy Project Scientist
J. Richard Kolden HRMS Sky Survey Implementation Manager
Arecibo Observatory, Puerto Rico
Dr. Daniel Altschuler Director
___ _____ ___
/_ /| /____/ \ /_ /| Ron Baalke | baalke@kelvin.jpl.nasa.gov
| | | | __ \ /| | | | Jet Propulsion Lab |
___| | | | |__) |/ | | |__ M/S 525-3684 Telos | Einstein's brain is stored
/___| | | | ___/ | |/__ /| Pasadena, CA 91109 | in a mason jar in a lab
|_____|/ |_|/ |_____|/ | in Wichita, Kansas.
--
Michael Corbin - via ParaNet node 1:104/422
UUCP: !scicom!paranet!User_Name
INTERNET: Michael.Corbin@p0.f428.n104.z1.FIDONET.ORG
--------------------------------------------------------------------
From: Michael.Corbin@p0.f428.n104.z1.FIDONET.ORG (Michael Corbin)
Subject: SETI - Part 1
Date: 5 Oct 92 07:05:03 GMT
(C) 1991 ParaNet(sm) Information Service. All Rights Reserved.
****************************************************************
ParaNet File Number: 00211
DATE OF UPLOAD: February 24, 1990
ORIGIN OF UPLOAD: ParaNet Headquarters
CONTRIBUTED BY: Michael F. Corbin
========================================================
IS ANYBODY OUT THERE?
by Michael Corbin
As we ponder the question of life elsewhere in the universe,
it is now without question that we should be utilizing our vast
technology to listen for intelligent radio signals coming from
other possibly civilized worlds in the galaxy.
As we continue to breach worldly boundaries with satellite
communications -- television and radio transmissions -- and all
manner of electromagnetic emissions that occur on Earth 24 hours
per day, have you ever wondered what happens to the signals? They
not only reach their intended destinations, but continue endlessly
into the vastness of space in all directions.
To answer our question -- "Is Anybody Out There?" -- we must
turn back the pages of history to the beginning of the radio age.
In a small laboratory in Colorado Springs, Colorado, a young
and enthusiastic inventor and scientist tuned in on what he
believed to be intelligent transmissions from outer space.
Thoroughly convinced that advanced beings were trying to signal
us, Nikola Tesla revealed this event to the public in 1899.
What did Tesla receive? Was it a beacon - much like the one
from the monolith of "2001: A Space Odyssey" - intended to give
life to what we know today as the Search for Extraterrestrial
Intelligence? A beacon to pique our curiosity and to formally
introduce us to perhaps our origins? Or did this research perish
with all of Tesla's research papers when seized by the United
States federal authorities? Read on.
Twenty-two years later, another young and enthusiastic
inventor, Guglielmo Marconi, the father of the "wireless," also
claimed to have received intelligently coded signals from a
civilized world in space.
Although not widely known, but nonetheless public, these
were not the only incidents where radio signals of a seemingly
intelligent nature were received.
A professor of Astronomy at Amherst College, Dr. David Todd
made a photographic record of radio signals emanating from Mars
in 1924 as it made a close approach to Earth.
According to Dr. Ronald Bracewell, a physicist with the
Radio Astronomy Institute at Stanford University, strange and
unexplained signals were received in 1927, 1928, and 1964.
What could account for such activity aside from galactic
neighbors attempting to contact us?
Some unusual radio emissions could have been pulsars.
Pulsars are very unusual because, rather than producing a
continuous radio intensity at the Earth, they produce short,
regularly spaced bursts of radio emission. Typically, these
bursts last about one-twentieth of a second and occur at
intervals of about one second.
However, pulsars were not the cause of an incident that
occurred in 1959 - an incident which shook NASA officials and
began what could be the most intense "Search for Extraterrestrial
Intelligence" to ever come to the fore. NASA detected radio
emissions from an unknown satellite circling the Earth. Perhaps
this was a Soviet satellite; it is unknown, as our research was
unable to find more information.
Following this event, a quiet effort was underway to begin a
listening project. It was called OZMA and was organized by Dr.
Otto Struve, one of the most distinguished astronomers of that
time and associated with the National Science Foundation.
Notwithstanding a public gone crazy on UFO activity, this
project's credibility was boosted by Dr. Struve's impressive
background and credentials which carried a lot of weight in the
scientific community. Dr. Struve announced soberly to the press
that there could be one million intelligently inhabited planets
in our galaxy alone.
Appointed by Struve, Dr. Frank Drake was Project OZMA's
director. Drake also echoed Struve's sentiments by pointing out
the tremendous benefits to our world by establishing contact with
beings far advanced of us.
Although the subject of UFOs was not discussed, the Air
Force was very uneasy about this listening project.
During formation of OZMA, it was determined by Philip
Morrison and Giuseppe Cocconi that a frequency of 1420 mHz would
be a universally recognizable communication channel.
In 1961, Drake and his staff at the National Radio Astronomy
Observatory in Green Bank, West Virginia took their first step in
the search by focusing on Tau-Ceti, one of the nearest suns
likely to have intelligent life.
Within two minutes something totally shocking happened.
They were receiving intelligently coded signals from the Tau-Ceti
system. As Dr. Drake related later, "the spooky signals had had
an unexpected effect on everyone." Within a short period of
time, the signals faded leaving the scientists in the room
literally stunned.
To avoid possible public panic, all discussion of this event
was kept quiet, but because of the sensational magnitude of the
event, word quickly leaked to the public. A swift and lethal
blow to the credibility of the project soon followed from the
Pentagon, which stated that the strange signals had been received
from a military station so secret that its identity could not be
revealed.
Abruptly, Dr. Struve closed Project OZMA. At a conference
before a bewildered press, Dr. Struve shocked them by stating
that it was "folly" to listen for messages from space, and
besides, it might be unwise for us to answer them without first
knowing their identity and possible intentions.
Quite peculiar behavior for a man of Struve's credentials,
considering his strong comments in favor of the project, not to
mention subsequent events in the SETI story.
Were the strange signals merely from an earthly military
station? Perhaps. But, if this were the case, would OZMA have to
close so abruptly? One can reasonably argue "no."
On the other hand, consider next the actions of a man who
claimed it was "folly" to listen in on our galactic neighbors.
With some urgency and in complete secret, November 1961 saw a
meeting held at Green Bank to discuss seriously the number of
worlds capable of communicating with Earth. On this panel were
many well-known scientists, among them the man who had suddenly
ridiculed the original project as "folly" -- Dr. Otto Struve, Dr.
Melvin Calvin, Dr. John C. Lilly, Dr. Frank Drake, and Dr. Carl
Sagan.
It was concluded at this meeting that "There are between
40,000,000 and 50,000,000 worlds which are either trying to signal
us or are listening for messages from Earth." This statement has
become known as "The Green Bank Forumla."
Following this, control of listening projects was turned over
to the Air Force Office of Scientific Research in Puerto Rico.
Although the true story of Tau-Ceti may never be publicly known,
it is known that this was the birth of SETI.
As part of NASA's Exobiology Program, NASA SETI has been
ongoing since 1982 and is geared towards understanding the
origin, evolution and distribution of life in the Universe.
<Continued in next message..>
--
Michael Corbin - via ParaNet node 1:104/422
UUCP: !scicom!paranet!User_Name
INTERNET: Michael.Corbin@p0.f428.n104.z1.FIDONET.ORG
--------------------------------------------------------------------
From: Michael.Corbin@p0.f428.n104.z1.FIDONET.ORG (Michael Corbin)
Subject: SETI - Part 2
Date: 5 Oct 92 07:06:04 GMT
<..Continued from previous message>
What does it take to launch a program of this sort?
Through Stanford University, a compact and flexible
prototype Multi-Channel Spectrum Analyzer (MCSA 1.0) has been
designed and built. It provides 144 channels with 576-Hertz
spectral resolution and 74,000 channels at 1/2-Hertz resolution.
Present signal recognition software algorithms have demonstrated
efficient and near optimal detection of continuous wave (CW)
signals and narrowband pulses whether stationary or drifting up
to (+/-)1 channel/observational frame.
In testing, this system was able, in the Targeted Search
mode, to detect the one-Watt signal from the Pioneer 10
spacecraft transmitter beyond the solar system using MCSA 1.0 at
Goldstone. In the test of the Sky Survey mode, it was able to map
a portion of the sky at a frequency corresponding to one sideband
of the Voyager 2 transmitter and to detect that spacecraft more
than 3 billion kilometers from Earth on its way to Neptune.
The operational phase of the program will consist of two
modes: the Targeted Search and the Sky Survey. The Targeted
Search will examine 800 to 1000 nearby Sun-like stars for
evidence of continuous wave (CW) and narrowband pulsed signals
over the frequency range from 1 to 3 GHz (Gigahertz). The Sky
Survey will search the entire sky for CW signals over the
frequency range 1 to 10 GHz. The Targeted Search will have
significantly more sensitivity than the Sky Survey, whereas the
Sky Survey covers a larger area of the sky and a greater
frequency range.
Are the millions of dollars put toward this research
justified? Would this suggest that science is convinced that
life exists beyond our tiny little planet?
Consider the next two statements from the Astronomy Survey
Committee of the National Academy of Sciences in 1972 and 1982,
respectively:
"Our civilization is within reach of one of
the greatest steps in its evolution:
knowledge of the existence, nature, and
activities of independent civilizations in
space. At this instant, through this very
document, are perhaps passing radio waves
bearing the conversations of distant creatures
-- conversations that we could record if we
but pointed a telescope in the right direction
and tuned to the proper frequency...
Indeed there exist the know-how and
instruments to search for extraterrestrial
civilizations...Each passing year has seen our
estimates of the probability of life in space
increase, along with our capabilities for
detecting it. More and more scientists feel
that contact with other civilizations is no
longer something beyond our dreams but a
natural event in the history of mankind that
will perhaps occur in the lifetime of many of
us. The promise is now too great, either to
turn away from it or to wait much longer
before devoting major resources to a search
for other intelligent beings...
In the long run, this may be one of science's
most important and most profound contributions
to mankind and to our civilization."
"While the Committee recognized that this
endeavor has a character different from that
normally associated with astronomical
research, intelligent organisms are as much a
part of the universe as stars and galaxies;
investigating whether some of the
electromagnetic radiation now arriving at
Earth was generated by intelligent beings in
space may thus be considered a legitimate part
of astronomy. Moreover, the techniques that
can now be most effectively brought to bear on
a SETI program for the 1980's are those of
astronomy...
It is hard to imagine a more exciting
astronomical discovery or one that would have
greater impact on human perceptions than the
detection of extraterrestrial intelligence."
What if we do receive communication from extraterrestrial
intelligence? What if we receive that big "hello" from across
the galaxy? Do we answer?
SETI - to be distinguished from communication with
extraterrestrial intelligence (CETI), which implies actual two-
way formulation of a mutually understandable language for
discourse - has had at least nine searches since its beginning in
1960, with no reported success.
Dr. Arthur C. Clarke, a highly respected author and space-
travel authority, believes that a malevolent super-race might
transmit vicious, compelling information which could cause us to
destroy ourselves.
Perhaps one person responsible for the seriousness with
which scientists take the possibility of life in the universe was
Nobel Prize winner Sir Martin Ryle, who stated that no signals be
intentionally sent to other stars for fear of an invasion or a
loss of human values when contact is made with a superior
intelligence.
Despite these warnings, for over fifty years, radio,
television and radar emissions have been traveling away from
Earth at the speed of light, making our presence in the universe
known.
If it is found that life exists elsewhere in the Universe,
we could benefit tremendously from such a discovery. It could
revolutionize many aspects of earthly life.
Or, on the other hand, it could be devastating to us.
Dr. Carl Sagan once stated we should refrain from
transmitting "because we do not know the intentions of a superior
galactic society."
Recently NASA was awarded $40 million dollars for the Search
for Extraterrestrial Intelligence from 1993 to 1999.
<Concluded in next message..>
--
Michael Corbin - via ParaNet node 1:104/422
UUCP: !scicom!paranet!User_Name
INTERNET: Michael.Corbin@p0.f428.n104.z1.FIDONET.ORG
--------------------------------------------------------------------
From: Michael.Corbin@p0.f428.n104.z1.FIDONET.ORG (Michael Corbin)
Subject: SETI - Conclusion
Date: 5 Oct 92 07:07:05 GMT
<<..Continued from previous message>>
Through efforts of a host of agencies associated with the
NASA/SETI program a set of guidelines have been established which
will act as a global protocol for dealing with our neighbors.
Called the "Declaration of Principles Concerning Activities
Following the Detection of Extraterrestrial Intelligence," it
reads as follows:
We, the institutions and individuals participating in the
search for extraterrestrial intelligence,
Recognizing that the search for extraterrestrial
intelligence is an integral part of space exploration and
is being undertaken for peaceful purposes and for the
common interest of all mankind,
Inspired by the profound significance for mankind of
detecting evidence of extraterrestrial intelligence, even
though the probability of detection may be low,
Recalling the Treaty of Principles Governing the Activities
of States in the Exploration and Use of Outer Space,
Including the Moon and Other Celestial Bodies, which
commits States Parties to that Treaty "to inform the
Secretary General of the United Nations as well as the
public and the international scientific community, to the
greatest extent feasible and practicable, of the nature,
conduct, locations and results" of their space exploration
activities (Article XI),
Recognizing that any initial detection may be incomplete or
ambiguous and thus require careful examination as well as
confirmation, and that it is essential to maintain the
highest standards of scientific responsibility and
credibility,
Agree to observe the following principles for disseminating
information about the detection of extraterrestrial
intelligence:
1. Any individual, public or private research
institution, or governmental agency that believes it has
detected a signal from or other evidence of
extraterrestrial intelligence (the discoverer) should seek
to verify that the most plausible explanation for the
evidence is the existence of extraterrestrial intelligence
rather than some other natural phenomenon or anthropogenic
phenomenon before making any public announcement. If the
evidence cannot be confirmed as indicating the existence of
extraterrestrial intelligence, the discoverer may
disseminate the information as appropriate to the discovery
of any unknown phenomenon.
2. Prior to making a public announcement that evidence
if extraterrestrial intelligence has been detected, the
discoverer should promptly inform all other observers or
research organizations that are parties to this
declaration, so that those other parties may seek to
confirm the discovery by independent observations at other
sites and so that a network can be established to enable
continuous monitoring of the signal or phenomenon. Parties
to this declaration should not make any public
announcement of this information until it is determined
whether this information is or is not credible evidence of
the existence of extraterrestrial intelligence. The
discoverer should inform his/her or its relevant national
authorities.
3. After concluding that the discovery appears to be
credible evidence of extraterrestrial intelligence, and
after informing other parties to this declaration, the
discoverer should inform observers throughout the world
through the Central Bureau for Astronomical Telegrams of
the International Astronomical Union, and should inform the
Secretary General of the United Nations in accordance with
Article XI of the Treaty on Principles Governing the
Activities of States in the Exploration and Use of Outer
Space, Including the Moon and Other Bodies. Because of
their demonstrated interest in and expertise concerning the
question of the existence of extraterrestrial intelligence,
the discoverer should simultaneously inform the following
international institutions of the discovery and should
provide them with all pertinent data and recorded
information concerning the evidence: the International
Telecommunication Union, the Committee on Space Research of
the International Council of Scientific Unions, the
International Astronautical Federation, the International
Academy of Astronautics, the International Institute of
Space Law, Commission 51 of the International Astronomical
Union and Commission J of the International Radio Science
Union.
4. A confirmed detection of extraterrestrial
intelligence should be disseminated promptly, openly, and
widely through scientific channels and public media,
observing the procedures in this declaration. The
discoverer should have the privilege of making the first
public announcement.
5. All data necessary for confirmation of detection
should be made available to the international scientific
community through publications, meetings, conferences, and
other appropriate means.
6. The discovery should be confirmed and monitored and
any data bearing on the evidence of extraterrestrial
intelligence should be recorded and stored permanently to
the greatest extent feasible and practicable, in a form
that will make it available for further analysis and
interpretation. These recordings should be made available
to the international institutions listed above and to
members of the scientific community for further objective
analysis and interpretation.
7. If the evidence of detection is in the form of
electromagnetic signals, the parties to this declaration
should seek international agreement to protect the
appropriate frequencies by exercising the extraordinary
procedures established within the World Administrative
Radio Council of the International Telecommunication Union.
8. No response to a signal or other evidence of
extraterrestrial intelligence should be sent until
appropriate international consultations have taken place.
The procedures for such consultations will be the subject
of a separate agreement, declaration of arrangement.
9. The SETI Committee of the International Academy of
Astronautics, in coordination with Commission 51 of the
International Astronomical Union, will conduct a continuing
review of procedures for the detection of extraterrestrial
intelligence and the subsequent handling of the data.
Should credible evidence of extraterrestrial intelligence
be discovered, an international committee of scientists and
other experts should be established to serve as a focal
point for continuing analysis of all observational evidence
collected in the aftermath of the discovery, and also to
provide advice on the release of collected in the aftermath
of the discovery, and also to provide advice on the release
of information to the public. This committee should be
constituted from representatives of each of the
international institutions listed above and such other
members as the committee may deem necessary. To facilitate
the convocation of such a committee at some unknown time in
the future, the SETI Committee of the International Academy
of Astronautics should initiate and maintain a current list
of willing representatives from each of the international
institutions listed above, as well as other individuals
with relevant skills, and should make that list
continuously available through the Secretariat of the
International Academy of Astronautics. The International
Academy of Astronautics will act as the Depository for this
declaration and will annually provide a current list of
parties to all the parties to this declaration.
We, as a global society, must act responsibly in our
endeavors in this search for extraterrestrial intelligence.
This is only one small piece in the overall picture.
Perhaps in our lifetimes we will discover the truth to this
enigma concerning UFOs and the possible connection they have with
a government-funded search.
So, the next time you turn on your television or you use the
telephone, ponder this question -- "Is Anybody Out There?"
=================================================================
--
Michael Corbin - via ParaNet node 1:104/422
UUCP: !scicom!paranet!User_Name
INTERNET: Michael.Corbin@p0.f428.n104.z1.FIDONET.ORG
*******************************************************************************
Submissions infopara@scicom.alphacdc.com
Administrative requests infopara-request@scicom.alphacdc.com
FTP archive grind.isca.uiowa.edu:/info/paranet/infopara
Permission to distribute Michael.Corbin@paranet.org
Private mail to Paranet/Fidonet users firstname.lastname@paranet.org
UUCP gateway {ncar,isis,csn}!scicom
*********************End**of**the**InfoPara**Newsletter************************
