SUBJECT: SETI OPTICAL SEARCH BEST ?                          FILE: UFO1003

PART 3

                              SETI 3

       Philosopher Clive Goodall will rebut Frank Tipler's arguments, and
   Noted philosopher Professor Neil Tennant will present his view of why
   there could be major problems in actually decoding the message on an ETI
   signal.  This may be the first time that philosophers have presented
   papers at a "technical" meeting on SETI, particularly one organized by
   SPIE.  Dr. Guillermo Lemarchand will describe both radio and optical
   SETI activities in Argentina and give an account of the MANIA optical
   SETI project devised by the late Professor Shvartsman of the former
   Soviet Union.  Drs. John Rather and Monte Ross (conference co-chairman)
   will give accounts of their approaches to interstellar laser communi-
   cations, while this author will present a review paper and describe the
   amateur approach to optical SETI.  There will be a discussion at the end
   of the conference, moderated by Charles Townes, who earlier will talk
   about his CO2 optical SETI laser work, and the CO2 OSETI observations
   being conducted by Dr. Albert Betz on Mount Wilson.

       Note that as with previous SETI publications, the latest book by
   SETI pioneer Professor Frank Drake and Dava Sobel IS ANYONE OUT THERE?
   hardly mentions the optical approach.  This conference intends to
   redress that omission.  This "controversial" OSETI conference should be
   a "fun" event but you do not need to be a laser communications engineer
   or SETI scientist to attend - you only need a curiosity about "our"
   place in the grand scheme of things.

       With large telescopes, Optical SETI is the one branch of visible
   astronomy, save for solar astronomy, that can be done during the day
   under a clear blue sky!

       Last October, we saw the celebration of the Quincentennial of
   Christopher Columbus's voyage to the Americas and the official start
   of NASA's Microwave Observing Project (MOP), recently renamed the High
   Resolution Microwave Survey (HRMS).  Numerous articles on SETI have
   appeared in recent magazine publications, including the September 1992
   issue of LIFE, the October issue of ASTRONOMY, and the November/December
   issue of SMITHSONIAN AIR & SPACE.  See also recent issues of TIME and
   NEWSWEEK.  The November issue of SKY & TELESCOPE has a long article
   about microwave SETI and mentions the optical approach.  This is
   probably the first published popular account of modern OSETI in the
   printed media.  See the bibliography at the end of this article.

       I have also begun the construction of what I believe to be the
   world's first amateur optical SETI (AMOSETI) Observatory.  This will be
   based around the Meade 10-inch LX200 Schmidt-Cassegrain telescope, and i
   one of the most advanced on the market today for use under computer and
   CCD control.  In the last paper of the conference, I will be reporting
   on the amateur approach to Optical SETI and any work done to date on my
   observatory system.  In many respects, the approach adopted by the
   author for AMOSETI is similar to that employed by Shvartsman and Beskin
   in the MANIA project, i.e., looking for very short pulses rather than CW
   beacon signals.   It is possible that AMOSETI will lead to a renaissance
   in amateur astronomy, where light pollution - the bane of astronomers -
   has no effect on ETI detection sensitivity!

       At this time during the sharp decline in the industrial-military
   complex, can there be a more ennobling way for defense conversion - to
   turn laser swords into SETI or CETI plowshares and help discover that we
   are not alone within the Milky Way galaxy?  Monte and I look forward to
   seeing you at this conference at the rebirth of a new branch of science.


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