The search for extraterrestrial intelligence, SETI
Philip Morrison (editor)
The search for extraterrestrial intelligence, SETI
Free
Description
Contents
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Over the past two decades there has developed an increasingly serious debate about the existence of extraterrestrial intelligent life. More recently, there have been significant deliberations about ways in which extraterrestrial intelligence might in fact be detected. In the past two years, a series of Science Workshops has examined both questions in more detail. The Workshop activities were part of a feasibility study on the Search for Extraterrestrial Intelligence (SETI) conducted by the NASA Arnes Research Center.

The objectives of the Science Workshops, as agreed at the second meeting in April 1975, were: to examine systematically the validity of the fundamental criteria and axioms associated with a program to detect extraterrestrial intelligent life; to identify areas of research in the astronomical sciences, and in other fields, that would improve the confidence levels of current probability estimates relevant to SETI; to enumerate the reasons for undertaking a search, the values and risks of success, and the consequences of failure; to explore alternative methods of conducting a search; to select, in a systematic way, preferred approaches; to indicate the conceptual design of a minimum useful system as required t o implement the preferred approaches; to delineate the new opportunities for astronomical research provided by the system and their implications for system design; to outline the scale and timing of the search and the resources required to carry it out; to examine the impact of conducting a search, and the impact of success or failure in terms of national, international, social and environmental considerations; and to recommend a course of action, including specific near-term activities.

This report presents the findings of the series of Workshops. The major conclusions of our deliberations are presented in Section I. First, an Introduction lays out the background and rationale for a SETI program, and then in The Impact of SETI, we examine the implications of the program. In particular, the Impact section examines the significance of the detection of signals and of information that may be contained in signals from extraterrestrial civilizations.

Language
English
ISBN
Unknown
Annotated Star Field
View of Arecibo Observatory in Puerto Rico
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Foreword
Workshop Members
Preface
CONSENSUS
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Frequency scan of a [alpha]-Ophinchi
Alternative Methods of Communication
The Rationale for a Preferred Frequency Band: The Water Hole
Figure 1
Figure 2
Figure 3
Figure 4
Radio Frequency Interference
A Preliminary Parametric Analysis of Search Systems
Concept of 300-m space SETI system
SETI Related Scientific and Technological Advances
The Science of SETI
Cosmic Evolution
Detection of Other Planetary Systems
The Orion Nebula
Workshop Members, Biographical Information
Selected Annotated Bibliography
The Maintenance of Archives
Searches to Date
The Soviet CETI Report
Responses to a Questionnaire Sent to Leading Radio Observatories
Protection of a Preferred Radio Frequency Band
Cultural Evolution
Search Strategies
Table 1
Arecibo search for ETI in M33
Notes on Search Space
Table 2
Table 3
Parametric Relations in a Whole Sky Search
Antennas at NASA Mohave R & D site
Stellar Census
Summary of Possible Uses of an Interstellar Search System for Radio Astronomy
Chart 1
Westerbork synthesis map of M51
Back
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