COSTS and DIFFICULTIES of METI
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Interstellar Communication: the Case for Spread Spectrum
Interstellar Communication: The Case for Spread Spectrum David G Messerschmitta aDepartment of Electrical Engineering and Computer Sciences, 253 Cory Hall, University of California, Berkeley, California 94720-1770, USA, [email protected], 1-925-465-5740 Abstract Spread spectrum, widely employed in modern digital wireless terrestrial radio systems, chooses a signal with a noise-like character and much higher bandwidth than necessary. This paper advocates spread spectrum modulation for interstellar communication, motivated by robust immunity to radio- frequency interference (RFI) of technological origin in the vicinity of the receiver while preserving full detection sensitivity in the presence of natural sources of noise. Receiver design for noise immunity alone provides no basis for choosing a signal with any specific character, therefore failing to reduce ambiguity. By adding RFI to noise immunity as a design objective, the conjunction of choice of signal (by the transmitter) together with optimum detection for noise immunity (in the receiver) leads through simple probabilistic argument to the conclusion that the signal should possess the statistical properties of a burst of white noise, and also have a large time-bandwidth product. Thus spread spectrum also provides an implicit coordination between transmitter and receiver by reducing the ambiguity as to the signal character. This strategy requires the receiver to guess the specific noise-like signal, and it is contended that this is feasible if an appropriate pseudorandom signal is generated algorithmically. For example, conceptually simple algorithms like the binary expansion of common irrational numbers like π are shown to be suitable. Due to its deliberately wider bandwidth, spread spectrum is more susceptible to dispersion and distortion in propagation through the interstellar medium, desirably reducing ambiguity in parameters like bandwidth and carrier frequency. -
The Search for Extraterrestrial Intelligence
THE SEARCH FOR EXTRATERRESTRIAL INTELLIGENCE Are we alone in the universe? Is the search for extraterrestrial intelligence a waste of resources or a genuine contribution to scientific research? And how should we communicate with other life-forms if we make contact? The search for extraterrestrial intelligence (SETI) has been given fresh impetus in recent years following developments in space science which go beyond speculation. The evidence that many stars are accompanied by planets; the detection of organic material in the circumstellar disks of which planets are created; and claims regarding microfossils on Martian meteorites have all led to many new empirical searches. Against the background of these dramatic new developments in science, The Search for Extraterrestrial Intelligence: a philosophical inquiry critically evaluates claims concerning the status of SETI as a genuine scientific research programme and examines the attempts to establish contact with other intelligent life-forms of the past thirty years. David Lamb also assesses competing theories on the origin of life on Earth, discoveries of ex-solar planets and proposals for space colonies as well as the technical and ethical issues bound up with them. Most importantly, he considers the benefits and drawbacks of communication with new life-forms: how we should communicate and whether we could. The Search for Extraterrestrial Intelligence is an important contribution to a field which until now has not been critically examined by philosophers. David Lamb argues that current searches should continue and that space exploration and SETI are essential aspects of the transformative nature of science. David Lamb is honorary Reader in Philosophy and Bioethics at the University of Birmingham. -
Project Cyclops : a Design Study of a System for Detecting
^^^^m•i.j . --f'v.i^ "^y^-!^ A Design Study of a System for Detecting Extraterrestrial Intelligent Life '• >..-, i,C%' PREPARED UNDER STANFORD /NASA /AMES RESEARCH CENTER >J^1t> 1971 SUMMER FACULTY FELLOWSHIP PROGRAM IN ENGINEERING SYSTEMS DESIGr CR 114445 (Revised Edition 7/73) Available to the public rB' ^ A Design Study of a System for Detecting Extraterrestrial Intelligent Life PREPARED UNDER STANFORD/ NASA/AMES RESEARCH CENTER 1971 SUMMER FACULTY FELLOWSHIP PROGRAM IN ENGINEERING SYSTEMS DESIGN Further copies of this report may be obtained by writing to Dr. John Billingham NASA/ Ames Research Center, Code LT Moffett Field, California 94035 weixesunr colligc LWRART CYCLOPS PEOPLE Co-Directors: Bernard M. Oliver Stanford University (Summer appointment) John Billingham Ames Research Center, NASA System Design and Advisory Group: James Adams Stanford University Edwin L. Duckworth San Francisco City College Charles L. Seeger New Mexico State University George Swenson University of Illinois Antenna Structures Group: Lawrence S. Hill California State College L.A. John Minor New Mexico State University Ronald L. Sack University of Idaho Harvey B. Sharfstein San Jose State College Pennsylvania Alan 1. Soler University of Receiver Group: Washington Ward J. Helms University of William Hord Southern Illinois University Pierce Johnson University of Missouri C. ReedPredmore Rice University Transmission and Control Group: Marvin Siegel Michigan State University Jon A. Soper Michigan Technological University Henry J. Stalzer, Jr. Cooper Union Signal Processing Group: Jonnie B. Bednar University of Tulsa Douglas B. Brumm Michigan Technological University James H. Cook Cleveland State University Robert S. Dixon Ohio State University Johnson Luh Purdue University Francis Yu Wayne State University /./ la J C, /o ) •»• < . -
Searching for Extraterrestrial Intelligence
THE FRONTIERS COLLEctION THE FRONTIERS COLLEctION Series Editors: A.C. Elitzur L. Mersini-Houghton M. Schlosshauer M.P. Silverman J. Tuszynski R. Vaas H.D. Zeh The books in this collection are devoted to challenging and open problems at the forefront of modern science, including related philosophical debates. In contrast to typical research monographs, however, they strive to present their topics in a manner accessible also to scientifically literate non-specialists wishing to gain insight into the deeper implications and fascinating questions involved. Taken as a whole, the series reflects the need for a fundamental and interdisciplinary approach to modern science. Furthermore, it is intended to encourage active scientists in all areas to ponder over important and perhaps controversial issues beyond their own speciality. Extending from quantum physics and relativity to entropy, consciousness and complex systems – the Frontiers Collection will inspire readers to push back the frontiers of their own knowledge. Other Recent Titles Weak Links Stabilizers of Complex Systems from Proteins to Social Networks By P. Csermely The Biological Evolution of Religious Mind and Behaviour Edited by E. Voland and W. Schiefenhövel Particle Metaphysics A Critical Account of Subatomic Reality By B. Falkenburg The Physical Basis of the Direction of Time By H.D. Zeh Mindful Universe Quantum Mechanics and the Participating Observer By H. Stapp Decoherence and the Quantum-To-Classical Transition By M. Schlosshauer The Nonlinear Universe Chaos, Emergence, Life By A. Scott Symmetry Rules How Science and Nature are Founded on Symmetry By J. Rosen Quantum Superposition Counterintuitive Consequences of Coherence, Entanglement, and Interference By M.P. -
Interstellar Communication. Iii. Optimal Frequency to Maximize Data Rate
Draft version November 17, 2017 INTERSTELLAR COMMUNICATION. III. OPTIMAL FREQUENCY TO MAXIMIZE DATA RATE Michael Hippke1 and Duncan H. Forgan2, 3 1Sonneberg Observatory, Sternwartestr. 32, 96515 Sonneberg, Germany 2SUPA, School of Physics & Astronomy, University of St Andrews, North Haugh, St Andrews, Scotland, KY16 9SS, UK 3St Andrews Centre for Exoplanet Science, University of St Andrews, UK ABSTRACT The optimal frequency for interstellar communication, using \Earth 2017" technology, was derived in papers I and II of this series (Hippke 2017a,b). The framework included models for the loss of photons from diffraction (free space), interstellar extinction, and atmospheric transmission. A major limit of current technology is the focusing of wavelengths λ < 300 nm (UV). When this technological constraint is dropped, a physical bound is found at λ ≈ 1 nm (E ≈ keV) for distances out to kpc. While shorter wavelengths may produce tighter beams and thus higher data rates, the physical limit comes from surface roughness of focusing devices at the atomic level. This limit can be surpassed by beam-forming with electromagnetic fields, e.g. using a free electron laser, but such methods are not energetically competitive. Current lasers are not yet cost efficient at nm wavelengths, with a gap of two orders of magnitude, but future technological progress may converge on the physical optimum. We recommend expanding SETI efforts towards targeted (at us) monochromatic (or narrow band) X-ray emission at 0.5-2 keV energies. 1. INTRODUCTION believed to originate from intelligent beings on Mars. The idea to communicate with Extraterrestrial Intel- In the optical, William Pickering(1909) suggested to ligence was born in the 19th century. -
Radio Astronomy
Edition of 2013 HANDBOOK ON RADIO ASTRONOMY International Telecommunication Union Sales and Marketing Division Place des Nations *38650* CH-1211 Geneva 20 Switzerland Fax: +41 22 730 5194 Printed in Switzerland Tel.: +41 22 730 6141 Geneva, 2013 E-mail: [email protected] ISBN: 978-92-61-14481-4 Edition of 2013 Web: www.itu.int/publications Photo credit: ATCA David Smyth HANDBOOK ON RADIO ASTRONOMY Radiocommunication Bureau Handbook on Radio Astronomy Third Edition EDITION OF 2013 RADIOCOMMUNICATION BUREAU Cover photo: Six identical 22-m antennas make up CSIRO's Australia Telescope Compact Array, an earth-rotation synthesis telescope located at the Paul Wild Observatory. Credit: David Smyth. ITU 2013 All rights reserved. No part of this publication may be reproduced, by any means whatsoever, without the prior written permission of ITU. - iii - Introduction to the third edition by the Chairman of ITU-R Working Party 7D (Radio Astronomy) It is an honour and privilege to present the third edition of the Handbook – Radio Astronomy, and I do so with great pleasure. The Handbook is not intended as a source book on radio astronomy, but is concerned principally with those aspects of radio astronomy that are relevant to frequency coordination, that is, the management of radio spectrum usage in order to minimize interference between radiocommunication services. Radio astronomy does not involve the transmission of radiowaves in the frequency bands allocated for its operation, and cannot cause harmful interference to other services. On the other hand, the received cosmic signals are usually extremely weak, and transmissions of other services can interfere with such signals. -
Nasa and the Search for Technosignatures
NASA AND THE SEARCH FOR TECHNOSIGNATURES A Report from the NASA Technosignatures Workshop NOVEMBER 28, 2018 NASA TECHNOSIGNATURES WORKSHOP REPORT CONTENTS 1 INTRODUCTION .................................................................................................................................................................... 1 What are Technosignatures? .................................................................................................................................... 2 What Are Good Technosignatures to Look For? ....................................................................................................... 2 Maturity of the Field ................................................................................................................................................... 5 Breadth of the Field ................................................................................................................................................... 5 Limitations of This Document .................................................................................................................................... 6 Authors of This Document ......................................................................................................................................... 6 2 EXISTING UPPER LIMITS ON TECHNOSIGNATURES ....................................................................................................... 9 Limits and the Limitations of Limits ........................................................................................................................... -
The Origins and Development of the Search for Extraterrestrial Intelligence, 1959-1971 Sierra E
James Madison University JMU Scholarly Commons Masters Theses The Graduate School Spring 2012 "A cosmic Rorschach test": The origins and development of the search for extraterrestrial intelligence, 1959-1971 Sierra E. Smith James Madison University Follow this and additional works at: https://commons.lib.jmu.edu/master201019 Part of the History Commons Recommended Citation Smith, Sierra E., ""A cosmic Rorschach test": The origins and development of the search for extraterrestrial intelligence, 1959-1971" (2012). Masters Theses. 334. https://commons.lib.jmu.edu/master201019/334 This Thesis is brought to you for free and open access by the The Graduate School at JMU Scholarly Commons. It has been accepted for inclusion in Masters Theses by an authorized administrator of JMU Scholarly Commons. For more information, please contact [email protected]. “A Cosmic Rorschach Test”: The Origins and Development of the Search for Extraterrestrial Intelligence, 1959-1971 Sierra E. Smith A thesis submitted to the Graduate Faculty of JAMES MADISON UNIVERSITY In Partial Fulfillment of the Requirements for the degree of Master of Arts History May 2012 Acknowledgements First and foremost, I would like to thank my thesis committee who has gone above and beyond the call of duty to guide me through this process. Despite being dragged into the twentieth century, Dr. Alison Sandman, my thesis director, helped articulate the ideas for my project far better than I could have alone. Thought-provoking conversations with Dr. Kevin Borg ensured that I thought broadly and deeply about both my project and my future plans. Dr. Steven Guerrier’s open door and enthusiasm for my project has been a constant throughout my graduate experience. -
Search for Extraterrestrial Intelligence (SETI) - the Next Steps (34Th Symposium) (IAA.1.1) (A4.) SETI I - Technical Aspects (1.)
56th International Astronautical Congress 2005 Search for Extraterrestrial Intelligence (SETI) - The Next Steps (34th Symposium) (IAA.1.1) (A4.) SETI I - Technical Aspects (1.) Author Dr. Douglas A. Vakoch The SETI Institute, United States, [email protected] ADVANTAGES OF ACTIVE SETI Abstract This paper will examine the potential benefits of Active SETI, a prospect raised in the Project Cyclops report, which noted “if our first search of the nearest 1000 target stars produced negative results we might wish to transmit beacons to these stars for a year or more before carrying the search deeper into space” (p. 153). Renewed discussion of that possibility is particularly timely in light of the recent completion of Project Phoenix, which surveyed nearly 1000 nearby stars. It has often been argued that the young age of human civilization, when compared to the older age of any extraterrestrial civilization we may contact, justifies our reliance on passive SETI as opposed to transmitting. Because transmission is more costly and requires longer timescales to succeed, the argument goes, we should be expected to take the easier role. However, this reasoning presupposes that the motivations of extraterrestrial civilizations are sufficiently benevolent that they will transmit de novo rather than only in reciprocation, and that they choose to make contact even prior to learning that we desire contact. This paper examines an alternative scenario, in which entry into the Galactic Club requires initiative on the part of the applicant, rather than passively waiting for an invitation. It proposes a solution to the troubling possibility that many civilizations are listening but none is transmitting. -
Searching for SETI: the Social Construction of Aliens and the Quest for a Technological Mythos
Searching for SETI: The Social Construction of Aliens and the Quest for a Technological Mythos John Marvin Bozeman Dissertation submitted to the faculty of the Virginia Polytechnic Institute and State University in partial fulfillment of the requirements for the degree of Doctor of Philosophy In Science and Technology Studies Janet A. Abbate, Co-Chair Shannon A. Brown, Co-Chair Lee L. Zwanziger Paul D. Renard March 24, 2015 Falls Church, Virginia Keywords: Search for Extraterrestrial Intelligence, SETI, Actor Network Theory, Social Construction of Technology, Rational Choice Theory of Religion, Transhumanism, Xenosalvation Copyright John M. Bozeman Searching for SETI: The Social Construction of Aliens and the Quest for a Technological Mythos John M. Bozeman ABSTRACT This dissertation uses Actor Network Theory (ANT) and Stark and Bainbridge’s rational choice theory of religion to analyze an established but controversial branch of science and technology, the Search for Extraterrestrial Intelligence (SETI). Of particular interest are the cultural, and sometimes religious, assumptions that its creators have built into it. The purpose of this analysis is not to discredit SETI, but instead to show how SETI, along with other avant-garde scientific projects, is founded, motivated, and propelled by many of the same types of values and visions for the future that motivate the founders of religious groups. I further argue that the utopian zeal found in SETI and similar movements is not aberrant, but instead common, and perhaps necessary, in many early- stage projects, whether technical or spiritual, which lack a clear near-term commercial or social benefit. DEDICATION In memory of my parents, James E. -
The Breakthrough Listen Search for Intelligent Life: 1.1–1.9 Ghz Observations of 692 Nearby Stars
The Astrophysical Journal, 849:104 (13pp), 2017 November 10 https://doi.org/10.3847/1538-4357/aa8d1b © 2017. The American Astronomical Society. All rights reserved. The Breakthrough Listen Search for Intelligent Life: 1.1–1.9 GHz Observations of 692 Nearby Stars J. Emilio Enriquez1,2 , Andrew Siemion1,2,3 , Griffin Foster1,4 , Vishal Gajjar5 , Greg Hellbourg1, Jack Hickish6 , Howard Isaacson1 , Danny C. Price1,7 , Steve Croft1 , David DeBoer6, Matt Lebofsky1, David H. E. MacMahon6, and Dan Werthimer1,5,6 1 Department of Astronomy, University of California, Berkeley, 501 Campbell Hall #3411, Berkeley, CA, 94720, USA; [email protected] 2 Department of Astrophysics/IMAPP, Radboud University, P.O. Box 9010, NL-6500 GL Nijmegen, The Netherlands 3 SETI Institute, Mountain View, CA 94043, USA 4 University of Oxford, Sub-Department of Astrophysics, Denys Wilkinson Building, Keble Road, Oxford, OX1 3RH, UK 5 Space Science Laboratory, 7-Gauss way, University of California, Berkeley, CA, 94720, USA 6 Radio Astronomy Laboratory, University of California at Berkeley, Berkeley, CA 94720, USA 7 Centre for Astrophysics & Supercomputing, Swinburne University of Technology, PO Box 218, Hawthorn, VIC 3122, Australia Received 2017 April 20; revised 2017 September 5; accepted 2017 September 8; published 2017 November 6 Abstract We report on a search for engineered signals from a sample of 692 nearby stars using the Robert C. Byrd Green Bank Telescope, undertaken as part of the Breakthrough Listen Initiative search for extraterrestrial intelligence. Observations were made over 1.1–1.9 GHz (L band), with three sets of five-minute observations of the 692 primary targets, interspersed with five-minute observations of secondary targets. -
Communication with Extraterrestrial Intelligence Through Radio Signals and Messages 1A
ISSN : 2230-7109 (Online) | ISSN : 2230-9543 (Print) IJECT VOL . 5, ISSU E SPL - 2, JAN - MAR C H 2014 Communication with Extraterrestrial Intelligence Through Radio Signals and Messages 1A. B. Bhattacharya, 2A. Sarkar 1,2Dept. of Physics, University of Kalyani, Kalyani, WB, India Abstract hundred yards wide could delineate twenty-mile wide shapes and The paper summarizes the present day research knowledge based then the trenches would be filled with water after which enough on communication with extraterrestrial intelligence through four kerosene could be poured on top of the water to burn for six hours. distinct means covering mathematical languages, pictorial systems Using this technique, a different signal could be sent every night. like the Arecibo message, algorithmic communication systems and In the mean time other astronomers were looking for signs of life computational approaches for detecting and deciphering ‘natural’ on other planets. In 1822, Franz von Gruithuisen [Cattermole and language communication. Moore, 1997] imagined a giant city and evidence of agriculture on the moon and believed evidence of life on Venus but astronomers Keywords using more sophisticated instruments refuted his claims. By the Arecibo Message, Communication, Extraterrestrial Intelligence, late 1800s, Astronomers believed the Kant-Laplace hypothesis, Resonant Receiver which stated that the farthest planets from the sun are the oldest and so Mars was more likely to have advanced civilizations than I. Introduction Venus. Subsequent investigations focused on contacting Martians. Communication with Extraterrestrial Intelligence (CETI) is Charles Cros [Ley, 1958] was convinced that pinpoints of light a subject matter under the SETI (Search for Extraterrestrial observed on Mars and Venus were the lights of large cities and Intelligence) research which focuses on composing and was attempted to get funding for a giant mirror with which to deciphering messages that could be understood theoretically signal the Martians.