What Happens When We Detect Alien Life?
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Defenses That Hurt Science ______By Avi Loeb on June 4, 2021
Defenses That Hurt Science _______ By Avi Loeb on June 4, 2021 In the highlighted subtitle of a recent New-York Times Op-Ed, Bret Stephens stated: "Sometimes science is hurt most by those who think they are defending it". This sentiment resonates with many examples that go beyond the topic of his Op-Ed. Let me elaborate. When the nitrogen iceberg model was proposed recently to explain the weird properties of the first interstellar object `Oumuamua, it was immediately embraced by mainstream astronomers with a sigh of relief that the anomalous object was finally explained. We had never seen a chunk of frozen nitrogen floating within the Solar system before, and being detected first - `Oumuamua should represent the most common type of objects ejected by other planetary systems; but this was of little concern for the advocates. Shortly afterwards, my student Amir Siraj and I posted a paper showing that this model requires much more raw material of heavy elements than available in stars within the Milky Way galaxy. This was not a reflection on the previously noted abundance problem for interstellar objects, but a specific deficiency of the nitrogen model - which associates `Oumuamua with a fragment chipped off the surface of a Pluto-like planet around another star. The limited supply of nitrogen on exo-Pluto surfaces and the requirement that the interstellar journey would last just half a billion years - or else most of the nitrogen would evaporate, leads to a mass budget problem. But why should the mainstream worry about a fundamental drawback when the agenda is to sideline the weirdness of `Oumuamua? In another recent Op-Ed, Seth Shostak from the SETI Institute downgraded the scientific credentials of the anticipated report on Unidentified Flying Objects (UFOs), to be delivered by the Pentagon and various intelligence agencies to Congress this month. -
SETI SETI Stands for Search for Extraterrestrial Intelligence, and Usually Is Meant As an Acronym for Searches for Radio Commu
SETI SETI stands for Search for Extraterrestrial Intelligence, and usually is meant as an acronym for searches for radio commu- nications from extraterrestrials which has been its backbone. It began with a seminal paper in 1959 by Giuseppe Cocconi and Philip Morrison in Nature suggesting that the best way to find extraterrestrial civilizations was to search in the radio near 1420 MHz (H spin-flip). The first SETI, project Ozma (1960, Frank Drake, originator of the Drake equation) used the 85- foot Green Bank, WV telescope; today SETI@home uses the 1000-foot Arecibo radio telescope in Puerto Rico. The Plane- tary Society has played an important role in supporting SETI, ever since the ban on Federal funding for it in 1982-83 and from 1992 to the present. Other projects have included Suit- case SETI, META, BETA, SERENDIP and META II. Thinking about SETI took a new turn in 1967 when Joce- lyn Bell and her advisor, Anthony Hewish, discovered pulsars, which they initially referred to, jokingly, as LGM (little green men). Another pioneer of SETI was Bernard Oliver, Vice Pres- ident of Hewlett Packard, who suggested in 1971 the cosmic waterhole hypothesis and emphasized the relative \quietness" of the radio spectrum between 1 and 1000 GHz. Project Ozma operated for about 3 months, devoting about 200 hours of observation to its two targets Tau Ceti and Epsilon Eridani. It scanned 7200 channels each with a bandwidth of 100 Hz, centered on 1420 MHz. By looking at adjacent frequencies, Doppler shifts caused by relative motions of our planets and Suns would be incorporated. -
The Radio Search for Technosignatures in the Decade 2020–2030
Astro2020 Science White Paper The radio search for technosignatures in the decade 2020–2030 Background photo: central region of the Galaxy by Yuri Beletsky, Carnegie Las Campanas Observatory Thematic Area: Planetary Systems Principal Author: Name: Jean-Luc Margot Institution: University of California, Los Angeles Email: [email protected] Phone: 310.206.8345 Co-authors: Steve Croft (University of California, Berkeley), T. Joseph W. Lazio (Jet Propulsion Laboratory), Jill Tarter (SETI Institute), Eric J. Korpela (University of California, Berkeley) March 11, 2019 1 Scientific context Are we alone in the universe? This question is one of the most profound scientific questions of our time. All life on Earth is related to a common ancestor, and the discovery of other forms of life will revolutionize our understanding of living systems. On a more philosophical level, it will transform our perception of humanity’s place in the cosmos. Observations with the NASA Kepler telescope have shown that there are billions of habitable worlds in our Galaxy [e.g., Borucki, 2016]. The profusion of planets, coupled with the abundance of life’s building blocks in the universe, suggests that life itself may be abundant. Currently, the two primary strategies for the search for life in the universe are (1) searching for biosignatures in the Solar System or around nearby stars and (2) searching for technosignatures emitted from sources in the Galaxy and beyond [e.g., National Academies of Sciences, Engineer- ing, and Medicine, 2018]. Given our present knowledge of astrobiology, there is no compelling reason to believe that one strategy is more likely to succeed than the other. -
Dr. Seth Shostak
Written Text for Congressional Testimony Advances in the Search for Life Seth Shostak, Senior Astronomer, SETI Institute 189 Bernardo Ave., #200, Mountain View, CA 94043, [email protected] It is no longer considered foolish to argue that biology could exist on some of the trillion other planets in our galaxy. Its discovery would produce a lasting change in our perceptions, demonstrating that life is not confined to our world. We would know that biology is not some sort of miracle, but a commonplace – an ubiquitous, cosmic infection. The discovery of intelligence elsewhere would be of even greater import, as we have always considered humans to be special, even the pinnacle of Creation. To learn that there are others out there – others whose cognitive abilities exceed our own – would be a discovery that would recalibrate how our species views itself. It would also have consequences that can be only vaguely gauged, in much the way that the discovery of the New World led to societal changes that were largely unpredictable at the time of its happening. However, the search for extraterrestrial intelligence, known by the acronym SETI, has been pursued for more than a half century with no unambiguous, positive result. We haven’t found conclusive proof of any intelligent (or even unintelligent) life beyond the confines of Earth. Claims that our planet is being visited by alien beings, while popular with the citizenry, are not considered credible by most scientists. However, recent developments in both astronomy and technology are accelerating the speed of SETI searches, and it is hardly fantastic to suggest that we could find evidence of cosmic company within a few decades. -
Biosignatures Search in Habitable Planets
galaxies Review Biosignatures Search in Habitable Planets Riccardo Claudi 1,* and Eleonora Alei 1,2 1 INAF-Astronomical Observatory of Padova, Vicolo Osservatorio, 5, 35122 Padova, Italy 2 Physics and Astronomy Department, Padova University, 35131 Padova, Italy * Correspondence: [email protected] Received: 2 August 2019; Accepted: 25 September 2019; Published: 29 September 2019 Abstract: The search for life has had a new enthusiastic restart in the last two decades thanks to the large number of new worlds discovered. The about 4100 exoplanets found so far, show a large diversity of planets, from hot giants to rocky planets orbiting small and cold stars. Most of them are very different from those of the Solar System and one of the striking case is that of the super-Earths, rocky planets with masses ranging between 1 and 10 M⊕ with dimensions up to twice those of Earth. In the right environment, these planets could be the cradle of alien life that could modify the chemical composition of their atmospheres. So, the search for life signatures requires as the first step the knowledge of planet atmospheres, the main objective of future exoplanetary space explorations. Indeed, the quest for the determination of the chemical composition of those planetary atmospheres rises also more general interest than that given by the mere directory of the atmospheric compounds. It opens out to the more general speculation on what such detection might tell us about the presence of life on those planets. As, for now, we have only one example of life in the universe, we are bound to study terrestrial organisms to assess possibilities of life on other planets and guide our search for possible extinct or extant life on other planetary bodies. -
Edited by Steven J. Dick and Mark L. Lupisella
Edited by Steven J. Dick and Mark L. Lupisella NASA SP-2009-4802 Library of Congress Cataloging-in-Publication Data Cosmos and Culture : Cultural Evolution in a Cosmic Context / Steven J. Dick and Mark Lupisella, editors. p. cm. -- (NASA SP ; 4802) Includes bibliographical references and index. 1. Cosmology--History. 2. Astronomy--History. 3. Culture--Origin. 4. Social evolution. 5. Human evolution. I. Dick, Steven J. II. Lupisella, Mark. QB981.C8263 2009 523.109--dc22 2009004348 ISBN 978-0-16-083119-5 For sale by the Superintendent of Documents, U.S. Government Printing Office Internet: bookstore.gpo.gov Phone: toll free (866) 512-1800; DC area (202) 512-1800 9 0 0 0 0 Fax: (202) 512-2104 Mail: Stop IDCC, Washington, DC 20402-0001 ISBN 978-0-16-083119-5 9 780160 831195 ISBN 978-0-16-083119-5 For sale by the Superintendent of Documents, U.S. Government Printing Office Internet: bookstore.gpo.gov Phone: toll free (866) 512-1800; DC area (202) 512-1800 9 0 0 0 0 Fax: (202) 512-2104 Mail: Stop IDCC, Washington, DC 20402-0001 ISBN 978-0-16-083119-5 9 780160 831195 Table of Contents Introduction – Steven J. Dick and Mark L. Lupisella v Part 1: The Cosmic Context Chapter 1 – Eric J. Chaisson Cosmic Evolution State of the Science 3 Chapter 2 – Steven J. Dick Cosmic Evolution History, Culture, and Human Destiny 25 Part 2: Cultural Evolution Chapter 3 – Kathryn Denning Social Evolution State of the Field 63 Chapter 4 – Daniel C. Dennett The Evolution of Culture 125 Chapter 5 – Howard Bloom The Big Burp and the Multiplanetary Mandate 145 Chapter 6 – John M. -
Astronomy Beat
ASTRONOMY BEAT ASTRONOMY BEAT /VNCFSt"QSJM XXXBTUSPTPDJFUZPSH 1VCMJTIFS"TUSPOPNJDBM4PDJFUZPGUIF1BDJöD &EJUPS"OESFX'SBLOPJ ª "TUSPOPNJDBM 4PDJFUZ PG UIF 1BDJöD %FTJHOFS-FTMJF1SPVEöU "TIUPO"WFOVF 4BO'SBODJTDP $" The Origin of the Drake Equation Frank Drake Dava Sobel Editor’s Introduction Most beginning classes in astronomy introduce their students to the Drake Equation, a way of summarizing our knowledge about the chances that there is intelli- ASTRONOMYgent life among the stars with which we humans might BEAT communicate. But how and why did this summary for- mula get put together? In this adaptation from a book he wrote some years ago with acclaimed science writer Dava Sobel, astronomer and former ASP President Frank Drake tells us the story behind one of the most famous teaching aids in astronomy. ore than a year a!er I was done with Proj- 'SBOL%SBLFXJUIUIF%SBLF&RVBUJPO 4FUI4IPTUBL 4&5**OTUJUVUF ect Ozma, the "rst experiment to search for radio signals from extraterrestrial civiliza- Mtions, I got a call one summer day in 1961 from a man to be invited. I had never met. His name was J. Peter Pearman, and Right then, having only just met over the telephone, we he was a sta# o$cer on the Space Science Board of the immediately began planning the date and other details. National Academy of Science… He’d followed Project We put our heads together to name every scientist we Ozma throughout, and had since been trying to build knew who was even thinking about searching for ex- support in the government for the possibility of dis- traterrestrial life in 1961. -
Curriculum Vitae G. Seth Shostak ______Tel
Curriculum Vitae G. Seth Shostak _______________________________________________________________________ tel. office: (650)-960-4530 e-mail: [email protected] Education Ph.D. astrophysics, California Institute of Technology, Pasadena, California B.A. physics, Princeton University, Princeton, New Jersey Experience Senior Astronomer, SETI Institute, Mtn. View, Calif. 2001-present Public Programs Scientist, SETI Institute, Mtn. View, Calif. 1991-2001 Cable TV Channel 27, Mtn. View, Calif. 1990-1991 Senior Software Engineer, Mira Technology, Los Altos, Calif. 1988-1989 Director and Founder, Digital Images Computer Animation, Groningen, The Netherlands 1983-1988 Research Associate, Kapteyn Astronomical Institute, State University of Groningen, The Netherlands 1975-1983 Senior Systems Analyst, Penn Central Transportation Co., Philadelphia, Penn. 1974-1975 Research Associate, National Radio Astronomy Observatory, Charlottesville, Virginia 1972-1974 Publications Astronomical: More than 60 research papers in refereed, professional journals Film: More than 50 articles for magazines and newspapers on film and video. Author of monthly column on film techniques in European magazines from 1980-1982, and 1985-1990. Science and Technology: Approximately three hundred popular articles published in magazines, newspapers and the Web, on a wide range of topics. Scripts: Several commissioned scripts for public relations videos produced for commercial clients. Two scripts for planetarium shows. Books: Editor of two scientific books, contributor to five popular -
Communication with Extraterrestrial Intelligence (CETI), Ed
Exoplanets, Extremophiles, and the Search for Extraterrestrial Intelligence Jill C. Tarter 1.0. Introduction We discovered the very first planetary worlds in orbit around a body other than the Sun in 1991 (Wolzczan and Frail 1992). They were small bodies (0.02, 4.3, and 3.9 times as massive as the Earth) and presented a puzzle because they orbit a neutron star (the remnant core of a more massive star that had previously exploded as a supernova) and it was not clear whether these bodies survived the explosion or reformed from the stellar debris. They still present a puzzle, but today we know of over five hundred other planetary bodies in orbit around hundreds of garden variety stars in the prime of their life cycle. Many of these planets are more massive than Jupiter, and some orbit closer to their stars than Mercury around the Sun. To date we have not found another planetary system that is an exact analog of the Earth (and the other planets of our solar system) orbiting a solar-type star, but we think that is because we have not yet had the right observing instruments. Those are on the way. In the next few years, we should know whether other Earth mass planets are plentiful or scarce. At the same time that we have been developing the capabilities to detect distant Earths, we have also been finding that life on Earth occurs in places that earlier scientists would have considered too hostile to support life. Scientists were wrong, or at least didn’t give microbes the respect they deserve. -
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. -
Women in Astronomy: an Introductory Resource Guide
Women in Astronomy: An Introductory Resource Guide by Andrew Fraknoi (Fromm Institute, University of San Francisco) [April 2019] © copyright 2019 by Andrew Fraknoi. All rights reserved. For permission to use, or to suggest additional materials, please contact the author at e-mail: fraknoi {at} fhda {dot} edu This guide to non-technical English-language materials is not meant to be a comprehensive or scholarly introduction to the complex topic of the role of women in astronomy. It is simply a resource for educators and students who wish to begin exploring the challenges and triumphs of women of the past and present. It’s also an opportunity to get to know the lives and work of some of the key women who have overcome prejudice and exclusion to make significant contributions to our field. We only include a representative selection of living women astronomers about whom non-technical material at the level of beginning astronomy students is easily available. Lack of inclusion in this introductory list is not meant to suggest any less importance. We also don’t include Wikipedia articles, although those are sometimes a good place for students to begin. Suggestions for additional non-technical listings are most welcome. Vera Rubin Annie Cannon & Henrietta Leavitt Maria Mitchell Cecilia Payne ______________________________________________________________________________ Table of Contents: 1. Written Resources on the History of Women in Astronomy 2. Written Resources on Issues Women Face 3. Web Resources on the History of Women in Astronomy 4. Web Resources on Issues Women Face 5. Material on Some Specific Women Astronomers of the Past: Annie Cannon Margaret Huggins Nancy Roman Agnes Clerke Henrietta Leavitt Vera Rubin Williamina Fleming Antonia Maury Charlotte Moore Sitterly Caroline Herschel Maria Mitchell Mary Somerville Dorrit Hoffleit Cecilia Payne-Gaposchkin Beatrice Tinsley Helen Sawyer Hogg Dorothea Klumpke Roberts 6. -
FRANK D. DRAKE Education 1952 Cornell University BA, Engineering
Biographical Sketch FRANK D. DRAKE Education 1952 Cornell University B.A., Engineering Physics (with honors) 1956 Harvard University M.S., Astronomy 1958 Harvard University Ph.D., Astronomy Professional Employment 1952-1956 U.S. Navy, Electronics Officer 1956-1958 Agassiz Station Radio Astronomy Project, Harvard University 1958-1963 National Radio Astronomy Observatory, Green Bank, West Virginia - Head of Telescope Operations & Scientific Services Division - Conducted planetary research and cosmic radio source studies 1963-64 Jet Propulsion Laboratory, Chief of Lunar & Planetary Sciences 1964-1984 Cornell University - Associate Professor of Astronomy (1964); then Full Professor (1966) - Associate Director, Center for Radiophysics & Space Research (1964-75) - Director, Arecibo Observatory, Arecibo, Puerto Rico (1966-1968) - Chairman, Astronomy Department, Cornell University (1969-71) - Director, National Astronomy & Ionosphere Center, part of which is the Arecibo Observatory (from its creation in 1970 until July 1981) - Goldwin Smith Professor of Astronomy, Cornell University (1976-84) 1984-Present University of California, Santa Cruz - Dean, Natural Sciences Division (1984-1988) - Acting Associate Vice Chancellor, University Advancement (1989-90) - Professor of Astronomy & Astrophysics (1984 – 1996) - Professor Emeritus of Astronomy & Astrophysics, (1996 –present) 1984-Present SETI Institute, Mountain View, California: - President (1984-2000) - Chairman, Board of Trustees, (1984-2003) - Chairman Emeritus, Board of Trustees, 2003- present - Director, Carl Sagan Center for the Study of Life in the Universe, 2004-present Professional Achievements 1959 Shared in the discovery of the radiation belts of Jupiter, and conducted early pulsar observational studies 1960 Conducted Project OZMA at NRAO, Green Bank, WV -- the first organized search for ETI signals 1961 Devised widely-known Drake Equation, giving an estimate of the number of communicative extraterrestrial civilizations that we might find in our galaxy.