Internalizing Null Extraterrestrial “Signals”: an Astrobiological App for a Technological Society
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Lecture-29 (PDF)
Life in the Universe Orin Harris and Greg Anderson Department of Physics & Astronomy Northeastern Illinois University Spring 2021 c 2012-2021 G. Anderson., O. Harris Universe: Past, Present & Future – slide 1 / 95 Overview Dating Rocks Life on Earth How Did Life Arise? Life in the Solar System Life Around Other Stars Interstellar Travel SETI Review c 2012-2021 G. Anderson., O. Harris Universe: Past, Present & Future – slide 2 / 95 Dating Rocks Zircon Dating Sedimentary Grand Canyon Life on Earth How Did Life Arise? Life in the Solar System Life Around Dating Rocks Other Stars Interstellar Travel SETI Review c 2012-2021 G. Anderson., O. Harris Universe: Past, Present & Future – slide 3 / 95 Zircon Dating Zircon, (ZrSiO4), minerals incorporate trace amounts of uranium but reject lead. Naturally occuring uranium: • U-238: 99.27% • U-235: 0.72% Decay chains: • 238U −→ 206Pb, τ =4.47 Gyrs. • 235U −→ 207Pb, τ = 704 Myrs. 1956, Clair Camron Patterson dated the Canyon Diablo meteorite: τ =4.55 Gyrs. c 2012-2021 G. Anderson., O. Harris Universe: Past, Present & Future – slide 4 / 95 Dating Sedimentary Rocks • Relative ages: Deeper layers were deposited earlier • Absolute ages: Decay of radioactive isotopes old (deposited last) oldest (depositedolder first) c 2012-2021 G. Anderson., O. Harris Universe: Past, Present & Future – slide 5 / 95 Grand Canyon: Earth History from 200 million - 2 billion yrs ago. Dating Rocks Life on Earth Earth History Timeline Late Heavy Bombardment Hadean Shark Bay Stromatolites Cyanobacteria Q: Earliest Fossils? Life on Earth O2 History Q: Life on Earth How Did Life Arise? Life in the Solar System Life Around Other Stars Interstellar Travel SETI Review c 2012-2021 G. -
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. -
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. -
Fermi's Paradox Is a Daunting Problem – Under Whatever Label
Fermi's Paradox Is a Daunting Problem – Under Whatever Label Milan M. Dirkovid1 Astronomical Observatory of Belgrade, Volgina 7, 11000 Belgrade, Serbia 1. Introduction Gray (2015) argued that Fermi's paradox (FP) is a misnomer, and it is not a valid paradox. Gray also speculated that the argument was misattributed to Fermi, whose lunchtime remarks did not pertain to the existence of extraterrestrial intelligence, but to the feasibility of interstellar travel. Instead, the paradox is ascribed to Hart and Tipler, and it is further suggested that the paradox is not a “real” problem or research subject and should not be used in debates about SETI projects. The arguments given are unpersuasive, ahistorical, and, in at least one instance, clearly hinge on literalistic and uncharitable reading of evidence. Instead, I argue the following three points: (i) Contrary to Gray’s assertion, the historical issue of naming of ideas or concepts is completely divorced from their epistemic status. (ii) FP is easily and smoothly generalized into the “Great Silence” paradox, so it makes no sense either theoretically or empirically to separate the two. (iii) In sharp contrast to the main implication of Gray’s paper, FP has become more aggravated lately due to advances in astrobiology. Research that deals with FP has greatly expanded in recent years on both a theoretical and observational stage (Davies 2010, 2012; Vukotid and Dirkovid 2012; Barlow 2013; Hair and Hedman 2013; Davies and Wagner 2013; Armstrong and Sandberg 2013; Lampton 2013; Cartin 2014; Nunn, Guy, and Bell 2014; Wright et al. 2014; Spivey 2015; Griffith et al. -
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. -
Arxiv:1908.02683V1 [Astro-Ph.IM] 31 Jul 2019
Draft version August 8, 2019 Typeset using LATEX default style in AASTeX62 Nine Axes of Merit for Technosignature Searches Sofia Z. Sheikh1 1Department of Astronomy & Astrophysics and Center for Exoplanets and Habitable Worlds 525 Davey Laboratory, The Pennsylvania State University, University Park, PA, 16802, USA ABSTRACT The diverse methodologies and myriad orthogonal proposals for the best technosignatures to search for in SETI can make it difficult to develop an effective and balanced search strategy, especially from a funding perspective. Here I propose a framework to compare the relative advantages and disadvantages of various proposed technosignatures based on nine \axes of merit". This framework was first developed at the NASA Technosignatures Workshop in Houston in 2018 and published in that report. I give the definition and rationale behind the nine axes as well as the history of each axis in the SETI and technosignature literature. These axes are then applied to three example classes of technosignature searches as an illustration of their use. An open-source software tool is available to allow technosignature researchers to make their own version of the figure. Keywords: extraterrestrial intelligence 1. INTRODUCTION Proposed searches for technosignatures range from radio wavelengths to gamma rays, take advantage of almost every astronomical dataset, and use interdisciplinary methodologies in such a way that comparing the merits of two dissimilar searches, even if they're ostensibly in the same field, can be an extremely difficult task. Each SETI practitioner has a different answer for the best strategy to find ETI, often in her own wavelength. Much of the SETI literature engages in promoting the values of a particular search strategy. -
What Happens When We Detect Alien Life?
SETI research e’ve never heard a peep from aliens. But improved technology is speeding up the search for extra- terrestrial intelligence (SETI), so what happens if today’s silence suddenly gives way to tomorrow’s discovery? Would the world Wrejoice in the news that someone’s out there? Would euphoria engulf humanity, as Nobel Prizes are doled out like after-dinner mints? That’s one view. But many people think the dis- covery would be hushed up as quickly as a Mafia informant, assuming that the public couldn’t handle the news. Or scarier still, kept secret for fear that an unauthorized response would tell a hostile race exactly where to send their interstellar battlewagons. That’s melodramatic enough. But has any serious consideration gone into what happens when our efforts to detect cos- mic intelligence pay off and we find a blip of a signal in the sea of radio noise WHAT HAPPENS WHEN WE DETECT that pours into the SETI antennas? Some think that addressing that question — even in a speculative way — is hubristic at best and wildly pre- sumptuous at worst. After all, SETI scientists have been torquing their telescopes toward celestial targets for ALINF E LI E? more than half a century without ever detecting such a signal. If we Scientists have been listening for signals from extraterrestrial haven’t won the E.T. lottery in all that time, why worry about what would civilizations for decades, but what would they do happen if we got the winning ticket? if they actually heard one? Simple: SETI researchers are buy- ing more tickets all the time, and the by Seth Shostak chances of scoring the big one keep going up. -
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. -
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. -
Jill Tarter PUBLIC LECTURE TRANSCRIPT
Jill Tarter PUBLIC LECTURE TRANSCRIPT March 3, 2015 KANE HALL 130 | 7:30 P.M. TABLE OF CONTENTS INTRODUCTION, page 1 Marie Clement, Graduate Student, Chemistry FEATURED SPEAKER, page 1 Jill Tarter, Bernard M. Oliver chair for SETI Q&A SESSION, page 8 OFFICE OF PUBLIC LECTURES So our speaker tonight is Dr. Jill Cornell Tarter. Jill Tarter holds INTRODUCTION the Bernard M. Oliver chair for SETI, the Search for Extraterrestrial Intelligence at the SETI Institute in Mountain View, California. Tarter received her Bachelor of Engineering Physics degree with distinction from Cornell University and her Marie Clement master's degree and Ph.D. in astronomy from the University of California Berkeley. She served as project scientist for NASA Graduate Student SETI program, the High Resolution Microwave Survey, and has conducted numerous observational programs at radio Good evening, and welcome to tonight's Jessie and John Danz observatories worldwide. Since the termination of funding for endowed public lecture with Jill Cornell Tarter. I am Marie NASA SETI program in 1993, she has served in a leadership role Clement, a graduate student in the chemistry department and a to secure private funding to continue this exploratory science. member of the student organization, Women in Chemical Tarter’s work has brought her wide recognition in the scientific Sciences. Before we introduce tonight's speaker, I want to community, including the Lifetime Achievement Award from share some background about the generous gift to the Women in Aerospace, two Public Service Medals from NASA, University of Washington that allows the Graduate School to Chabot Observatory’s Person of the Year award, Women of host the series: the Jessie and John Danz Endowment. -
The Search for Extraterrestrial Intelligence (Seti)
27 Jul 2001 20:34 AR AR137-13.tex AR137-13.SGM ARv2(2001/05/10) P1: GSR Annu. Rev. Astron. Astrophys. 2001. 39:511–48 Copyright c 2001 by Annual Reviews. All rights reserved THE SEARCH FOR EXTRATERRESTRIAL INTELLIGENCE (SETI) Jill Tarter SETI Institute, 2035 Landings Drive, Mountain View, California 94043; e-mail: [email protected] Key Words exobiology, astrobiology, bioastronomy, optical SETI, life in the universe ■ Abstract The search for evidence of extraterrestrial intelligence is placed in the broader astronomical context of the search for extrasolar planets and biomarkers of primitive life elsewhere in the universe. A decision tree of possible search strategies is presented as well as a brief history of the search for extraterrestrial intelligence (SETI) projects since 1960. The characteristics of 14 SETI projects currently operating on telescopes are discussed and compared using one of many possible figures of merit. Plans for SETI searches in the immediate and more distant future are outlined. Plans for success, the significance of null results, and some opinions on deliberate transmission of signals (as well as listening) are also included. SETI results to date are negative, but in reality, not much searching has yet been done. INTRODUCTION From the dawn of civilization, humans have looked skyward and wondered whether by University of Oregon on 09/13/06. For personal use only. we share this universe with other sentient beings. For millennia we have asked our philosophers and priests to answer this question for us. Answers have always been forthcoming and have reflected the belief system represented by the person providing the answers (Dick 1998). -
Searches for Life and Intelligence Beyond Earth
Technologies of Perception: Searches for Life and Intelligence Beyond Earth by Claire Isabel Webb Bachelor of Arts, cum laude Vassar College, 2010 Submitted to the Program in Science, Technology and Society in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy in History, Anthropology, and Science, Technology and Society at the Massachusetts Institute of Technology September 2020 © 2020 Claire Isabel Webb. All Rights Reserved. The author hereby grants to MIT permission to reproduce and distribute publicly paper and electronic copies of this thesis document in whole or in part in any medium now known or hereafter created. Signature of Author: _____________________________________________________________ History, Anthropology, and Science, Technology and Society August 24, 2020 Certified by: ___________________________________________________________________ David Kaiser Germeshausen Professor of the History of Science (STS) Professor of Physics Thesis Supervisor Certified by: ___________________________________________________________________ Stefan Helmreich Elting E. Morison Professor of Anthropology Thesis Committee Member Certified by: ___________________________________________________________________ Sally Haslanger Ford Professor of Philosophy and Women’s and Gender Studies Thesis Committee Member Accepted by: ___________________________________________________________________ Graham Jones Associate Professor of Anthropology Director of Graduate Studies, History, Anthropology, and STS Accepted by: ___________________________________________________________________