Vol 11 No 1, Winter 2005
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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. -
A Direct Communication Proposal to Test the Zoo Hypothesis
Space Policy 38 (2016) 22e26 Contents lists available at ScienceDirect Space Policy journal homepage: www.elsevier.com/locate/spacepol Viewpoint A direct communication proposal to test the Zoo Hypothesis Joao~ Pedro de Magalhaes~ Institute of Integrative Biology, University of Liverpool, Biosciences Building, Room 245, Crown Street, Liverpool, L69 7ZB, UK article info abstract Article history: Whether we are alone in the universe is one of the greatest mysteries facing humankind. Given the >100 Received 3 March 2016 billion stars in our galaxy, many have argued that it is statistically unlikely that life, including intelligent Accepted 16 June 2016 life, has not emerged anywhere else. The lack of any sign of extraterrestrial intelligence, even though on a Available online 26 July 2016 cosmic timescale extraterrestrial civilizations would have enough time to cross the galaxy, is known as Fermi's Paradox. One possible explanation for Fermi's Paradox is the Zoo Hypothesis which states that Keywords: one or more extraterrestrial civilizations know of our existence and can reach us, but have chosen not to Active SETI disturb us or even make their existence known to us. I propose here a proactive test of the Zoo Hy- Astrobiology fi Fermi's Paradox pothesis. Speci cally, I propose to send a message using television and radio channels to any extrater- Messaging to extraterrestrial intelligence restrial civilization(s) that might be listening and inviting them to respond. Even though I accept this is METI unlikely to be successful in the sense of resulting in a response from extraterrestrial intelligences, the possibility that extraterrestrial civilizations are monitoring us cannot be dismissed and my proposal is consistent with current scientific knowledge. -
June 2012 FINAL
! Vol.!60,!No.!5!+!May!2012! ! Wednesday, June 20, 2012 – General Meeting Randall Museum . 199 Museum Way . San Francisco 7:00 pm Doors Open . 7:30 pm Announcements . 8:00 pm Speaker SFAA’s General Meetings occur on the 3rd Wednesday of#each#month#(except#January)# # ! ADAM MILLER, Graduate Student, UC Berkeley THE VERY BRIGHTEST SUPERNOVAE: NATURE'S NEW MYSTERIOUS EXPLOSIONS DEFY CONVENTIONAL EXPLANATION Join Adam Miller for a presentation addressing various sub-types of supernovae, dominant energy sources powering them, methods used to discover new supernovae and recent surveys leading to discovery of thousands of new supernovae. These surveys have uncovered a new class of super-luminous supernovae that are as much as 100 times brighter than the conventional explosion at the end of the life of a massive star. New theories are being developed to understand these mysterious explosions, and future surveys should provide dozens of new examples to better study them. Adam Miller is a graduate student in the UC Berkeley Department of Astronomy and a member of the Palomar Transient Factory (PTF). He received a bachelors in physics and theater at MIT and a master's in physics from the University of Cambridge. He is currently working toward a doctorate at UC Berkeley. His research interests include anything that "goes bump in the night": all astronomical objects that vary in brightness over long or short durations of time. As a member of the PTF, he has contributed to their discovery of more than one thousand supernovae in the past three years, including the very bright supernova 2011fe in the spiral galaxy M101, which was featured on PBS NewsHour. -
View As a PDF File
September 2010 onomica tr l A s s A s e o s c i o a J t i EPHEMERIS o n a n S SJAA Alien Life: Wanna Bet? SJAA Activities Calendar Paul Kohlmiller Jim Van Nuland August (late) You can bet on almost anything. The 28 General Meeting at 8 p.m. Our speaker is Dr. Seth Shostak from the SETI Institute. entire science called astrobiology is His talk is on “New Approaches to the Search for Extraterrestrial Intelligence”. betting that there is life somewhere other than Earth. What are the September odds? Currently the odds on finding 3 Astronomy Class at Houge Park. 7:30 p.m. Topic is TBA. intelligent life are dropping. There 3 Houge Park star party. Sunset 7:33 p.m., 23% moon rises 2:09 a.m. Star party is a betting office online based in hours: 8:30 until 11:30. England that will give odds on finding 4 Dark Sky weekend. Sunset 7:32 p.m., 14% moon rises 3:21 a.m. extraterrestrial intelligent life. It is 11 Dark Sky weekend. Sunset 7:21 p.m., 20% moon sets 9:11 p.m. Henry Coe Park’s called William Hill. They dropped the “Astronomy” lot has been reserved. odds from 1000-1 to 100-1 when the 17 Houge Park star party. Sunset 7:12 p.m., 78% moon sets 2:32 a.m. Star party first almost Earth-like exoplanets were discovered. hours: 8:00 until 11:00. 25 General Meeting at 8 p.m. Slide and Equipment night (aka “Show and Tell”). -
CURRICULUM VITAE DOUGLAS A. VAKOCH Center for SETI Research
CURRICULUM VITAE DOUGLAS A. VAKOCH Center for SETI Research Department of Clinical Psychology SETI Institute California Institute of Integral Studies 189 N. Bernardo Ave., Suite 100 1453 Mission Street Mountain View, CA 94043, USA San Francisco, CA 94103, USA Office Phone: +1-650-960-4514 Office Phone: +1-415-575-6244 Office Fax: +1-650-968-5830 Office Fax: +1-415-575-1266 Email: [email protected] Email: [email protected] Residence 943 Cherry Way Hayward, CA 94541 Home Phone: 510-481-5719 PROFESSIONAL APPOINTMENTS Professor, Department of Clinical Psychology, California Institute of Integral Studies, 2011-present Associate Professor, Department of Clinical Psychology, California Institute of Integral Studies, 2008-2011 Assistant Professor, Department of Clinical Psychology, California Institute of Integral Studies, 2005-2008 Director of Interstellar Message Composition, SETI Institute, 2001-present Social Scientist, SETI Institute, 1999-present Research Associate, Department of Psychology, University of California, Davis, 1999- 2001, 2005-2007 National Research Service Award Postdoctoral Fellow, Department of Psychology, Vanderbilt University, 1996-1998 Predoctoral Clinical Intern, Departments of Rehabilitation Medicine and Psychiatry, University of Wisconsin-Madison Hospital and Clinics, 1995-1996 EDUCATION Ph.D., Clinical Psychology with Quantitative Minor, State University of New York at Stony Brook, 1996. Dissertation: Predictors of prognosis for patients with interpersonal problems: The role of therapists’ epistemology, experience, optimism, and theoretical orientation. M.A., Psychology, State University of New York at Stony Brook, 1994. M.A., History and Philosophy of Science, University of Notre Dame, 1991. B.A., Religion, Carleton College, 1983. Senior Thesis: Psychological analyses of the mystic path in Christianity and Buddhism. -
Vol 11 No 2, Spring 2005
SearchLites Vol. 11 No. 2, Spring 2005 The Quarterly Newsletter of The SETI League, Inc. Offices: 433 Liberty Street Scaling Back on SETICon PO Box 555 Little Ferry NJ Little Ferry, NJ.., 19 February 2005 -- Five years after initiating its SETICon Technical 07643 USA Symposium, the nonprofit, membership-supported SETI League has had to scale back the annual membership event to more modest proportions. Because The SETI League chose Phone: to make its meetings affordable and accessible to a wide range of amateur radio astrono- (201) 641-1770 Facsimile: mers, the events have proved a steady drain on the grassroots science group's limited fi- (201) 641-1771 nancial resources. Hence, the organization's 2005 annual meeting will be held in conjunc- Email: tion with another, much larger and well-established conference. [email protected] Web: "The last few SETICons cost us about $4,000 each to put on," notes Dr. H. Paul www.setileague.org Shuch, volunteer executive director of The SETI League. "Depending as we do upon President: membership dues and individual contributions, we thought our limited funding would be Richard Factor better spent on SETI science than on hosting scientific meetings." Consequently, Shuch Registered Agent: announced, The SETI League's 2005 Annual Membership Meeting will be held on the Marc Arnold, Esq. campus of The College of New Jersey, in conjunction with the annual Trenton Computer Secretary/Treasurer: A. Heather Wood Festival. Executive Director: H. Paul Shuch, Ph.D. This year's Trenton Computer Festival is scheduled to run the weekend of 16-17 April, 2005, with The SETI League's membership meeting to be held there on Sunday morning, 17 April, from 10 AM until Noon. -
Starry Messages: Searching for Signatures of Interstellar Archaeology
FERMILAB-PUB-09-607-AD Starry Messages: Searching for Signatures of Interstellar Archaeology Richard A. Carrigan, Jr., Fermi National Accelerator Laboratory*, Batavia, IL 60510, USA [email protected] 630-840-8755 Summary Searching for signatures of cosmic-scale archaeological artifacts such as Dyson spheres or Kardashev civilizations is an interesting alternative to conventional SETI. Uncovering such an artifact does not require the intentional transmission of a signal on the part of the original civilization. This type of search is called interstellar archaeology or sometimes cosmic archaeology. The detection of intelligence elsewhere in the Universe with interstellar archaeology or SETI would have broad implications for science. For example, the constraints of the anthropic principle would have to be loosened if a different type of intelligence was discovered elsewhere. A variety of interstellar archaeology signatures are discussed including non-natural planetary atmospheric constituents, stellar doping with isotopes of nuclear wastes, Dyson spheres, as well as signatures of stellar and galactic-scale engineering. The concept of a Fermi bubble due to interstellar migration is introduced in the discussion of galactic signatures. These potential interstellar archaeological signatures are classified using the Kardashev scale. A modified Drake equation is used to evaluate the relative challenges of finding various sources. With few exceptions interstellar archaeological signatures are clouded and beyond current technological capabilities. However SETI for so- called cultural transmissions and planetary atmosphere signatures are within reach. Keywords: Interstellar archaeology, Dyson spheres, Kardashev scale, SETI, Drake equation ACKNOWLEDGEMENT *Operated by the Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the United States Department of Energy. -
Interstellar Messaging—An Embodied Perspective Carrie Paterson, California State University, Fullerton
Interstellar Messaging—An Embodied Perspective Carrie Paterson, California State University, Fullerton. [email protected] This paper suggests rationales and new methodologies for sending interstellar messages in the search for extra-terrestrial intelligence. While it is widely accepted that radio signals are the most applicable way to send interstellar messages, other methods should also be explored. I propose multi-colored lasers with light polarization be considered for sending signals because of the possibilities to create multi-channel, pluralistic and complex representations of terrestrial environments and the embodied experience of living on Earth. This paper gives the background to justify the proposal. As far as we know, Earth is a unique heavenly body, though new findings suggest habitable planets in the Milky Way galaxy and the universe on the whole are common. Any signal should reflect an acknowledgement that life on Earth—and indeed, our intelligence— arises from and is specific to our environment. While this paper cannot concentrate on the technical aspects of encoding interstellar messages to differentiate a signal from noise1 or the physics of optical signals due to time and my own lack of expertise, it will cover the historical aspects of interstellar messaging, and a critique of how our bodies have been envisioned and translated into binary code for transmission through space. As well, I lay the groundwork for future explorations about the new freedoms and conflicts that technological developments have proven to bring to the science of interstellar messaging, and how a confrontation of past efforts opens a window onto creative ideas for constructing future signals. As an artist-researcher I have studied the history of interstellar communications, both in signals and on spacecraft, as well as current trends. -
Report 2017 Research, Education and Public Outreach Activity Report 2017 Research, Education and Public Outreach
Activity Report 2017 Research, Education and Public Outreach Activity Report 2017 Research, Education and Public Outreach Nathalie A. Cabrol Director, Carl Sagan Center, Pamela Harman, Acting Director, Center for Education Rebecca McDonald Director, Center for Outreach Bill Diamond President & CEO The SETI Institute: 189 N Bernardo Avenue Suite 200, Mountain View, CA 94043. Phone: (650) 961-6633 Activity Report 2017 Research, Education and Public Outreach TABLE OF CONTENTS Peer-reviewed publications 10 Conferences: Abstracts & Proceedings 18 Technical Reports & Data Releases 29 Outreach, Media Coverage, Web Stories & Interviews 31 Invited Talks (Professional & Public) 39 Highlights, Significant Events & Activities 46 Fieldwork 52 Honors & Awards 54 Missions, Observations & Strategic Planning 56 Acknowledgements 60 The SETI Institute: 189 N Bernardo Avenue Suite 200, Mountain View, CA 94043. Phone: (650) 961-6633 Activity Report 2017 Research, Education and Public Outreach FROM THE SETI INSTITUTE President and CEO Dear friends, The scientists, educators and outreach professionals of the SETI Institute had yet another banner year of productivity in 2017. We are delighted to present our 2nd annual report, cataloging the research and education programs of the Institute, as well as the myriad of mainstream media stories about our people and our work. Among the highlights from this year’s report are 147 peer-reviewed articles in scientific journals, 225 conference proceedings and abstracts, 172 media stories and interviews, and 177 invited talks. -
New SETI Prospects Opened up by Current Information Networking Elisabeth Piotelat, Florence Raulin-Cerceau
New SETI prospects opened up by current information networking Elisabeth Piotelat, Florence Raulin-Cerceau To cite this version: Elisabeth Piotelat, Florence Raulin-Cerceau. New SETI prospects opened up by current information networking. International Journal of Astrobiology, Cambridge University Press (CUP), 2013, Special Issue, 12 (3), pp.208-211. 10.1017/S1473550413000141. hal-01360236 HAL Id: hal-01360236 https://hal.archives-ouvertes.fr/hal-01360236 Submitted on 27 Sep 2016 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. New SETI prospects opened up by current information networking Elisabeth Piotelat Laboratoire d'Informatique pour la Mécanique et les Sciences de l'Ingénieur (LIMSI-CNRS), Orsay, France Florence Raulin Cerceau Centre Alexandre Koyré (UMR 8560 EHESS/CNRS/MNHN) Muséum national d’Histoire naturelle, Paris, France Corresponding author: [email protected] Phone: +33/1 69 85 80 06 Fax: +33/1 69 85 80 88 Address: LIMSI-CNRS, B.P. 133, 91403 Orsay Cedex Abstract This paper proposes to think the fc factor of the Drake equation over, i.e. the fraction of planets with intelligent creatures capable of interstellar communication as defined by Frank Drake in 1961. -
Life in the Universe
Northeastern Illinois University Life in the Universe Greg Anderson Department of Physics & Astronomy Northeastern Illinois University Winter-Spring 2020 c 2012-2020 G. Anderson Introduction to Astronomy – slide 1 / 92 Northeastern Illinois Overview University Daing Rocks Life on Earth How Did Life Arise? Life in the Solar System Life Around Other Stars Interstellar Travel SETI Review c 2012-2020 G. Anderson Introduction to Astronomy – slide 2 / 92 Northeastern Illinois University Daing Rocks Zircon Dating Sedimentary Grand Canyon Life on Earth How Did Life Arise? Life in the Solar System Life Around Daing Rocks Other Stars Interstellar Travel SETI Review c 2012-2020 G. Anderson Introduction to Astronomy – slide 3 / 92 Northeastern Illinois Zircon Dating University 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 2012-2020 G. Anderson Introduction to Astronomy – slide 4 / 92 Northeastern Illinois Dating Sedimentary Rocks University • Relative ages: Deeper layers were deposited earlier • Absolute ages: Decay of radioactive isotopes old (deposited last) oldest (depositedolder first) c 2012-2020 G. Anderson Introduction to Astronomy – slide 5 / 92 Grand Canyon: Earth History from 200 million - 2 billion yrs ago. Northeastern Illinois University Daing Rocks Life on Earth Earth History Timeline Late Heavy Bombardment Hadean Greenland Shark Bay Stromatolites Cyanobacteria Life on Earth Q: Earliest Fossils? O2 History Q: Life on Earth How Did Life Arise? Life in the Solar System Life Around Other Stars Interstellar Travel SETI Review c 2012-2020 G. -
Quantifying Past Transmissions Using the San Marino Scale
IAC-07-A4.2.04 QUANTIFYING PAST TRANSMISSIONS USING THE SAN MARINO SCALE Shuch, H. Paul Almár, Iván The SETI League, Inc. Konkoly Observatory 121 Florence Drive Hungarian Academy of Sciences Cogan Station PA 17728 USA Budapest, Hungary [email protected] [email protected] ABSTRACT To date, at least five experiments which could be classified as Active SETI, or METI (Messaging to Extra-Terrestrial Intelligence) have been conducted from Planet Earth: the well-known Arecibo Message of 1974, two Cosmic Call transmissions from Evpatoria, the Teen-Age Message to the Stars also transmitted from Evpatoria, and the paradigm- altering Invitation to ETI, being quasi-transmitted continuously via the Internet. In addi- tion, planetary defense radar transmissions from Earth, radiated for the purpose of detect- ing potentially hazardous asteroids, can be considered inadvertent METI signals, to the extent that they can be detected over interstellar distances. Planetary radar transmissions from both Goldstone and Arecibo are considered. Each of these various emissions is ana- lyzed in terms of duration, directionality, information content, and transmitter power, and then each is assigned an integer ordinal value on the proposed San Marino scale for quan- tifying transmissions from Earth. A comparative analysis of these quantified transmis- sions underscores the difference in impact of various METI experiments, suggesting the utility of the San Marino Scale as a valuable analytical tool for making informed policy decisions. INTRODUCTION ing the potential impact of such trans- missions from Earth. Here we apply the SETI, the well established science San Marino Scale to several historical involved with Searching for Extra- transmissions, to better assess its utility.