Astrobiology and the Search for Life Beyond Earth in the Next Decade
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[email protected], Rectorville, VA 20140
VEXAG Organizing Committee / Venus STDT Contact Info TWT - 12 JUne 08 Name Function Affiliation Address Phone Cell Fax E-Mail Adriana Ocampo NASA Program Executive NASA Headquarters Suite 3X63 202-358-2152 202-297-3530 202-358-3097 [email protected] NASA Headquarters 300 E-Street SW Washington DC 20546-0001 Ellen Stofan VEXAG Chair Proxemy, Inc. Windrush Farm 540-364-0092 540-364-1071 [email protected] P. O. Box 338 [email protected], Rectorville, VA 20140 David Grinspoon Earth-Venus Climate Denver Museum Dept. Of Space Sciences 303-370-6469 303-370-6005 [email protected], Connections of Nature and Science 2001 Coloradlo Blvd. Denver, CO 80205 Mark Allen Technology for Venus JPL Mail Stop 183-401 818-354-3665 818 393-4445 [email protected], In-Situ Exploration Focus Jet Propulsion Laboratory Group Lead 4800 Oak Grove Drive Pasadena CA 91109-8099 Steve Mackwell Planetary Formation and LPI Lunar and Planetary Institute 281-486-2128 281-389-3032 281-486-2127 [email protected] Evolution Focus Group Lead 3600 Bay Area Blvd. 281-486-2180 Houston, TX 77058 281-486-2100 Kevin Baines Atmospheric Evolution JPL Mail Stop 183-601 818-354-0481 818-667-2040 818-354-5148 [email protected] Focus Group Lead Jet Propulsion Laboratory 4800 Oak Grove Drive Pasadena CA 91109-8099 Jim Cutts Technology for Venus JPL Mail Stop 301-345 818-354-4120 626-375-9898 818-354-8333 [email protected] In-Situ Exploration Focus Jet Propulsion Laboratory Group Lead 4800 Oak Grove Drive Pasadena CA 91109-8099 Larry Esposito Earth-Venus Climate LASP - Univ of Colorado LASP - Univ of Colorado 303-492-5990 303-492-6946 [email protected] Connections 1234 Innovation Drive Boulder, CO 80303-7814 Mark Bullock Venus STDT Chair Southwest Research Inst. -
SETI Is Part of Astrobiology
SETI is Part of Astrobiology Jason T. Wright Department of Astronomy & Physics Center for Exoplanets and Habitable Worlds Penn State University Phone: (814) 863-8470 [email protected] I. SETI is Part of Astrobiology “Traditional SETI is not part of astrobiology” declares the NASA Astrobiology Strategy 2015 document (p. 150). This is incorrect.1 Astrobiology is the study of life in the universe, in particular its “origin, evolution, distribution, and future in the universe.” [emphasis mine] Searches for biosignatures are searches for the results of interactions between life and its environment, and could be sensitive to even primitive life on other worlds. As such, these searches focus on the origin and evolution of life, using past life on Earth as a guide. But some of the most obvious ways in which Earth is inhabited today are its technosignatures such as radio transmissions, alterations of its atmosphere by industrial pollutants, and probes throughout the Solar System. It seems clear that the future of life on Earth includes the development of ever more obvious technosignatures. Indeed, the NASA Astrobiology Strategy 2015 document acknowledges “the possibility” that such technosignatures exist, but erroneously declares them to be “not part of contemporary SETI,” and mentions them only to declare that we should “be aware of the possibility” and to “be sure to include [technosignatures] as a possible kind of interpretation we should consider as we begin to get data on the exoplanets.” In other words, while speculation on the nature of biosignatures and the design of multi-billion dollar missions to find those signatures is consistent with NASA’s vision for astrobiology, speculation on the nature of technosignatures and the design of observations to find them is not. -
ASU Colloquium
New Frontiers in Artifact SETI: Waste Heat, Alien Megastructures, and "Tabby's Star" Jason T Wright Penn State University SESE Colloquium Arizona State University October 4, 2017 Contact (Warner Bros.) What is SETI? • “The Search for Extraterrestrial Intelligence” • A field of study, like cosmology or planetary science • SETI Institute: • Research center in Mountain View, California • Astrobiology, astronomy, planetary science, radio SETI • Runs the Allen Telescope Array • Berkeley SETI Research Center: • Hosted by the UC Berkeley Astronomy Department • Mostly radio astronomy and exoplanet detection • Runs SETI@Home • Runs the $90M Breakthrough Listen Project Communication SETI The birth of Radio SETI 1960 — Cocconi & Morrison suggest interstellar communication via radio waves Allen Telescope Array Operated by the SETI Institute Green Bank Telescope Operated by the National Radio Astronomy Observatory Artifact SETI Dyson (1960) Energy-hungry civilizations might use a significant fraction of available starlight to power themselves Energy is never “used up”, it is just converted to a lower temperature If a civilization collects or generates energy, that energy must emerge at higher entropy (e.g. mid-infrared radiation) This approach is general: practically any energy use by a civilization should give a star (or galaxy) a MIR excess IRAS All-Sky map (1983) The discovery of infrared cirrus complicated Dyson sphere searches. Credit: NASA GSFC, LAMBDA Carrigan reported on the Fermilab Dyson Sphere search with IRAS: Lots of interesting red sources: -
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. -
Optical SETI: the All-Sky Survey
Professor van der Veen Project Scientist, UCSB Department of Physics, Experimental Cosmology Group class 4 [email protected] frequencies/wavelengths that get through the atmosphere The Planetary Society http://www.planetary.org/blogs/jason-davis/2017/20171025-seti-anybody-out-there.html THE ATMOSPHERE'S EFFECT ON ELECTROMAGNETIC RADIATION Earth's atmosphere prevents large chunks of the electromagnetic spectrum from reaching the ground, providing a natural limit on where ground-based observatories can search for SETI signals. Searching for technology that we have, or are close to having: Continuous radio searches Pulsed radio searches Targeted radio searches All-sky surveys Optical: Continuous laser and near IR searches Pulsed laser searches a hypothetical laser beacon watch now: https://www.youtube.com/watch?time_continue=41&v=zuvyhxORhkI Theoretical physicist Freeman Dyson’s “First Law of SETI Investigations:” Every search for alien civilizations should be planned to give interesting results even when no aliens are discovered. Interview with Carl Sagan from 1978: Start at 6:16 https://www.youtube.com/watch?v=g- Q8aZoWqF0&feature=youtu.be Anomalous signal recorded by Big Ear Telescope at Ohio State University. Big Ear was a flat, aluminum dish three football fields wide, with reflectors at both ends. Signal was at 1,420 MHz, the hydrogen 21 cm ‘spin flip’ line. http://www.bigear.org/Wow30th/wow30th.htm May 15, 2015 A Russian observatory reports a strong signal from a Sun-like star. Possibly from advanced alien civilization. The RATAN-600 radio telescope in Zelenchukskaya, at the northern foot of the Caucasus Mountains location: star HD 164595 G-type star (like our Sun) 94.35 ly away, visually located in constellation Hercules 1 planet that orbits it every 40 days unusual radio signal detected – 11 GHz (2.7 cm) claim: Signal from a Type II Kardashev civilization Only one observation Not confirmed by other telescopes Russian Academy of Sciences later retracted the claim that it was an ETI signal, stating the signal came from a military satellite. -
The Copernican Principle Rules out BLC1 As a Technological Radio Signal from the Alpha Centauri System
Draft version January 13, 2021 Typeset using LATEX twocolumn style in AASTeX62 The Copernican Principle Rules Out BLC1 as a Technological Radio Signal from the Alpha Centauri System Amir Siraj1 and Abraham Loeb1 1Department of Astronomy, Harvard University, 60 Garden Street, Cambridge, MA 02138, USA ABSTRACT Without evidence for occupying a special time or location, we should not assume that we inhabit privileged circumstances in the Universe. As a result, within the context of all Earth-like planets orbiting Sun-like stars, the origin of a technological civilization on Earth should be considered a single outcome of a random process. We show that in such a Copernican framework, which is inherently optimistic about the prevalence of life in the Universe, the likelihood of the nearest star system, Alpha Centauri, hosting a radio-transmitting civilization is ∼ 10−8. This rules out, a priori, Breakthrough Listen Candidate 1 (BLC1) as a technological radio signal from the Alpha Centauri system, as such a scenario would violate the Copernican principle by about eight orders of magnitude. We also show that the Copernican principle is consistent with the vast majority of Fast Radio Bursts being natural in origin. Keywords: technosignatures; astrobiology; search for extraterrestrial intelligence; biosignatures 1. INTRODUCTION lihood of searches for primitive and intelligent life, us- The Copernican principle asserts that we are not priv- ing a Drake-type approach. Westby & Conselice(2020) ileged observers of the Universe. Successes of its appli- applied the Copernican principle to the search for intel- cation include the rejection of Ptolemaic geocentrism ligent life, but in forms that featured strict boundaries and the adoption of the modern cosmological princi- in time, thereby not reflecting a truly random process. -
40Th Annual Meeting of the AAS Division for Planetary Sciences
40th Annual Meeting of the AAS Division for Planetary Sciences 10-15 October 2008 - Ithaca, New York, Statler Hotel, 130 Statler Drive, Ithaca, NY 14853 Friday, Saturday, Sunday, Monday, Tuesday, Wednesday, 10 October 11 October 12 October 13 October 14 October 15 October 8:00 Registration Park Atrium, Statler Hotel 8 am-4 pm Registration 8 am-noon 8:30- 1 Exoplanets I 20 Titan: Upper Atmosphere 50 Outer Planets II 59 Galilean Satellites 10:00 Statler Auditorium Statler Auditorium Statler Auditorium Statler Auditorium 2 Comets I 21 Planetary Rings: Theory 51 Mercury 60 Asteroid Composition DPS Members Meeting Statler Ballroom Statler Ballroom Statler Ballroom Statler Ballroom Statler Auditorium 3 Mars: Surface 22 MB Asteroids & Trojans 52 Asteroid Discovery & Orbits Uris Hall Uris Hall Uris Hall 10:00- Coffee Break Coffee Break Coffee Break Coffee Break Coffee Break 10:30 10:30- 4 Exoplanets II 23 Titan: Lower Atmosphere 34 Titan: Subsurface 53 Outer Planets III 61 Saturnian Satellites 12:00 Statler Auditorium Statler Auditorium Statler Auditorium Statler Auditorium Statler Auditorium 5 Comets II 24 Planetary Rings: Physical 35 Outer Planets I 54 Laboratory Research 62 Venus Statler Ballroom Statler Ballroom Statler Ballroom Statler Ballroom Statler Ballroom 6 Mars: Atmosphere 25 Near Earth Asteroids 36 Icy Dwarf Planets 55 Asteroid Evolution Uris Hall Uris Hall Uris Hall Uris Hall 12:00- Lunch Lunch Lunch Lunch 1:30 Meet the IAU NSF Town Hall DPS Women Green Conferencing Yale/Princeton Rooms Yale/Princeton Rooms Yale/Princeton Rooms Yale/Princeton Rooms 1:30- 7 Special Session 37 Special Session 56 Special Session 2:30 Dynamical Classification 26 Prize Lectures Exoplanets Mission Highlights of Planetary Bodies Kuiper Prize: Statler Auditorium Statler Auditorium All talks in any given session Statler Auditorium Michael F. -
Astrobiology and the Search for Life Beyond Earth in the Next Decade
Astrobiology and the Search for Life Beyond Earth in the Next Decade Statement of Dr. Andrew Siemion Berkeley SETI Research Center, University of California, Berkeley ASTRON − Netherlands Institute for Radio Astronomy, Dwingeloo, Netherlands Radboud University, Nijmegen, Netherlands to the Committee on Science, Space and Technology United States House of Representatives 114th United States Congress September 29, 2015 Chairman Smith, Ranking Member Johnson and Members of the Committee, thank you for the opportunity to testify today. Overview Nearly 14 billion years ago, our universe was born from a swirling quantum soup, in a spectacular and dynamic event known as the \big bang." After several hundred million years, the first stars lit up the cosmos, and many hundreds of millions of years later, the remnants of countless stellar explosions coalesced into the first planetary systems. Somehow, through a process still not understood, the laws of physics guiding the unfolding of our universe gave rise to self-replicating organisms − life. Yet more perplexing, this life eventually evolved a capacity to know its universe, to study it, and to question its own existence. Did this happen many times? If it did, how? If it didn't, why? SETI (Search for ExtraTerrestrial Intelligence) experiments seek to determine the dis- tribution of advanced life in the universe through detecting the presence of technology, usually by searching for electromagnetic emission from communication technology, but also by searching for evidence of large scale energy usage or interstellar propulsion. Technology is thus used as a proxy for intelligence − if an advanced technology exists, so to does the ad- vanced life that created it. -
GRAIL Twins Toast New Year from Lunar Orbit
Jet JANUARY Propulsion 2012 Laboratory VOLUME 42 NUMBER 1 GRAIL twins toast new year from Three-month ‘formation flying’ mission will By Mark Whalen lunar orbit study the moon from crust to core Above: The GRAIL team celebrates with cake and apple cider. Right: Celebrating said. “So it does take a lot of planning, a lot of test- the other spacecraft will accelerate towards that moun- GRAIL-A’s Jan. 1 lunar orbit insertion are, from left, Maria Zuber, GRAIL principal ing and then a lot of small maneuvers in order to get tain to measure it. The change in the distance between investigator, Massachusetts Institute of Technology; Charles Elachi, JPL director; ready to set up to get into this big maneuver when we the two is noted, from which gravity can be inferred. Jim Green, NASA director of planetary science. go into orbit around the moon.” One of the things that make GRAIL unique, Hoffman JPL’s Gravity Recovery and Interior Laboratory (GRAIL) A series of engine burns is planned to circularize said, is that it’s the first formation flying of two spacecraft mission celebrated the new year with successful main the twins’ orbit, reducing their orbital period to a little around any body other than Earth. “That’s one of the engine burns to place its twin spacecraft in a perfectly more than two hours before beginning the mission’s biggest challenges we have, and it’s what makes this an synchronized orbit around the moon. 82-day science phase. “If these all go as planned, we exciting mission,” he said. -
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. -
CASKAR: a CASPER Concept for the SKA Phase 1 Signal Processing Sub-System
CASKAR: A CASPER concept for the SKA phase 1 Signal Processing Sub-system Francois Kapp, SKA SA Outline • Background • Technical – Architecture – Power • Cost • Schedule • Challenges/Risks • Conclusions Background CASPER Technology MeerKAT Who is CASPER? • Berkeley Wireless Research Center • Nancay Observatory • UC Berkeley Radio Astronomy Lab • Oxford University Astrophysics • UC Berkeley Space Sciences Lab • Metsähovi Radio Observatory, Helsinki University of • Karoo Array Telescope / SKA - SA Technology • NRAO - Green Bank • New Jersey Institute of Technology • NRAO - Socorro • West Virginia University Department of Physics • Allen Telescope Array • University of Iowa Department of Astronomy and • MIT Haystack Observatory Physics • Harvard-Smithsonian Center for Astrophysics • Ohio State University Electroscience Lab • Caltech • Hong Kong University Department of Electrical and Electronic Engineering • Cornell University • Hartebeesthoek Radio Astronomy Observatory • NAIC - Arecibo Observatory • INAF - Istituto di Radioastronomia, Northern Cross • UC Berkeley - Leuschner Observatory Radiotelescope • Giant Metrewave Radio Telescope • University of Manchester, Jodrell Bank Centre for • Institute of Astronomy and Astrophysics, Academia Sinica Astrophysics • National Astronomical Observatories, Chinese Academy of • Submillimeter Array Sciences • NRAO - Tucson / University of Arizona Department of • CSIRO - Australia Telescope National Facility Astronomy • Parkes Observatory • Center for Astrophysics and Supercomputing, Swinburne University -
Summary Venus Exploration Analysis Group (VEXAG) Meeting #8 Thursday— September 2, 2010 Monona Terrace Convention Center, Madison, Wisconsin
Summary Venus Exploration Analysis Group (VEXAG) Meeting #8 Thursday— September 2, 2010 Monona Terrace Convention Center, Madison, Wisconsin Some 50 members of the Venus community met on Thursday—September 2, 2010 at the Monona Terrace Convention Center, Madison, Wisconsin. The goals of this meeting were to provide updates on the current and future Venus missions, on plans for completing the Next Decadal Survey, and on NASA plans for completing the current New Frontiers and Discovery Phase-A studies and proposals. Earlier in the week, VEXAG sponsored a very successful International Workshop on “Venus Our Closest Earth-like Planet: From Surface to Thermosphere - How does it work?” with significant international participation. Presentations at VEXAG Meeting #8 included: • A welcome and well-received report by Jim Green of NASA Headquarters on the status of NASA’s Planetary Science Program • A welcome and well-received report by Tibor Kremik of NASA Glenn Research Center on the status of NASA’s new Planetary Science Technology Panel • A welcome and well-received report by Ellen Stofan, Chair of the Inner Planets Panel on the current status of the Planetary Sciences Decadal Survey • Reports on the current status the European Venus Express, the Japanese Venus Climate Orbiter (Akatsuki), and Russian Venera missions • A report on VORTEX, the Venus In Situ Explorer Project, a student study by University of Alabama at Huntsville and College of Charleston • A report on NASA Goddard’s Venus Test Chamber There were eight open-microphone presentations covering diverse topics such as application of Stirling engines to Venus exploration, a prototype Venus seismometer, comparisons of Earth and Venus climate models, the possibility of measuring Venus rotation to improve both atmospheres and interior, use of Doppler lidar measurements to remotely sense Venus winds, the utility of magnetometers on Venus missions, observations from balloons, and a coordinated campaign for ground and spacecraft observations of Venus.