A Study of Scientific Literacy

Total Page:16

File Type:pdf, Size:1020Kb

A Study of Scientific Literacy Communicating astrobiology in public: A study of scientific literacy PhD thesis submitted for the requirements of Doctor of Philosophy, Science Communication AUSTRALIAN CENTRE FOR ASTROBIOLOGY DEPARTMENT OF BIOTECHNOLOGY AND BIOMOLECULAR SCIENCES Carol Ann Oliver Master of Science Communication Supervisors: Professor Malcolm Walter and Professor Paul Davies Associate supervisor: Professor Richard Dawkins June, 2008 i | Page Abstract The majority of adults in the US and in Europe appear to be scientifically illiterate. This has not changed in more than half a century. It is unknown whether the Australian public is also scientifically illiterate because no similar testing is done here. Public scientific illiteracy remains in spite of improvements in science education, innovative approaches to public outreach, the encouraging of science communication via the mass media, and the advent of the Internet. Why is it that there has been so little change? Is school science education inadequate? Does something happen between leaving high school education and becoming an adult? Does Australia suffer from the same apparent malady? The pilot study at the heart of this thesis tests a total of 692 Year Ten (16-year-old) Australian students across ten high schools and a first year university class in 2005 and 2006, using measures applied to adults. Twenty-six percent of those tested participated in a related scientific literacy project utilising in-person visits to Macquarie University in both years. A small group of the students (64) tested in 2005 were considered the best science students in seven of the ten high schools. Results indicate that no more than 20% of even the best high school science students - on the point of being able to end their formal science education - are scientifically literate if measured by adult standards. Another pilot test among 150 first year university students supports that indication. This compares to a scientific literacy rate of 28% for the US public. This thesis finds that the scientific literacy enterprise – in all its forms – fails scrutiny. Either we believe our best science students are leaving high school scientifically illiterate or there is something fundamentally wrong in our perceptions of public scientific illiteracy. This pilot study – probably the first of its kind – indicates we cannot rely on our current perceptions of a scientifically illiterate public. It demonstrates that a paradigm shift in our thinking is required about what scientific literacy is and in our expectations of a scientifically literate adult public. In the worst case scenario, governments are pouring millions of dollars into science education and public outreach with little or no basis for understanding whether either is effective. That is illogical, even irresponsible. It also impacts on the way astrobiology – or any science – is communicated in public. ii | Page Acknowledgements This work has been part of a longer personal journey, encouraged by my family, friends and colleagues who supported my desire to reach this goal and beyond. I would specifically like to thank my supervisors, Professor Malcolm Walter of the Australian Centre for Astrobiology at the University of New South Wales and Professor Paul Davies of the Beyond Center for Fundamental Concepts in Science at Arizona State University. They gracefully faced the challenge of a multiple relationship as student, colleague and friend. My thanks, too, to Professor Richard Dawkins of Oxford University who has maintained an open door whenever I visited the UK. Unless one lives on a desert island to undertake a PhD, the other stalwarts constantly there are family. My adult son James and adult daughter Gemma, my ex-husband Barry, my sister Shirley, her husband Sam, and my Mother have provided support throughout. Thank you does not seem enough to say. I wish my Father had survived to see me undertake this work. I know he would have been thrilled. I would also like to thank all my friends and colleagues for their advice and support. There are too many to mention, but I would like to make specific mention of Dr Seth Shostak and Edna DeVore of the SETI Institute in California, Jennifer Fergusson, Mikayla Keen, Eric Dalgliesh, and fellow students and colleagues at the Australian Centre for Astrobiology, in particular Associate Professor Simon George and Associate Professor Jeremy Bailey. I would like to thank, too, my friends and colleagues in NASA, at Arizona State University, and at the University of Glamorgan in Wales. Finally, and especially, I would like to thank Richard Dartt, who came into my life in 2008. He reminded me of why, at the age of 58, I wanted to complete this doctorate, and encouraged me to do so. Carol Oliver June, 2008 iii | Page iv | Page TABLE OF CONTENTS DECLARATION....................................................................................................... i ABSTRACT............................................................................................................. ii ACKNOWLEDGEMENTS....................................................................................... iii TABLE OF CONTENTS......................................................................................... v FRONT: “Look again at that dot. That’s here. That’s home. That’s us”.................. ix CHAPTER 1: THESIS OVERVIEW 1.1 Science and the public................................................................................... 1 1.2 Language of science...................................................................................... 7 1.3 Scientific literacy............................................................................................ 8 1.3.1 Scientific literacy and the public understanding of science.............. 10 1.3.2 What is meant by ‘general public audience’?................................... 12 1.3.3 Models in science communication.................................................... 13 1.3.4 Scientists communicating science.................................................... 14 1.3.5 Paucity of evidence.......................................................................... 18 1.3.6 Expectations and testing.................................................................. 20 1.4 Project aims and data collection..................................................................... 21 1.5 Project hypothesis.......................................................................................... 24 1.6 Alternative hypotheses................................................................................... 25 1.7 Related research questions............................................................................ 26 1.8 Title of the thesis............................................................................................ 27 CHAPTER 2: SCIENCE COMMUNICATION 2.1 Overview......................................................................................................... 31 2.2 Scientific literacy............................................................................................. 35 2.3 Communication within science communication.............................................. 45 2.4 Lessons from history...................................................................................... 50 2.5 Knowledge transfer........................................................................................ 52 2.6 The Internet: Moving goalposts or another game entirely?............................ 55 2.7 Courting disaster in a science-based society?............................................... 59 2.8 The 20% solution............................................................................................ 60 2.9 Summary........................................................................................................ 60 CHAPTER 3: SCIENTIFIC LITERACY AND SCIENCE EDUCATION 3.1 Overview........................................................................................................ 65 3.2 Correlations of education and adult scientific literacy.................................... 66 v | Page 3.3 International testing for student scientific literacy.......................................... 68 3.3.1 Differences between surveys........................................................... 68 3.3.2 TIMSS results................................................................................... 69 3.3.3 PISA 2006 results............................................................................. 70 3.3.4 Surveys vs. thesis hypothesis........................................................... 72 3.4 Summary........................................................................................................ 73 CHAPTER 4: THE PILBARA PROJECT 4.1 Overview........................................................................................................ 75 4.2 Relevance to the thesis.................................................................................. 79 4.3 Partnerships................................................................................................... 80 4.4 Design............................................................................................................ 81 4.5 Creating the Pilbara Virtual Field Trip............................................................ 81 4.6 Virtual environments in the classroom........................................................... 83 4.7 Testing and results........................................................................................
Recommended publications
  • Geobiology of the Late Paleoproterozoic Duck Creek Formation, Western Australia
    Precambrian Research 179 (2010) 135–149 Contents lists available at ScienceDirect Precambrian Research journal homepage: www.elsevier.com/locate/precamres Geobiology of the late Paleoproterozoic Duck Creek Formation, Western Australia Jonathan P. Wilson a,b,∗, Woodward W. Fischer b, David T. Johnston a, Andrew H. Knoll c, John P. Grotzinger b, Malcolm R. Walter e, Neal J. McNaughton i, Mel Simon d, John Abelson d, Daniel P. Schrag a, Roger Summons f, Abigail Allwood g, Miriam Andres h, Crystal Gammon b, Jessica Garvin j, Sky Rashby b, Maia Schweizer b, Wesley A. Watters f a Department of Earth and Planetary Sciences, Harvard University, USA b Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA c Department of Organismic and Evolutionary Biology, Harvard University, USA d The Agouron Institute, USA e Australian Centre for Astrobiology, University of New South Wales, Australia f Massachusetts Institute of Technology, USA g Jet Propulsion Laboratory, USA h Chevron Corp., USA i Curtin University of Technology, Australia j University of Washington, USA article info abstract Article history: The ca. 1.8 Ga Duck Creek Formation, Western Australia, preserves 1000 m of carbonates and minor Received 25 August 2009 iron formation that accumulated along a late Paleoproterozoic ocean margin. Two upward-deepening Received in revised form 12 February 2010 stratigraphic packages are preserved, each characterized by peritidal precipitates at the base and iron Accepted 15 February 2010 formation and carbonate turbidites in its upper part. Consistent with recent studies of Neoarchean basins, carbon isotope ratios of Duck Creek carbonates show no evidence for a strong isotopic depth gradient, but carbonate minerals in iron formations can be markedly depleted in 13C.
    [Show full text]
  • Westminsterresearch the Astrobiology Primer V2.0 Domagal-Goldman, S.D., Wright, K.E., Adamala, K., De La Rubia Leigh, A., Bond
    WestminsterResearch http://www.westminster.ac.uk/westminsterresearch The Astrobiology Primer v2.0 Domagal-Goldman, S.D., Wright, K.E., Adamala, K., de la Rubia Leigh, A., Bond, J., Dartnell, L., Goldman, A.D., Lynch, K., Naud, M.-E., Paulino-Lima, I.G., Kelsi, S., Walter-Antonio, M., Abrevaya, X.C., Anderson, R., Arney, G., Atri, D., Azúa-Bustos, A., Bowman, J.S., Brazelton, W.J., Brennecka, G.A., Carns, R., Chopra, A., Colangelo-Lillis, J., Crockett, C.J., DeMarines, J., Frank, E.A., Frantz, C., de la Fuente, E., Galante, D., Glass, J., Gleeson, D., Glein, C.R., Goldblatt, C., Horak, R., Horodyskyj, L., Kaçar, B., Kereszturi, A., Knowles, E., Mayeur, P., McGlynn, S., Miguel, Y., Montgomery, M., Neish, C., Noack, L., Rugheimer, S., Stüeken, E.E., Tamez-Hidalgo, P., Walker, S.I. and Wong, T. This is a copy of the final version of an article published in Astrobiology. August 2016, 16(8): 561-653. doi:10.1089/ast.2015.1460. It is available from the publisher at: https://doi.org/10.1089/ast.2015.1460 © Shawn D. Domagal-Goldman and Katherine E. Wright, et al., 2016; Published by Mary Ann Liebert, Inc. This Open Access article is distributed under the terms of the Creative Commons Attribution Noncommercial License (http://creativecommons.org/licenses/by- nc/4.0/) which permits any noncommercial use, distribution, and reproduction in any medium, provided the original author(s) and the source are credited. The WestminsterResearch online digital archive at the University of Westminster aims to make the research output of the University available to a wider audience.
    [Show full text]
  • Jet Propulsion Laboratory, Digital Converters
    Jet JUNE Propulsion 2014 Laboratory VOLUME 43 NUMBER 6 JPL 2025 What will JPL be like in 2025? What kind of missions will it be building and flying? How different will the lab be from the JPL of today? Those were the questions on the minds of Executive Council members in early May when they held their annual planning retreat. Over three days they laid out the broad strokes of strategies to make each of the lab’s major program areas robust a decade or more from now. “JPL is currently in good shape, but to remain that way we have to focus on where we are going across the next decade,” JPL Director Charles Elachi said follow- ing the off-site meeting. Among the strategies planned for JPL’s major units, in coming years the Solar System Exploration Director- ate hopes to create missions across a broad spectrum of scales—from flagships to miniature spacecraft. One major focus is to explore the ocean worlds in the outer solar system. The first step for this goal is to continue the development of what is hoped will be the next outer planet mission, Europa Clipper. Thanks to the power of NASA’s new Space Launch System, missions to the outer planets may become more frequent. JPL would also like to execute the first interplanetary mission using a pair of miniature cube- sat spacecraft. The Asteroid Redirect Mission in which JPL has a key role may serve as a model for future Clockwise: 1) Europa Clipper; 2) Mars; 3) Mars Sample Return lander; 4) solar system; 5) Earth satellites; 6) the pulsar planets PSR B1257+12 b, c, and d; 7) spiral closer collaborations with other NASA centers.
    [Show full text]
  • Mars 2020 Mission and NASA’S Mars Exploration Program, Visit: Mars.Nasa.Gov/Mars2020 September 2019 NASA Facts
    National Aeronautics and Space Administration Mars 2020 Over the past two decades, missions flown to benefit future robotic and human exploration by NASA’s Mars Exploration Program have of Mars. shown us that Mars was once very different from the cold, dry planet it is today. Evidence Key Objectives discovered by landed and orbital missions point • Explore a geologically diverse landing site to wet conditions billions of years ago. These environments lasted long enough to potentially • Assess ancient habitability support the development of microbial life. • Seek signs of ancient life, particularly in special rocks known to preserve signs of life over time The Mars 2020 rover is designed to better understand the geology of Mars and seek signs of • Gather rock and soil samples that could be ancient life. The mission will collect and store a set returned to Earth by a future NASA mission of rock and soil samples that could be returned to • Demonstrate technology for future robotic and Earth in the future. It will also test new technology human exploration Mission Timeline Key Hardware • Launch in July-August 2020 from Cape The rover will carry seven instruments to conduct Canaveral Air Force Station, Florida unprecedented science and test new technology • Launching on a ULA Atlas 541 procured under on the Red Planet. They are: NASA’s Launch Services Program • Mastcam-Z, an advanced camera system with • Land on Mars on February 18, 2021 at the panoramic and stereoscopic imaging capability site of an ancient river delta in a lake that once with the ability to zoom. The instrument also filled Jezero Crater will determine mineralogy of the Martian surface and assist with rover operations.
    [Show full text]
  • PIXL Seminar, Nov 2015 Why Micro XRF?
    Silicon drift detector response function to hard x-rays (with an introduction on quantitative MicroXRF And the Planetary Instrument for X-ray Lithochemistry) Nicolas Michel-Hart with special thanks to Tim Elam for project guidance Applied Physics Laboratory – University of Washington X-ray Fluorescence and μXRF http://in.niton.com/en/ https://xos.com/technologies/xrf/ https://en.wikipedia.org/wiki/X-ray_fluorescence#/media/File:XRFScan.jpg Elam, PIXL Seminar, Nov 2015 Why Micro XRF? Biosignatures (ooids) hosted in a 2.7 billion-year-old carbonate rock Elam, PIXL Seminar, Nov 2015 Some pixels can be very different Area of element maps Visible light image Recent microbialite from the Death Valley Area Elam, PIXL Seminar, Nov 2015 Mars 2020 Mission • M2020 Science Objectives – Habitability: Characterize the geologic record for astrobiologically relevant environments and geologic diversity – Biosignatures: Search for materials with high biosignature preservation potential – Sample Caching: Obtain a pristine set of geologically diverse samples and cache for future return to Earth – Prepare for Humans: Demonstrate in situ resource utilization technologies and characterize dust size and morphology • Mission life: 1.5 Mars years/1005 Martian days • Flight Instruments delivered by Fall 2018, Launch July 2020, Land February 2021 • Instrument Complement: – Mastcam-Z and Supercam for panoramic/stereo imaging and chemical analysis – MEDA for weather – RIMFAX ground penetrating radar – MOXIE technology experiment to produce Oxygen from CO2 – SHERLOC
    [Show full text]
  • The Detection of Long-Chain Bio-Markers Using Atomic Force Microscopy
    applied sciences Article The Detection of Long-Chain Bio-Markers Using Atomic Force Microscopy Mark S. Anderson Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA 91109, USA; [email protected]; Tel.: +1-818-354-3278 Received: 15 February 2019; Accepted: 22 March 2019; Published: 27 March 2019 Abstract: The detection of long-chain biomolecules on mineral surfaces is presented using an atomic force microscope (AFM). This is achieved by using the AFM’s ability to manipulate molecules and measure forces at the pico-newton scale. We show that a highly characteristic force-distance signal is produced when the AFM tip is used to detach long-chain molecules from a surface. This AFM force spectroscopy method is demonstrated on bio-films, spores, fossils and mineral surfaces. The method works with AFM imaging and correlated tip enhanced infrared spectroscopy. The use of AFM force spectroscopy to detect this class of long chain bio-markers has applications in paleontology, life detection and planetary science. Keywords: long-chain bio-markers 2; AFM 3; tip enhanced spectroscopy 1. Introduction Scanning probe microscopes are fundamental tools in microscopy and nanotechnology. The most widely utilized of the probe microscopes is the atomic force microscope (AFM) that was first described in 1986 by Binnig, Gerber and Quate [1]. With an AFM, a tip mounted on a micro-fabricated cantilever is scanned over the surface and the interaction between the tip and the substrate is detected by monitoring the deflection of the cantilever [2]. These microscopes are remarkable for their ability to image individual atoms or molecules.
    [Show full text]
  • The Breakthrough Listen Search for Intelligent Life: Observations of 1327 Nearby Stars Over 1.10–3.45 Ghz Submitted to Apj
    Draft version June 17, 2019 Typeset using LATEX twocolumn style in AASTeX62 The Breakthrough Listen Search for Intelligent Life: Observations of 1327 Nearby Stars over 1.10{3.45 GHz Danny C. Price,1, 2 J. Emilio Enriquez,1, 3 Bryan Brzycki,1 Steve Croft,1 Daniel Czech,1 David DeBoer,1 Julia DeMarines,1 Griffin Foster,1, 4 Vishal Gajjar,1 Nectaria Gizani,1, 5 Greg Hellbourg,1 Howard Isaacson,1, 6 Brian Lacki,7 Matt Lebofsky,1 David H. E. MacMahon,1 Imke de Pater,1 Andrew P. V. Siemion,1, 8, 3, 9 Dan Werthimer,1 James A. Green,10 Jane F. Kaczmarek,10 Ronald J. Maddalena,11 Stacy Mader,10 Jamie Drew,12 and S. Pete Worden12 1Department of Astronomy, University of California Berkeley, Berkeley CA 94720 2Centre for Astrophysics & Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia 3Department of Astrophysics/IMAPP,Radboud University, Nijmegen, Netherlands 4Astronomy Department, University of Oxford, Keble Rd, Oxford, OX13RH, United Kingdom 5Hellenic Open University, School of Science & Technology, Parodos Aristotelous, Perivola Patron, Greece 6University of Southern Queensland, Toowoomba, QLD 4350, Australia 7Breakthrough Listen, Department of Astronomy, University of California Berkeley, Berkeley CA 94720 8SETI Institute, Mountain View, California 9University of Malta, Institute of Space Sciences and Astronomy 10Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 1710, Australia 11Green Bank Observatory, West Virginia, 24944, USA 12The Breakthrough Initiatives, NASA Research Park, Bld. 18, Moffett Field, CA, 94035, USA (Received June 17, 2019; Revised June 17, 2019; Accepted XXX) Submitted to ApJ ABSTRACT Breakthrough Listen (BL) is a ten-year initiative to search for signatures of technologically capable life beyond Earth via radio and optical observations of the local Universe.
    [Show full text]
  • NASA Announces Mars 2020 Rover Payload to Explore the Red Planet As Never Before - 2020 Mission Plans
    mars.jpl.nasa.gov NASA Announces Mars 2020 Rover Payload to Explore the Red Planet as Never Before - 2020 Mission Plans 5 min read• original Payload for NASA's Mars 2020 Rover This diagram shows the science instruments for NASA's Mars 2020 rover mission. Credit: NASA Planning for NASA's 2020 Mars rover envisions a basic structure that capitalizes on the design and engineering work done for the NASA rover Curiosity, which landed on Mars in 2012, but with new science instruments selected through competition for accomplishing different science objectives. Credit: NASA/JPL-Caltech The next rover NASA will send to Mars in 2020 will carry seven carefully-selected instruments to conduct unprecedented science and exploration technology investigations on the Red Planet. NASA announced the selected Mars 2020 rover instruments Thursday at the agency's headquarters in Washington. Managers made the selections out of 58 proposals received in January from researchers and engineers worldwide. Proposals received were twice the usual number submitted for instrument competitions in the recent past. This is an indicator of the extraordinary interest by the science community in the exploration of the Mars. The selected proposals have a total value of approximately $130 million for development of the instruments. The Mars 2020 mission will be based on the design of the highly successful Mars Science Laboratory rover, Curiosity, which landed almost two years ago, and currently is operating on Mars. The new rover will carry more sophisticated, upgraded hardware and new instruments to conduct geological assessments of the rover's landing site, determine the potential habitability of the environment, and directly search for signs of ancient Martian life.
    [Show full text]
  • Diverse Microstructures from Archaean Chert from the Mount
    Precambrian Research 158 (2007) 228–262 Diverse microstructures from Archaean chert from the Mount Goldsworthy–Mount Grant area, Pilbara Craton, Western Australia: Microfossils, dubiofossils, or pseudofossils? Kenichiro Sugitani a,∗, Kathleen Grey b,c, Abigail Allwood c,1, Tsutomu Nagaoka d, Koichi Mimura e, Masayo Minami f, Craig P. Marshall c,g, Martin J. Van Kranendonk b,c, Malcolm R. Walter c a Department of Environmental Engineering and Architecture, Graduate School of Environmental Studies, Nagoya University, Nagoya 464-8601, Japan b Geological Survey of Western Australia, Department of Industry and Resources, 100 Plain Street, East Perth, WA 6004, Australia c Australian Centre for Astrobiology, Macquarie University, Sydney, NSW 2109, Australia d School of Informatics and Sciences, Nagoya University, Nagoya 464-8601, Japan e Department of Earth and Environmental Sciences, Graduate School of Environmental Studies, Nagoya University, Nagoya 464-8601, Japan f Nagoya University Center for Chronological Research, Nagoya 464-8602, Japan g School of Chemistry, The University of Sydney, Sydney, NSW 2006, Australia Received 7 February 2007; received in revised form 16 March 2007; accepted 16 March 2007 Abstract A diverse assemblage of indigenous carbonaceous microstructures, classified here as highly probable microfossils to pseudomi- crofossils, is present in the >ca. 2.97 Ga Farrel Quartzite (Gorge Creek Group) at Mount Grant and Mount Goldsworthy, Pilbara Craton, Western Australia. The microstructures are an integral part of the primary sedimentary fabrics preserved in black chert beds. The interbedding of chert with layers of large silicified crystal pseudomorphs and fine to coarse grained volcaniclastic/clastic beds indicate deposition in a partially evaporitic basin with terrigenous clastic and volcaniclastic input.
    [Show full text]
  • Machine Learning in Astronomy: a Workman’S Manual
    EBOOK-ASTROINFORMATICS SERIES MACHINE LEARNING IN ASTRONOMY: A WORKMAN’S MANUAL November 23, 2017 Snehanshu Saha, Kakoli Bora, Suryoday Basak, Gowri Srinivasa, Margarita Safonova, Jayant Murthy and Surbhi Agrawal PESIT South Campus Indian Institute of Astrophysics, Bangalore M. P.Birla Institute of Fundamental Research, Bangalore 1 Preface The E-book is dedicated to the new field of Astroinformatics: an interdisciplinary area of research where astronomers, mathematicians and computer scientists collaborate to solve problems in astronomy through the application of techniques developed in data science. Classical problems in astronomy now involve the accumulation of large volumes of complex data with different formats and characteristic and cannot now be addressed using classical techniques. As a result, machine learning algorithms and data analytic techniques have exploded in importance, often without a mature understanding of the pitfalls in such studies. The E-book aims to capture the baseline, set the tempo for future research in India and abroad and prepare a scholastic primer that would serve as a standard document for future research. The E-book should serve as a primer for young astronomers willing to apply ML in astronomy, a way that could rightfully be called "Machine Learning Done Right" borrowing the phrase from Sheldon Axler ((Linear Algebra Done Right)! The motivation of this handbook has two specific objectives: • develop efficient models for complex computer experiments and data analytic tech- niques which can be used in astronomical data analysis in short term and various related branches in physical, statistical, computational sciences much later (larger goal as far as memetic algorithm is concerned). • develop a set of fundamentally correct thumb rules and experiments, backed by solid mathematical theory and render the marriage of astronomy and Machine Learning stability and far reaching impact.
    [Show full text]
  • Research Scientist and Principle Investigator NASA Dr Abigail Allwood
    Research Scientist and Principle Investigator NASA Dr Abigail Allwood What do you work in and what is your specialty? My research at the NASA Jet Propulsion Laboratory focuses on earliest evidence of life on Earth, the nature of earliest terrestrial biota and ecosystems, morphological biosignatures, developing methods and approaches to biosignature detection on Mars, Mars Sample Return science, planetary instrument development, and life detection evaluation in returned samples. I am also the Principle Investigator for the NASA Mars 2020 Rover Mission. How did you become interested in this area and when did you first start? I was drawn to Earth Science by the opportunities it presented to go outdoors and do lots of field work. It was quite an amazing feeling as an Earth Scientist to be able to go to a place where there are outcrops of rock and look deep into Earth’s past and understand what was going on millions or even billions of years ago. I liken it to reading the pages of a book; the layers of the rock record, and I feel it gives you a sense of perspective on your own life today. What study path have you taken to get here? I came to work at NASA as an Earth Scientist by a very circuitous route. I first studied the Bachelor of Science majoring in Earth Science, at QUT. The skills gained from the very practical and hands-on nature of the degree undoubtedly carried me through my career to where I am today. As I came towards the end of my degree I originally thought I was going to go into the oil or mining industry.
    [Show full text]
  • 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).
    [Show full text]