Science Teachers Taketo Thestage

Total Page:16

File Type:pdf, Size:1020Kb

Science Teachers Taketo Thestage titel_SiS_Issue19RZ:scienceinschool 27.05.2011 18:49 Uhr Seite 1 How many schools Summer 2011 Issue19 and teachers do you reach – worldwide? In this issue: A planet from another galaxy Also: Science teachers taketo thestage Advertising in Science in School · Choose between advertising in the quarterly print journal or on our website. · Website: reach over 30 000 science educators worldwide – every month. · In print: target up to 15 000 European science educators every quarter, including over 3300 named subscribers. · Distribute your flyers, brochures, CD-ROMs or other materials either to over 3300 named subscribers or to all recipients of the print copies. For more details, see www.scienceinschool.org/advertising Published by EIROforum: ISSN: 1818-0353 Initially supported by the European Union: Subscribe (free in Europe): www.scienceinschool.org Highlighting the best in science teaching and research About Science in School Science in School promotes inspiring science teaching by encouraging communication between Editorial teachers, scientists and everyone else involved in European science education. The journal addresses science teaching both across Europe and across disciplines: highlighting the best in teaching and cutting-edge research. It covers not only biology, physics and chemistry, ife in space – scientists and lay people alike but also earth sciences, engineering and medicine, focusing on interdisciplinary work. are intrigued by this possibility. Recently, The contents include teaching materials; cutting- edge science; interviews with young scientists astronomers have found a planet orbiting and inspiring teachers; reviews of books and other L resources; and European events for teachers and a star that entered the Milky Way from another schools. galaxy (see page 26). Does that whet your appetite Science in School is published quarterly, both online and in print. The website is freely available, with for space travel? Why not discuss what we would articles in many European languages. The English- language print version is distributed free of charge need to live on another planetary body and get your within Europe. students to design a space habitat (see page 43)? Contact us Dr Eleanor Hayes / Dr Marlene Rau One of the many considerations for this activity is cosmic radiation – Science in School European Molecular Biology Laboratory high-energy particles that fall on Earth and other planets from space. Meyerhofstrasse 1 69117 Heidelberg One type of particle produced by cosmic rays is the neutrino; as Susana Germany Cebrián explains, thousands of them pass through your body in the time [email protected] Subscriptions it takes you to read these lines (see page 55). Register online to: · Receive an email alert when each issue is published Whereas huge detectors are necessary to find neutrinos, UK physics · Request a free print subscription (within Europe) · Swap ideas with teachers and scientists in the teacher Becky Parker and her students use tiny detectors to find other Science in School online forum cosmic particles – doing real science at school, with help from CERN. · Post comments on articles in Science in School. Submissions Learn more about the project and how to join on page 69. We welcome articles submitted by scientists, teachers and others interested in European science education. Another inspiring science teacher, Bernhard Sturm, introduced his See the author guidelines on our website. students to the chemistry of amber (see page 36). This fossilised resin is Referee panel Before publication, Science in School articles are also analysed by palaeontologists at the European Synchrotron Radiation reviewed by European science teachers to check that Facility, where their chemist colleagues have recently revealed why the they are suitable for publication. If you would like to join our panel of referees, please read the guidelines famously bright yellows of van Gogh’s paintings are darkening over time on our website. (see page 19). The culprit is thought to be a chemical reaction initiated Book reviewers If you teach science in Europe and would like to by light. review books or other resources for Science in School, please read the guidelines on our website. Reverse this process and, as Emma Welsh explains, the result is Translators We offer articles online in many European languages. chemiluminescence: the production of light from a chemical reaction If you would like to volunteer to translate articles into (see page 62). One of the applications of chemiluminescence is the your own language, please read the guidelines for translators on our website. detection of blood at crime scenes using luminol. Forensic scientists, however, perform not only chemical but also genetic analyses, such as Advertising in Science in School – new lower prices DNA fingerprinting. Using this method, your students can solve a murder Science in School is the only European journal aimed at secondary-school science teachers across Europe mystery in the Gene Jury team’s DNA detective game (see page 30). and across the full spectrum of sciences. It is freely available online, and 15 000 full-colour printed If that sounds too lurid, you may prefer the Moja Island role play, to copies are distributed each quarter. The readership of Science in School includes determine the best sustainable energy solutions for fictitious island everyone involved in European science teaching, communities (see page 50). including: · Secondary-school science teachers · Scientists Is background reading what you are looking for, rather than games? Then · Primary-school teachers you may be interested in Laurence Reed and Jackie de Belleroche’s report · Teacher trainers · Science communicators. on the latest research into schizophrenia (see page 13), Andrew Wildes’ Web advertisements description of his life as a neutron scientist at the Institut Laue-Langevin Reach over 30 000 science educators worldwide every month. (see page 10), or one of the book or website reviews by our readers. You · € 200-350 per week can find all these articles and more on the Science in School website Print advertisements Reach over 15 000 readers per issue. (www.scienceinschool.org). · Full page: € 1495 · Half page: € 999 Marlene Rau · Quarter page: € 560 · Back cover (full page): € 1995 Editor of Science in School Distribution [email protected] Distribute flyers, DVDs or other materials to 3000 named subscribers or to all 15 000 print recipients. www.scienceinschool.org For more information, see www.scienceinschool.org/advertising or contact [email protected] i I Science in School I Issue 19 : Summer 2011 www.scienceinschool.org Contents Image courtesy of Vlue / iStockphoto i Editorial News from the EIROs 2 Rockets, genomes and particle accelerators Event 6 Science teachers take to the stage Feature article 13 10 Life in the line of fire Image courtesy of the Van Gogh Museum, Amsterdam Cutting-edge science 13 Investigating the causes of schizophrenia 19 Van Gogh’s darkening legacy 26 A planet from another galaxy Teaching activities 30 The DNA detective game 36 Amber: an introduction to organic chemistry 19 Science education projects 43 Building a space habitat in the classroom Image courtesy of dtimiraos / iStockphoto 50 Moja Island: learning about renewable energy sources Science topics 55 Neutrinos: an introduction 62 What is chemiluminescence? Teacher profile 69 Schoolhouse scientists 30 Image courtesy of NASA Additional online material Reviews Exploring the Mystery of Matter: The ATLAS Experiment Ask a Biologist website 2010-2011 State of the Wild: A Global Portrait Forthcoming events for schools: www.scienceinschool.org/events To read the whole issue, see: www.scienceinschool.org/2011/issue19 43 At the end of each article in this issue, you may notice a square black and white pattern. With the aid of a smart phone, this QR code will lead you straight to the online version of the article. All you need to do is download a free QR code reader app (such as BeeTagg or i-Nigma) for your smart phone and scan the code with your phone’s camera. To find a suitable one for your phone, see: http://tinyurl.com/byk4wg Hint: the apps works better in good light conditions, and with a steady hand. You may also want to try holding your camera at different distances from the code. You can then use all the live links to the references and resources, download the PDF, send the article to your friends, leave comments, and much more. What do you think about this new feature? Does it work for you? Leave your feedback here: www.scienceinschool.org/QRfeedback Image courtesy of Kamioka Observatory, 55 ICRR (Institute for Cosmic Ray Research), www.scienceinschool.org Science in School I Issue 19 : Summer 2011 I 1 The University of Tokyo The permanent exhibition ‘The Universe of particles’ at CERN Rockets, genomes and particle accelerators N ER / C lut ngb el Ju cha f Mi sy o urte e co Imag Science in School is published by EIROforum, a collaboration of research organisations. Eleanor Hayes, Editor-in-Chief of Science in School, reviews some of the latest news from the EIROforum members. mous particle accelerators, beams of CERN: visit the world’s largest neutrons or high-energy X-rays, large particle physics laboratory telescopes or the International Space In 2010, a stunning 58 000 people Station. visited CERN in Geneva, Switzerland. Whether individually or as part of The permanent exhibition entitled EIROforum, the EIROs are also in- ‘The Universe of particles’ attracts EIROforum volved in many outreach and educa- many visitors, offering them an over- IROforum, the publisher of Sci- tion activities – for school students, view of CERN’s research goals, tools ence in School, is a partnership teachers and the general public. Sci- and impact throughout the world. of eight European inter-govern- ence in School is one example of a joint After that, many visitors go on to find Emental scientific research organisa- EIROforum activity; this article details out more about the research at CERN, tions (EIROs).
Recommended publications
  • Catholic Christian Christian
    Religious Scientists (From the Vatican Observatory Website) https://www.vofoundation.org/faith-and-science/religious-scientists/ Many scientists are religious people—men and women of faith—believers in God. This section features some of the religious scientists who appear in different entries on these Faith and Science pages. Some of these scientists are well-known, others less so. Many are Catholic, many are not. Most are Christian, but some are not. Some of these scientists of faith have lived saintly lives. Many scientists who are faith-full tend to describe science as an effort to understand the works of God and thus to grow closer to God. Quite a few describe their work in science almost as a duty they have to seek to improve the lives of their fellow human beings through greater understanding of the world around them. But the people featured here are featured because they are scientists, not because they are saints (even when they are, in fact, saints). Scientists tend to be creative, independent-minded and confident of their ideas. We also maintain a longer listing of scientists of faith who may or may not be discussed on these Faith and Science pages—click here for that listing. Agnesi, Maria Gaetana (1718-1799) Catholic Christian A child prodigy who obtained education and acclaim for her abilities in math and physics, as well as support from Pope Benedict XIV, Agnesi would write an early calculus textbook. She later abandoned her work in mathematics and physics and chose a life of service to those in need. Click here for Vatican Observatory Faith and Science entries about Maria Gaetana Agnesi.
    [Show full text]
  • Contents #110 1
    Contents #110 1. Contents 2. Editorial #110 3. In this issue 4. Education News and Views 7. Good Practical Science John Holman 8. Irish Success at the International Chemistry Olympiad Odilla Finlayson 10. ARTIST - Action Research To Innovate Science Teaching Sarah Hayes, Peter Childs and Aimee Stapleton 12. Chemists you should know: #2 Niels Bohr – into atomic orbits Adrian J. Ryder 15. Classical Chemical Quotations #8 Niels Bohr 16. The world’s largest crystal model Robert Krickl 19. Teaching science in the USA Emma Ryan 23. Science Integration as a Precursor to Effective STEM education Miriam Hamilton 28. How does it work? The chemistry of the brown ring test for nitrate ions 30. TEMI idea: The amazing polydensity bottle 31. TEMI idea: The mystery of the disappearing precipitate 34. Zippie Chemistry Enda Carr 38. Places to visit Glengowla Mines, Co. Galway 40. Diary 41. Lithium the light metal powering the future – from brines to batteries ` Conference Reports 46. 10 th IViCE, Irish Variety in Chemistry Education Claire McDonnell 48. Science on Stage Europe Enda Carr 49. 11 th Chemistry Demonstration Workshop 51. 6th Annual BASF Summer School for Chemistry Teachers Declan Kennedy 53. 7th Eurovariety in University Chemistry Teaching Peter E. Childs 56. ESERA 2017 Peter E. Childs 58. Science at the National Ploughing Championships 2017 Aimee Stapleton, Martin McHugh, Sarah Hayes 60. Chemlingo: what’s in a name – nitre or natron? Peter E. Childs 61. The danger of cherry stones 62. The two faces of rubber 64. Information page Disclaimer The views expressed in Chemistry in Action! are those of the authors and the Editor is not responsible for any views expressed.
    [Show full text]
  • Melvin Schwartz 1932-2006
    MELVIN SCHWARTZ 1932-2006 A Biographical Memoir by N. P. SAMIOS AND P. YAMIN © 2012 The National Academy of Sciences Any opinions expressed in this memoir are those of the authors and do not necessarily reflect the views of the National Academy of Sciences. MELVIN SCHWARTZ Courtesy of Brookhaven National Laboratories. November 2, 1932–August 28, 2006 BY N. P. SAMIOS AND P. YAMIN MEL SCHWARTZ DIED ON August 28, 2006, in Twin Falls, Idaho. He was born on 1 November 2, 1932, in New York City. He grew up in the Great Depression, but with a sense of optimism and desire to use his mind for the betterment of human- kind. He entered the Bronx High School of Science in the fall of 1945. It was there that his interest in physics began and that he recognized the importance of interactions with peers in determining his sense of direction in life. One of his classmates and future colleagues recalled that “even then” he wanted a Nobel Prize. Mel noted: My interest in physics began at the age of 12 when I entered the Bronx High School of Science. The four years I spent there were certainly among the most exciting and stimulating in my life, mostly because of the interaction with the other students of similar background, interest, and ability. MELVIN SCHWARTZ MELVIN On Sunday afternoons he attended a school run by the secular and Zionist Yiddish and many others. As Mel commented, “This faculty [was] at this time unmatched by any in the world, largely Nationaler Arbeter Farband (Jewish National Workers Alliance).
    [Show full text]
  • 01Ii Beam Line
    STA N FO RD LIN EA R A C C ELERA TO R C EN TER Fall 2001, Vol. 31, No. 3 CONTENTS A PERIODICAL OF PARTICLE PHYSICS FALL 2001 VOL. 31, NUMBER 3 Guest Editor MICHAEL RIORDAN Editors RENE DONALDSON, BILL KIRK Contributing Editors GORDON FRASER JUDY JACKSON, AKIHIRO MAKI MICHAEL RIORDAN, PEDRO WALOSCHEK Editorial Advisory Board PATRICIA BURCHAT, DAVID BURKE LANCE DIXON, EDWARD HARTOUNI ABRAHAM SEIDEN, GEORGE SMOOT HERMAN WINICK Illustrations TERRY ANDERSON Distribution CRYSTAL TILGHMAN The Beam Line is published quarterly by the Stanford Linear Accelerator Center, Box 4349, Stanford, CA 94309. Telephone: (650) 926-2585. EMAIL: [email protected] FAX: (650) 926-4500 Issues of the Beam Line are accessible electroni- cally on the World Wide Web at http://www.slac. stanford.edu/pubs/beamline. SLAC is operated by Stanford University under contract with the U.S. Department of Energy. The opinions of the authors do not necessarily reflect the policies of the Stanford Linear Accelerator Center. Cover: The Sudbury Neutrino Observatory detects neutrinos from the sun. This interior view from beneath the detector shows the acrylic vessel containing 1000 tons of heavy water, surrounded by photomultiplier tubes. (Courtesy SNO Collaboration) Printed on recycled paper 2 FOREWORD 32 THE ENIGMATIC WORLD David O. Caldwell OF NEUTRINOS Trying to discern the patterns of neutrino masses and mixing. FEATURES Boris Kayser 42 THE K2K NEUTRINO 4 PAULI’S GHOST EXPERIMENT A seventy-year saga of the conception The world’s first long-baseline and discovery of neutrinos. neutrino experiment is beginning Michael Riordan to produce results. Koichiro Nishikawa & Jeffrey Wilkes 15 MINING SUNSHINE The first results from the Sudbury 50 WHATEVER HAPPENED Neutrino Observatory reveal TO HOT DARK MATTER? the “missing” solar neutrinos.
    [Show full text]
  • Glossary of Terms Absorption Line a Dark Line at a Particular Wavelength Superimposed Upon a Bright, Continuous Spectrum
    Glossary of terms absorption line A dark line at a particular wavelength superimposed upon a bright, continuous spectrum. Such a spectral line can be formed when electromag- netic radiation, while travelling on its way to an observer, meets a substance; if that substance can absorb energy at that particular wavelength then the observer sees an absorption line. Compare with emission line. accretion disk A disk of gas or dust orbiting a massive object such as a star, a stellar-mass black hole or an active galactic nucleus. An accretion disk plays an important role in the formation of a planetary system around a young star. An accretion disk around a supermassive black hole is thought to be the key mecha- nism powering an active galactic nucleus. active galactic nucleus (agn) A compact region at the center of a galaxy that emits vast amounts of electromagnetic radiation and fast-moving jets of particles; an agn can outshine the rest of the galaxy despite being hardly larger in volume than the Solar System. Various classes of agn exist, including quasars and Seyfert galaxies, but in each case the energy is believed to be generated as matter accretes onto a supermassive black hole. adaptive optics A technique used by large ground-based optical telescopes to remove the blurring affects caused by Earth’s atmosphere. Light from a guide star is used as a calibration source; a complicated system of software and hardware then deforms a small mirror to correct for atmospheric distortions. The mirror shape changes more quickly than the atmosphere itself fluctuates.
    [Show full text]
  • Foundation Document Manhattan Project National Historical Park Tennessee, New Mexico, Washington January 2017 Foundation Document
    NATIONAL PARK SERVICE • U.S. DEPARTMENT OF THE INTERIOR Foundation Document Manhattan Project National Historical Park Tennessee, New Mexico, Washington January 2017 Foundation Document MANHATTAN PROJECT NATIONAL HISTORICAL PARK Hanford Washington ! Los Alamos Oak Ridge New Mexico Tennessee ! ! North 0 700 Kilometers 0 700 Miles More detailed maps of each park location are provided in Appendix E. Manhattan Project National Historical Park Contents Mission of the National Park Service 1 Mission of the Department of Energy 2 Introduction 3 Part 1: Core Components 4 Brief Description of the Park. 4 Oak Ridge, Tennessee. 5 Los Alamos, New Mexico . 6 Hanford, Washington. 7 Park Management . 8 Visitor Access. 8 Brief History of the Manhattan Project . 8 Introduction . 8 Neutrons, Fission, and Chain Reactions . 8 The Atomic Bomb and the Manhattan Project . 9 Bomb Design . 11 The Trinity Test . 11 Hiroshima and Nagasaki, Japan . 12 From the Second World War to the Cold War. 13 Legacy . 14 Park Purpose . 15 Park Signifcance . 16 Fundamental Resources and Values . 18 Related Resources . 22 Interpretive Themes . 26 Part 2: Dynamic Components 27 Special Mandates and Administrative Commitments . 27 Special Mandates . 27 Administrative Commitments . 27 Assessment of Planning and Data Needs . 28 Analysis of Fundamental Resources and Values . 28 Identifcation of Key Issues and Associated Planning and Data Needs . 28 Planning and Data Needs . 31 Part 3: Contributors 36 Appendixes 38 Appendix A: Enabling Legislation for Manhattan Project National Historical Park. 38 Appendix B: Inventory of Administrative Commitments . 43 Appendix C: Fundamental Resources and Values Analysis Tables. 48 Appendix D: Traditionally Associated Tribes . 87 Appendix E: Department of Energy Sites within Manhattan Project National Historical Park .
    [Show full text]
  • Sc Ence Celebrating the Neutrino Number 25 1997
    Los Alamos Sc ence Celebrating the Neutrino Number 25 1997 Celebrating the Neutrino . .1 The Evidence for Oscillations . .116 Bill Louis, Vern Sandberg, Gerry Garvey, Hywel White, Geoffrey Mills, and Rex Tayloe Reines-Cowan Experiments—Detecting the Poltergeist . .4 Neutrino oscillations are invoked as the explanation in experiments with solar, atmospheric, and accelerator- A compilation of papers and notes by Fred Reines and Clyde Cowan, Jr. produced (LSND) neutrinos. This summary of the experimental results for mixing angles and neutrino masses includes an interesting model that makes all three data sets consistent. The neutrino’s existence was inferred by Wolfgang Pauli in 1930, who feared that his clever construct might elude detection forever. Twenty-five years later, Fred Reines, Clyde Cowan, Jr., and a Los Alamos team detected the evasive particle. Their dedication to the chase and their innovative detection techniques set The Nature of Neutrinos in Muon Decay and Physics Beyond the Standard Model . .128 a precedent for all future neutrino experiments. Peter Herczeg Beta Decay and the Missing Energy . .7 Experiments that search for electron antineutrinos from m1-decay are sensitive not only to neutrino oscillations Fermi’s Theory of Beta Decay and Neutrino Processes . .8 but also to a class of muon decays that require leptonic interactions not present in the Standard Model. The author explores whether such decays could explain the observed excess of e1 events in the LSND experiments. The Oscillating Neutrino—An Introduction to Neutrino Masses and Mixing . .28 Exorcising Ghosts—In Pursuit of the Missing Solar Neutrinos . .136 Richard Slansky, Stuart Raby, Terry Goldman, and Gerry Garvey as told to Necia Grant Cooper Andrew Hime Today, the neutrino is at the center of particle physics as experimenters around the world explore the possibility that this tiny particle changes its identity just by moving between two points.
    [Show full text]
  • David Featonby “Retired” from School Physics Teaching After 35 Years in the Classroom, Working Successfully with Pupils of A
    David Featonby “retired” from school physics teaching after 35 years in the classroom, working successfully with pupils of all abilities in a large comprehensive school in Newcastle on Tyne , England. Since retiring he has worked with the Institute of Physics UK as a Teacher Trainer in the North East of England and throughout the UK. He has represented UK at Science on Stage in Geneva 2005, Grenoble 2007, Berlin 2008, Copenhagen in 2011 and Slubice in 2013. David now works with the International Science on Stage (Europe) Committee as UK representative and member of the Executive Board. He is author of articles in the European journal Science in School and several "hands on" articles in the international journal Physics Education, including a regular column entitled “What happens Next?” He has led workshops at many conferences throughout the UK and Europe. David is particularly interested in making Physics accessible to all and showing the physics in everyday things to the public, whatever their age. Most recently he was given a special commendation from the Institute of Physics for his recent article on the Tippee Top, and has been instrumental in raising awareness of the problems children with Colour vision deficiency experience in science. David is a member of the latest Science on Sate i-stage group producing on line materials for teachers on “Science and Football”. David is a keen musician (playing violin, and Northumbrian small pipes )and recently led an international choir at Science on Stage in London. Apart from his science David spends time at home in a community orchestra, is a governor of his local school, a keen member of his village church and a grandfather! Science on Stage…“From teachers, for teachers” …is a teacher network established in 2000 …is a non-profit association since 2011 with headquarters in Berlin …has National Steering Committees (NSCs) in 25 countries …reaches about 100.000 teachers and teacher trainers, e.g.
    [Show full text]
  • Science on Stage Position and Statements
    SCIENCE ON STAGE POSITION AND STATEMENTS Science on Stage is the leading network for STEM teachers in Europe: For over 15 years our non-profit initiative has been providing a platform to support committed STEM teachers the exchange of best-practice teaching ideas across borders and in the long-term set-up of international teacher co-operations. Following the principle ‘from teachers for teachers’ the focus is on teachers as educational experts. Science on Stage is supporting their international professionalization: From primary to secondary school – motivated teachers are key to help students develop the skills they need for the societal challenges of the future. SCIENCE ON STAGE: TEACHER PROFESSIONALISM FROM TEACHERS FOR TEACHERS FOCUS ON TEACHERS REAL CHANGES START AT THE BASE challenge: Committed teachers should be supported in their personal and professional growth. The appreciation of the teaching challenge: Representatives of politics, industry and education profession itself should be strengthened in society. providers agree that professional and well-trained teachers play a key role when it comes to facing large scale societal challenges of the Science on Stage supports teachers‘ motivation by organising future. international educational festivals, international cooperation between teachers as well as cross-border teacher trainings. By Science on Stage, the European Network for STEM Teachers, experiencing these kind of personal exchanges with like-minded continues to support the in-service training, motivation and colleagues, teachers’ self esteem is strengthened and new skills are networking between teachers with good practice teaching ideas. gained. As a public platform for good practice teaching ideas it is Teachers have engaged with Science on Stage over the past 15 years especially important to us to highlight our teachers’ commitment to via non-bureaucratic and effective exchange activities.
    [Show full text]
  • Presentation 2009 the Association, the Activities, the Ambitions
    The European Science Teaching Network Science on Stage Belgium Presentation 2009 p.1 Presentation 2009 The association, the activities, the ambitions. SCIENCE ON STAGE BELGIUM is part of SCIENCE ON STAGE EUROPE The European Science teaching network ASBL SCIENCE ON STAGE BELGIUM VZW www.scienceonstage.be The European Science Teaching Network Science on Stage Belgium Presentation 2009 p.2 A consultation platform for science teachers SCIENCE ON STAGE is a European initiative which is supported by the European Commission, 7 large European research centres, the European Physical Society (EPS) and the European Association for Astronomy and Education (EAAE). SCIENCE ON STAGE is consulting platform which offers science teachers all over Europe to meet each other, to exchange ideas, to try out didactic methods, to look for experiments and to exchange material. • The 7 research centres are: - The European Organization for Nuclear Research (CERN) - The European Fusion Development Agreement (EFDA) - The European Molecular Biology Laboratory (EMBL) - The European Space Agency (ESA) - The European Southern Laboratory (ESO) - The European Synchrotron Radiation Facility (ESRF) - The Institute Laue-Langevin (ILL) ASBL SCIENCE ON STAGE BELGIUM VZW www.scienceonstage.be The European Science Teaching Network Science on Stage Belgium Presentation 2009 p.3 • Science on Stage Europe members are Austria, Belgium, Bulgaria, Cyprus, Czech Republic, Denmark, Finland, France, Germany, Greece, Hungary, Ireland, Italy, Lithuania, Luxembourg, Malta, Netherlands, Norway,
    [Show full text]
  • Science on Stage: Gathering Momentum
    sis_15_RZ.qxq:Layout 1 28.05.2010 19:15 Uhr Seite 2 Our image of the world – a project combining astronomy and art Schools from all over Austria display their projects Walking with the planets (Kinderplane- tenweg) Science on Stage: gathering momentum Science on Stage Austria ing festival in Copenhagen, Denmark, their enthusiasm for science, to swap I was lucky enough to attend the in 2011w1 – and it wasn’t an easy ideas and to gain inspiration for their Science on Stage Austria event as a choice for the eight scientists, educa- teaching. Another success for Science member of the jury. After two days, tors, and members of the Austrian edu- on Stage. my head was in a whirl: how to com- cation ministry who made up the jury. For more details, including the win- pare a primary school’s 7 km scale All the 41 projects presented were ning projects, visit the Science on model of the Solar System – complete wonderful; all represented inspiration Stage Austria websitew2. with a rucksack full of experiments and hard work by teachers and stu- for the children to perform on each dents alike. There were ideas for ‘planet’ – with a project in which sec- measuring your mass (not your Science on Stage Belgium ondary-school students developed weight), getting a feel for food webs Where could you take a virtual trip experiments to explain the physics of (with the help of some cuddly toys), to Mars, learn how to build a ‘green’ music to younger children? And how investigating the beauty of polarisa- battery, or discover the physics of should we judge those against some tion, or using Excel to model predator music? Again, at Science on Stage – impressive original research into the and prey populations; there were also this time in Belgium, where on 27 effects of diet on health, performed by plays, demonstrations and hands-on February 2010, 140 teachers, inspec- students at an agricultural secondary experiments.
    [Show full text]
  • The European Science Teachers' Network
    SCIENCE ON STAGE EUROPE The European Science Teachers’ Network FROM TEACHERS FOR TEACHERS www.science-on-stage.eu tb Science on Stage Europe brings together science teachers from across Europe to exchange best practice and teaching ideas and concepts with passionate col- leagues from over 30 countries. Science on Stage Europe believes that the best way to improve science teaching and to encourage more schoolchildren to consider a career in science or engineering is to motivate and inform their teachers. The non-profit organisation was founded in 2000 and reaches 100,000 teachers Europe-wide. The countries involved are: ICELAND JOIN FINLAND US! NORWAY CANADA SWEDEN LATVIA DENMARK LITHUANIA UNITED KINGDOM IRELAND THE NETHERLANDS POLAND GERMANY BELGIUM CZECH REPUBLIC UKRAINE SLOVAKIA KAZAKHSTAN FRANCE AUSTRIA HUNGARY SWITZERLAND SLOVENIA ROMANIA SERBIA BULGARIA ITALY GEORGIA SPAIN ALBANIA PORTUGAL GREECE TURKEY CYPRUS Activities Science on Stage festival Every two years Science on Stage Europe orga nises Europe’s biggest science teaching festival. Teachers from all over Europe exchange their ideas, projects and methods at stands, in work shops and on stage. These ideas are after wards spread throughout Europe via follow-up activities: Teacher training International projects The Science on Stage countries Working groups of international teachers organise teacher training events develop materials for their colleagues in Eu- involving an international project rope. Science on Stage publishes these and a national festival project. concepts, which can be ordered or down- loaded for free. Travel scholarships Teachers from different countries who par- Teaching materials ticipated in the festival can meet again to Science on Stage publishes teaching mate- continue their work and to develop joint rials developed by teachers for teachers in projects.
    [Show full text]