Life on Earth…And Els Ewhere? Activit Y 3 23 50 Activit Y 5 = Nasa S Astrobiology Institute Activit Y 5 53

Total Page:16

File Type:pdf, Size:1020Kb

Life on Earth…And Els Ewhere? Activit Y 3 23 50 Activit Y 5 = Nasa S Astrobiology Institute Activit Y 5 53 Life on Earth …and elsewhere? Students come to class filled with questions about life on other worlds. They have seen fantastic scenarios presented on television and in films. They have read and heard about exploring and colonizing space. They have followed the drama of manned and robotic space missions. The answers to the questions that arise out of these experiences are often complex and multidimensional. How can teachers meaningfully address such questions? The hands-on activities in this Educator Resource Guide lay the con- ceptual groundwork for understanding questions fundamental to the field of astrobiology. They enable students to examine the nature of life, what it requires, its limits, and where it might be found. Through these experiences, students learn important ideas related to the search for extraterrestrial life. After completing the activities in this guide, students will understand more about the nature of life, the habitability of planets, how astrobiol- ogists gain insight into the possibility of extraterrestrial life, the interdis- ciplinary nature of astrobiology, and the difficulties and subtleties of the search for life. Not only will students have a better grasp of the con- cepts, but they will also deepen their appreciation for the many things that are necessary in order for life to arise and persist. Ultimately, the ambition of the guide is to inspire students to stay abreast of develop- ments—and perhaps even to become involved—in the search for life on other worlds. This curriculum guide was produced by TERC under a grant from the NASA Astrobiology Institute. Visit http://nai.nasa.gov/teachers/ for additional astrobiology resources for teachers, and more information on the NASA Astrobiology Institute. Version 2.0 2006 Cover images courtesy of NASA and the Hubble Heritage Team: http://heritage.stsci.edu/public/gallery/galindex.html#gallery 2 INTRODUCTION Life on Earth Activity Overview …and elsewhere? ACTIVITY What is life?...............................................................................................................5 …and elsewhere? Defining Life 1 2–3 daYS* • Compare real and fake or live and dead objects and brainstorm ideas about what life is • Refine the definition by playing 20 Questions to identify an object or organism • Test the definition by comparing “mystery” samples ACTIVITY What does life require? .............................................................................. 11 Understanding that Life Needs Water, Nutrients, and Energy 2 2 DAYS* • Grow organisms in one of 12 classroom environments and identify com- mon requirements (e.g., water, nutrients, and energy) • Design a mission to identify habitable places by searching for water, nutrients, and energy • The Math Extension—Measuring Calories ACTIVITY What makes a world habitable? ......................................................23 Assessing Planets As Candidates for Life 3 1–2 daYS* • Examine Habitability Cards, which discuss each planet and the six large moons in terms of water temperature, atmosphere, energy, and nutri- ents, and identify the top candidates for life in the solar system • The Math Extension—Inverse Square Law ACTIVITY What can life tolerate?.................................................................................37 Identifying the Range of Terrestrial Life 4 2–4 daYS* • Meet some extremophiles. What conditions do they tolerate? • Play a card game similar to Rummy. Students create a set by matching an extremophile, an extreme habitat on Earth, and an extraterrestrial habitat that may be similar to an Earth habitat. • Assemble a crew of extremophiles and target them to specific locations on a planet or moon • Debate the ethics of sending Earth life to other worlds ACTIVITY Is there life on other worlds? ...............................................................49 Determining the Chances of Extraterrestrial Life 5 1–2 daYS* • Discuss the question, “What is the chance that we are the only life in the universe?” • Determine what we need to know to predict the chances of extraterrestrial life • Make estimates for each Drake Equation term and discuss the range of predictions in the class * FOR TIME ESTIMATES, ONE DAY EQUALS A • The Math Extension—Estimation 50-MINUTE CLASS PERIOD ACTIVITY OVERVIEW 3 Using This Guide A CTIVITY Is there life on other worlds? CO NCEPTS Recommended Procedure Activity Guide 3 •The chances for life What makes a world habitable? elsewhere in the galaxy could be either high STEP To get a sense of what your students think Students typically think or low, depending on PURPOSE when they hear the term “extraterrestrial,” of “extraterrestrials” in whether one s assump- 1 ask them: terms of science fic- tions and estimates are If life is playing a game of planetary hide and seek To assess the possi- tion. Pro mpting them conservative or optimistic. to consider other Introduction Do you think there is intelligent life in our galaxy with which we can bility of life in the with us, then our job is to find it. But where in this What is the chance forms of life often solar system that we are the only communicate? In 1961, Dr. Frank Drake identified eight terms to immense solar system should we begin to look, •Finding even simple life Are there changes their answers, forms will be a break- life in the universe? such things as or at least the reasons help people think about what would have to take place for such and what should we be looking for? One way through discovery. extraterrestrials? they provide. C ONTEXT communication to be possible. astrobiologists narrow the number of possible • The large number of “hiding places” is to understand what makes a Activity 3 builds on the work the stu- stars significantly planet or moon habitable. They then look close- increases the possibility What do See what you think the chances are by making your own estimate dents have done ly at these habitable places. of extraterrestrial life. you mean by for each of the terms below. The conservative and optimistic val- defining and exam- extraterrestrials? ining life. Students ues indicate the range of opinion among scientists with regard to No life beyond Earth has ever been found. Does apply this work to each term. You can use the conservative or optimistic estimates the question of this mean that life is a rare accident that hap- SKILL S whether there is life or use another value, depending on your own intuition. pened on Earth due to an extraordinary set of cir- W ould you be on other planets and • Understand that our interested in a planet cumstances and is unlikely to happen elsewhere? moons, a question galaxy contains a large inhabited by microbes, Do you think that Currently, all other planets and moons seem to lack that people have number of stars plants, and insects? Why there are any forms or why not? long pondered and of life elsewhere in at least one major requirement for life. Despite this • Understand and that drives much of the universe? Why? fact, Europa, Mars, and possibly Titan seem to have or Estimate the terms of the the space program. Drake Equation have had conditions conducive to life. Most astrobiologists This activity also feel that, if extraterrestrial life were found, it would be bacte- familiarizes students • Calculate how many civi- STEP Have the class define the term, extraterres- In 1961, Dr. Frank with the planetary lizations with radio tech- ria-like, living beneath a planets or moon s surface, and using trial. Try to get them to broaden the mean- Drake developed an bodies in the solar nology we can chemical energy for its needs. 2 ing to include anything from microbes to equation to estimate system. communicate with plants to intelligent creatures to any living the number of other civilizations that exist in thing. our Milky Way galaxy Finding any kind of life beyond Earth would TIME that we can detect STEP be a profound discovery. It would help us Mention that astrobiology involves thinking using radio technology. 1 to 2 class periods MATERIAL S understand more about how planets and about whether or not there is extraterrestri- It does this by making 3 al life, where it might be, and how we can estimates of eight com- moons can generate the chemistry that • one Activity Guide (pages 53 and 54) learn more about it. ponent factors. Since leads to life and about the conditions that for each student we are unsure whether What to Do To estimate the number of worlds in the Milky Way life can tolerate. Furthermore, it would help STEP To have students identify the factors related there is life out there, let alone intelligent life • blank overhead trans- galaxy that have intelligent life that we can detect provide some important clues to the question to the existence of extraterrestrial life, ask with which we can parencies 4 them what information they would need to using radio technology, follow these steps: of whether life is a rare or common occurrence communicate, there is determine the probability of extraterrestrial no correct solution to • transparency markers in the universe. life. You might begin by saying, “Lets see if the equation — the value of each factor is • calculators w e can estimate how many worlds out 1 Make estimates for each of the eight terms listed there have life (or intelligent life with which open to interpretation. on the Using the Drake Equation w orkshee.t w e can communicate). What would we need to know?” Try to keep your prompting 2 Convert percentages to decimals before multiplying. 3 Multiply the estimates you made for the eight terms. The Drake Equation The number of worlds within Number of stars in the Milky Way Percent of appro- Percent of these our Galaxy that have intelli- galaxy priate stars that stars that are gent life whose radio emis- have planetary appropriate sions should be detectable XX systems X LIFE ON EARTH…AND ELS EWHERE? ACTIVIT Y 3 23 50 ACTIVIT Y 5 = NASA S ASTROBIOLOGY INSTITUTE ACTIVIT Y 5 53 A Background Reading The Recommended The Activity Guide leads stu- starts the investigation and Procedure details how to dents through an activity informs teachers about the implement the activity.
Recommended publications
  • Issues Paper on Exploring Space Technologies for Sustainable Development and the Benefits of International Research Collaboration in This Context
    United Nations Commission on Science and Technology for Development Inter-sessional Panel 2019-2020 7-8 November 2019 Geneva, Switzerland Issues Paper on Exploring space technologies for sustainable development and the benefits of international research collaboration in this context Draft Not to be cited Prepared by UNCTAD Secretariat1 18 October 2019 1 Contributions from the Governments of Austria, Belgium, Botswana, Brazil, Canada, Japan, Mexico, South Africa, Turkey, the United Kingdom, United States of America, as well as from the Economic and Social Commission for Asia and the Pacific, the Food and Agriculture Organization, the International Telecommunication Union, the United Nations Office for Disaster Risk Reduction and the World Food Programme are gratefully acknowledged. Contents Table of figures ....................................................................................................................................... 3 Table of boxes ......................................................................................................................................... 3 I. Introduction .................................................................................................................................... 4 II. Space technologies for the Sustainable Development Goals ......................................................... 5 1. Food security and agriculture ..................................................................................................... 5 2. Health applications ....................................................................................................................
    [Show full text]
  • Glossary - Cellbiology
    1 Glossary - Cellbiology Blotting: (Blot Analysis) Widely used biochemical technique for detecting the presence of specific macromolecules (proteins, mRNAs, or DNA sequences) in a mixture. A sample first is separated on an agarose or polyacrylamide gel usually under denaturing conditions; the separated components are transferred (blotting) to a nitrocellulose sheet, which is exposed to a radiolabeled molecule that specifically binds to the macromolecule of interest, and then subjected to autoradiography. Northern B.: mRNAs are detected with a complementary DNA; Southern B.: DNA restriction fragments are detected with complementary nucleotide sequences; Western B.: Proteins are detected by specific antibodies. Cell: The fundamental unit of living organisms. Cells are bounded by a lipid-containing plasma membrane, containing the central nucleus, and the cytoplasm. Cells are generally capable of independent reproduction. More complex cells like Eukaryotes have various compartments (organelles) where special tasks essential for the survival of the cell take place. Cytoplasm: Viscous contents of a cell that are contained within the plasma membrane but, in eukaryotic cells, outside the nucleus. The part of the cytoplasm not contained in any organelle is called the Cytosol. Cytoskeleton: (Gk. ) Three dimensional network of fibrous elements, allowing precisely regulated movements of cell parts, transport organelles, and help to maintain a cell’s shape. • Actin filament: (Microfilaments) Ubiquitous eukaryotic cytoskeletal proteins (one end is attached to the cell-cortex) of two “twisted“ actin monomers; are important in the structural support and movement of cells. Each actin filament (F-actin) consists of two strands of globular subunits (G-Actin) wrapped around each other to form a polarized unit (high ionic cytoplasm lead to the formation of AF, whereas low ion-concentration disassembles AF).
    [Show full text]
  • Wastewater Technology Fact Sheet: Ammonia Stripping
    United States Office of Water EPA 832-F-00-019 Environmental Protection Washington, D.C. September 2000 Agency Wastewater Technology Fact Sheet Ammonia Stripping DESCRIPTION Ammonia stripping is a simple desorption process used to lower the ammonia content of a wastewater stream. Some wastewaters contain large amounts of ammonia and/or nitrogen-containing compounds that may readily form ammonia. It is often easier and less expensive to remove nitrogen from wastewater in the form of ammonia than to convert it to nitrate-nitrogen before removing it (Culp et al., 1978). Ammonia (a weak base) reacts with water (a weak acid) to form ammonium hydroxide. In ammonia stripping, lime or caustic is added to the wastewater until the pH reaches 10.8 to 11.5 standard units which converts ammonium hydroxide ions to ammonia gas according to the following reaction(s): + - NH4 + OH 6 H2O + NH38 Source: Culp, et. al, 1978. Figure 1 illustrates two variations of ammonia FIGURE 1 TWO TYPES OF STRIPPING stripping towers, cross-flow and countercurrent. In TOWERS a cross-flow tower, the solvent gas (air) enters along the entire depth of fill and flows through the packing, as the alkaline wastewater flows it may be more economical to use alternate downward. A countercurrent tower draws air ammonia removal techniques, such as steam through openings at the bottom, as wastewater is stripping or biological methods. Air stripping may pumped to the top of a packed tower. Free also be used to remove many hydrophobic organic ammonia (NH3) is stripped from falling water molecules (Nutrient Control, 1983). droplets into the air stream, then discharged to the atmosphere.
    [Show full text]
  • Ozonedisinfection.Pdf
    ETI - Environmental Technology Initiative Project funded by the U.S. Environmental Protection Agency under Assistance Agreement No. CX824652 What is disinfection? Human exposure to wastewater discharged into the environment has increased in the last 15 to 20 years with the rise in population and the greater demand for water resources for recreation and other purposes. Disinfection of wastewater is done to prevent infectious diseases from being spread and to ensure that water is safe for human contact and the environment. There is no perfect disinfectant. However, there are certain characteristics to look for when choosing the most suitable disinfectant: • Ability to penetrate and destroy infectious agents under normal operating conditions; • Lack of characteristics that could be harmful to people and the environment; • Safe and easy handling, shipping, and storage; • Absence of toxic residuals, such as cancer-causing compounds, after disinfection; and • Affordable capital and operation and maintenance (O&M) costs. What is ozone disinfection? One common method of disinfecting wastewater is ozonation (also known as ozone disinfection). Ozone is an unstable gas that can destroy bacteria and viruses. It is formed when oxygen molecules (O2) collide with oxygen atoms to produce ozone (O3). Ozone is generated by an electrical discharge through dry air or pure oxygen and is generated onsite because it decomposes to elemental oxygen in a short amount of time. After generation, ozone is fed into a down-flow contact chamber containing the wastewater to be disinfected. From the bottom of the contact chamber, ozone is diffused into fine bubbles that mix with the downward flowing wastewater. See Figure 1 on page 2 for a schematic of the ozonation process.
    [Show full text]
  • Prebiological Evolution and the Metabolic Origins of Life
    Prebiological Evolution and the Andrew J. Pratt* Metabolic Origins of Life University of Canterbury Keywords Abiogenesis, origin of life, metabolism, hydrothermal, iron Abstract The chemoton model of cells posits three subsystems: metabolism, compartmentalization, and information. A specific model for the prebiological evolution of a reproducing system with rudimentary versions of these three interdependent subsystems is presented. This is based on the initial emergence and reproduction of autocatalytic networks in hydrothermal microcompartments containing iron sulfide. The driving force for life was catalysis of the dissipation of the intrinsic redox gradient of the planet. The codependence of life on iron and phosphate provides chemical constraints on the ordering of prebiological evolution. The initial protometabolism was based on positive feedback loops associated with in situ carbon fixation in which the initial protometabolites modified the catalytic capacity and mobility of metal-based catalysts, especially iron-sulfur centers. A number of selection mechanisms, including catalytic efficiency and specificity, hydrolytic stability, and selective solubilization, are proposed as key determinants for autocatalytic reproduction exploited in protometabolic evolution. This evolutionary process led from autocatalytic networks within preexisting compartments to discrete, reproducing, mobile vesicular protocells with the capacity to use soluble sugar phosphates and hence the opportunity to develop nucleic acids. Fidelity of information transfer in the reproduction of these increasingly complex autocatalytic networks is a key selection pressure in prebiological evolution that eventually leads to the selection of nucleic acids as a digital information subsystem and hence the emergence of fully functional chemotons capable of Darwinian evolution. 1 Introduction: Chemoton Subsystems and Evolutionary Pathways Living cells are autocatalytic entities that harness redox energy via the selective catalysis of biochemical transformations.
    [Show full text]
  • Solar System Simulator NASA SUMMER of INNOVATION
    National Aeronautics and Space Administration Solar System Simulator NASA SUMMER OF INNOVATION UNIT Earth and Space Science – Year of the Solar System DESCRIPTION This online software generates views of GRADE LEVELS the bodies of our planetary system at any th th 7 – 9 date from any artificial or natural point of observation. CONNECTION TO CURRICULUM Science and technology OBJECTIVES TEACHER PREPARATION TIME Students will: 1 hour • Investigate how to determine the relative position of the sun, LESSON TIME NEEDED planets, and a number of 30 minutes Complexity: Basic planetary spacecraft using a simple web-based program • Explore how planets change their position in space over time NATIONAL STANDARDS National Science Education Standards (NSTA) Science and Technology Standards • Abilities of technological design • Understanding about science and technology Earth and Space Science • Earth in the solar system • Objects in the sky Common Core State Standards for Mathematics (NCTM) Number and Operations in Base Ten • Perform operations with multi-digit whole numbers and with decimals to hundredths Operations and Algebraic Thinking • Generate and analyze patterns ISTE NETS and Performance Indicators for Students (ISTE) Creativity and Innovation • Use models and simulations to explore complex systems and issues. Technology Operations and Concepts • Understand and use technology systems Aerospace Education Services Project MANAGEMENT MATERIALS Take time to practice with this software. While simple, it offers a • Computer with Internet variety of views with which to become familiar. access On the simulator homepage, a FIELD OF VIEW of 2 will show the inner solar system very nicely. It will be difficult to see the position of ALL the planets at one time.
    [Show full text]
  • Where Less May Be More: How the Rare Biosphere Pulls Ecosystems Strings
    The ISME Journal (2017) 11, 853–862 OPEN © 2017 International Society for Microbial Ecology All rights reserved 1751-7362/17 www.nature.com/ismej MINI REVIEW Where less may be more: how the rare biosphere pulls ecosystems strings Alexandre Jousset1, Christina Bienhold2,3, Antonis Chatzinotas4,5, Laure Gallien6,7, Angélique Gobet8, Viola Kurm9, Kirsten Küsel10,5, Matthias C Rillig11,12, Damian W Rivett13, Joana F Salles14, Marcel GA van der Heijden15,16,17, Noha H Youssef18, Xiaowei Zhang19, Zhong Wei20 and WH Gera Hol9 1Utrecht University, Department of Biology, Institute of Environmental Biology, Ecology and Biodiversity Group, Utrecht, The Netherlands; 2Alfred Wegener Institute Helmholtz Centre for Polar and Marine Research, Bremerhaven, Germany; 3Max Planck Institute for Marine Microbiology, Bremen, Germany; 4Helmholtz Centre for Environmental Research – UFZ, Leipzig, Germany; 5German Centre for Integrative Biodiversity Research (iDiv), Halle-Jena-Leipzig, Leipzig, Germany; 6Swiss Federal Institute for Forest, Snow and Landscape Research WSL, Birmensdorf, Switzerland; 7Center for Invasion Biology, Department of Botany & Zoology, Stellenbosch University, Matieland, South Africa; 8Sorbonne Universités, UPMC Université Paris 06, CNRS, UMR 8227, Integrative Biology of Marine Models, Station Biologique de Roscoff, F-29688, Roscoff Cedex, France; 9Netherlands Institute of Ecology, Department of Terrestrial Ecology, Wageningen, The Netherlands; 10Friedrich Schiller University Jena, Institute of Ecology, Jena, Germany; 11Freie Universtät Berlin,
    [Show full text]
  • Experimental and Statistical Analysis of Nutritional Requirements for the Growth of the Extremophile Deinococcus Geothermalis DSM 11300
    Experimental and statistical analysis of nutritional requirements for the growth of the extremophile Deinococcus geothermalis DSM 11300 Julie Bornot, Cesar Arturo Aceves-Lara, Carole Molina-Jouve, Jean-Louis Uribelarrea, Nathalie Gorret To cite this version: Julie Bornot, Cesar Arturo Aceves-Lara, Carole Molina-Jouve, Jean-Louis Uribelarrea, Nathalie Gor- ret. Experimental and statistical analysis of nutritional requirements for the growth of the ex- tremophile Deinococcus geothermalis DSM 11300. Extremophiles, Springer Verlag, 2014, 18 (6), pp.1009-1021. 10.1007/s00792-014-0671-8. hal-01268947 HAL Id: hal-01268947 https://hal.archives-ouvertes.fr/hal-01268947 Submitted on 11 Mar 2019 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. OATAO is an open access repository that collects the work of Toulouse researchers and makes it freely available over the web where possible This is an author’s version published in: http://oatao.univ-toulouse.fr/22999 Official URL: https://doi.org/10.1007/s00792-014-0671-8 To cite this version: Bornot, Julie and Aceves-Lara, César-Arturo and Molina-Jouve, Carole and Uribelarrea, Jean-Louis and Gorret, Nathalie Experimental and statistical analysis of nutritional requirements for the growth of the extremophile Deinococcus geothermalis DSM 11300.
    [Show full text]
  • Bayesian Analysis of the Astrobiological Implications of Life's
    Bayesian analysis of the astrobiological implications of life's early emergence on Earth David S. Spiegel ∗ y, Edwin L. Turner y z ∗Institute for Advanced Study, Princeton, NJ 08540,yDept. of Astrophysical Sciences, Princeton Univ., Princeton, NJ 08544, USA, and zInstitute for the Physics and Mathematics of the Universe, The Univ. of Tokyo, Kashiwa 227-8568, Japan Submitted to Proceedings of the National Academy of Sciences of the United States of America Life arose on Earth sometime in the first few hundred million years Any inferences about the probability of life arising (given after the young planet had cooled to the point that it could support the conditions present on the early Earth) must be informed water-based organisms on its surface. The early emergence of life by how long it took for the first living creatures to evolve. By on Earth has been taken as evidence that the probability of abiogen- definition, improbable events generally happen infrequently. esis is high, if starting from young-Earth-like conditions. We revisit It follows that the duration between events provides a metric this argument quantitatively in a Bayesian statistical framework. By (however imperfect) of the probability or rate of the events. constructing a simple model of the probability of abiogenesis, we calculate a Bayesian estimate of its posterior probability, given the The time-span between when Earth achieved pre-biotic condi- data that life emerged fairly early in Earth's history and that, billions tions suitable for abiogenesis plus generally habitable climatic of years later, curious creatures noted this fact and considered its conditions [5, 6, 7] and when life first arose, therefore, seems implications.
    [Show full text]
  • Measurement of Cp/Cv for Argon, Nitrogen, Carbon Dioxide and an Argon + Nitrogen Mixture
    Measurement of Cp/Cv for Argon, Nitrogen, Carbon Dioxide and an Argon + Nitrogen Mixture Stephen Lucas 05/11/10 Measurement of Cp/Cv for Argon, Nitrogen, Carbon Dioxide and an Argon + Nitrogen Mixture Stephen Lucas With laboratory partner: Christopher Richards University College London 5th November 2010 Abstract: The ratio of specific heats, γ, at constant pressure, Cp and constant volume, Cv, have been determined by measuring the oscillation frequency when a ball bearing undergoes simple harmonic motion due to the gravitational and pressure forces acting upon it. The γ value is an important gas property as it relates the microscopic properties of the molecules on a macroscopic scale. In this experiment values of γ were determined for input gases: CO2, Ar, N2, and an Ar + N2 mixture in the ratio 0.51:0.49. These were found to be: 1.1652 ± 0.0003, 1.4353 ± 0.0003, 1.2377 ± 0.0001and 1.3587 ± 0.0002 respectively. The small uncertainties in γ suggest a precise procedure while the discrepancy between experimental and accepted values indicates inaccuracy. Systematic errors are suggested; however it was noted that an average discrepancy of 0.18 between accepted and experimental values occurred. If this difference is accounted for, it can be seen that we measure lower vibrational contributions to γ at room temperature than those predicted by the equipartition principle. It can be therefore deduced that the classical idea of all modes contributing to γ is incorrect and there is actually a „freezing out‟ of vibrational modes at lower temperatures. I. Introduction II. Method The primary objective of this experiment was to determine the ratio of specific heats, γ, for gaseous Ar, N2, CO2 and an Ar + N2 mixture.
    [Show full text]
  • Messengers from Outer Space
    The complete absence of national laboratories for standardizing radiation measurements and the lack of physics departments in most radiotherapy centres in Latin America warrant the setting up of one or more regional dosimetry facilities, the functions of which would be primarily to calibrate dosimeters; to provide local technical assistance by means of trained staff; to check radiation equipment and dosimeters; to arrange a dose-intercomparison service; and to co-operate with local personnel dosimetry services. To be most effective, this activity should be in the charge of local personnel, with some initial assistance in the form of equipment and experts provided by the Agency. Although the recommendations were presented to the IAEA as the or­ ganization responsible for the setting up of the panel, the participants re­ commended that the co-operation of the World Health Organization and the Pan-American Health Organization should be invited. It was also suggested that the panel report be circulated to public health authorities in the countries represented. MESSENGERS FROM OUTER SPACE Although no evidence has yet been confirmed of living beings reaching the earth from space, it has been estimated that hundreds of tons of solid matter arrive every day in the form of meteorites or cosmic dust particles. Much is destroyed by heat in the atmosphere but fragments recovered can give valuable information about what has been happening in the universe for billions of years. Some of the results of worldwide research on meteorites were given at a symposium in Vienna during August. During six days of discussions a total of 73 scientific papers was present­ ed and a special meeting was held for the purpose of improving international co-operation in the research.
    [Show full text]
  • The Water on Mars Vanished. This Might Be Where It Went
    The water on Mars vanished. This might be where it went. timesofindia.indiatimes.com/home/science/the-water-on-mars-vanished-this-might-be-where- it-went-/articleshow/81599751.cms NYT News Service | Mar 20, 2021, 10:32 IST Mars was once wet, with an ocean’s worth of water on its surface. Today, most of Mars is as dry as a desert except for ice deposits in its polar regions. Where did the rest of the water go? Some of it disappeared into space. Water molecules, pummeled by particles of solar wind, broke apart into hydrogen and oxygen atoms, and those, especially the lighter hydrogen atoms, sped out of the atmosphere, lost to outer space. A tall outcropping of rock, with layered deposits of sediments in the distance, marking a remnant of an ancient, long-vanished river delta in Jezero Crater, are pictured in this undated image taken by NASA's Mars rover Perseverance. (Reuters) But most of the water, a new study concludes, went down, sucked into the red planet’s rocks. And there it remains, trapped within minerals and salts. Indeed, as much as 99% of the water that once flowed on Mars could still be there, the researchers estimated in a paper published this week in the journal Science. Data from the past two decades of robotic missions to Mars, including NASA ’s Curiosity rover and the Mars Reconnaissance Orbiter, showed a wide distribution of what geologists call hydrated minerals. “It became very, very clear that it was common and not rare to find evidence of water alteration,” said Bethany Ehlmann, a professor of planetary science at the California Institute of Technology and one of the authors of the paper.
    [Show full text]