Middle School Earth Science: Human Impact
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Lecture 2A Structure and Composition of the Earth Plate Tectonics
Engineering and Environmental Geology (EART 3012) – 2014 Lecture 2A Structure and composition of the Earth Plate tectonics Dr Tom Raimondo See Marshak pg. 42–53; 78–100 Figures taken from Earth: Portrait of a Planet, WW Norton & Co. Course outline and introduction Sweet weekly homework Every week, there are regular tasks that must be completed. There are clear expectations about the amount of time you should spend studying this course. Contact time per Non-contact time per week week Lectures 2 hours 1–2 hours pre- reading and revision Practicals 2 hours 1 hour pre-reading Weekly quizzes - 30 mins to 1 hour eModules - 30 mins to 1 hour Textbook online - 30 mins to 1 hour resources Total 4 hours 4–5 hours Lecture 2A Why do I need to know all this stuff? . Knowing the structure and composition of the Earth forms the basis for all geological concepts . We need to have a understanding of how the Earth behaves as a whole, and what its properties are, before we can consider more specific Earth systems and cycles . Plate tectonics is the fundamental geological theory for how the Earth works and how we can predict its behaviour . We need to understand this theory to be able to understand and interpret a range of geological phenomena (e.g. earthquakes, volcanoes, tsunamis, landslides, etc.) Lecture 2A Lecture outline Part 1: Structure and composition of the Earth . Layers of the Earth: crust, mantle and core . Lithosphere and asthenosphere Part 2: Plate tectonics . What is a tectonic plate? . Types of plate boundaries . Other plate features . -
Amplify Science Earth's Changing Climate
Lawrence Hall of Science has new instructional materials that address the Next Generation Science Standards! Check out these Middle School Units… As just one example, compare Middle School units from three different Hall programs. See for yourself how each program goes about addressing the Middle School NGSS Standards related to Human Impacts and Climate Change, and choose the approach that best meets the needs of your school district. MS NGSS Performance Expectations: Human Impacts and Climate Change • MS-ESS3-2. Analyze and interpret data on natural hazards to forecast future catastrophic events and inform the development of technologies to mitigate their effects. • MS-ESS3-3. Apply scientific principles to design a method for monitoring and minimizing a human impact on the Environment. • MS-ESS3-4. Construct an argument supported by evidence for how increases in human population and per-capita consumption of natural resources impact Earth’s systems. • MS-ESS3-5. Ask questions to clarify evidence of the factors that have caused the rise in global temperatures over the past century. Sample Units from Three Different Hall Programs • Amplify Science—Earth’s Changing Climate: Vanishing Ice Earth’s Changing Climate Engineering Internship • FOSS—Weather and Water • Ocean Sciences Sequence—The Ocean-Atmosphere Connection and Climate Change ©The Regents of the University of California ©The Regents of the University of California Description of two Middle School units from Amplify Science Earth’s Changing Climate: Vanishing Ice and Earth’s Changing Climate Engineering Internship Grade 6-8 Units — requiring at least 19 and 10 45-minute class sessions respectively (two of 27 Middle School Amplify Science units) The Problem: Why is the ice on Earth’s surface melting? Students’ Role: In the role of student climatologists, students investigate what is causing ice on Earth’s surface to melt in order to help the fictional World Climate Institute educate the public about the processes involved. -
Earth's Interior
11/7/2012 Please do the Audio Setup Wizard ! 11/7/12 Science Class Connect with Mrs. McFarland & Mr. Gluckin Earth’s Interior Ohio Academic Content Standards Today’s Class Agenda • Review Ground Rules for Earth and Space Sciences Classes The Universe • Earth’s Stats 9. Describe the interior structure of Earth and the Earth’s crust as • Composition of the Earth divided into tectonic plates riding on top of the slow moving currents of magma in the mantle. – Crust/Mantle/Core 11. Use models to analyze the size and shape of Earth, its surface and • Structures of the Earth its interior (e.g. globes, topographic maps and satellite images). – Lithosphere/Asthenosphere • Lithospheric Plates The Study Island lesson is due by 4pm on Thursday: SI 2e • State of matter and heat Student Centered Objectives – Convection Currents I will be able to describe the layers on the inside of the Earth. • Reminders I will be able use images to look at the Earth’s interior by composition. • Today’s Slides I will understand the different physical properties of the Earth’s layers. • Exit Ticket • Your Questions Ground rules Earth’s Stats • Please close all other apps & web pages. No Facebook, games, music, etc. • The Earth's mass is about 5.98 x 1024 kg. • No off‐topic chat • Be respectful of each other • Don’t share personal information • Earth is the densest planet in our Solar • I can see all chat … even “private chat” System (mass/volume). • Earth is made of several layers with different compositions and physical properties, like temperature, density, and the viscosity (“aka” ability to flow). -
The Health and Social Benefits of Nature and Biodiversity Protection
The Health and Social Benefits of Nature and Biodiversity Protection Executive Summary Patrick ten Brink, Konar Mutafoglu, Jean-Pierre Schweitzer, Marianne Kettunen, Clare Twigger-Ross, Yoline Kuipers, Manon Emonts, Liisa Tyrväinen, Teppo Hujala, Ann Ojala A project funded by the European Commission (ENV.B.3/ETU/2014/0039) Funded by the European Commission, DG Environment (ENV.B.3/ETU/2014/0039) Legal notice The contents and views contained in this report are those of the authors, and do not necessarily represent those of the European Commission. Cite this report: ten Brink P., Mutafoglu K., Schweitzer J.-P., Kettunen M., Twigger-Ross C., Kuipers Y., Emonts M., Tyrväinen L., Hujala T., Ojala A. (2016) The Health and Social Benefits of Nature and Biodiversity Protection – Executive summary. A report for the European Commission (ENV.B.3/ETU/2014/0039), Institute for European Environmental Policy, London / Brussels. Corresponding author: Patrick ten Brink – [email protected] Acknowledgements: This executive summary by the core author team builds on and benefits from the inputs by the wider study team – including Owen White and Jonathan Baker (Collingwood Environmental Planning), Irene Lucius and Magdalena Peneva (WWF Danube-Carpathian Programme), Holger Robrecht, Pamela Mühlmann and Elisa Kerschbaumer (ICLEI Europe), Rudolf de Groot (Wageningen University), the extensive literature cited, and the case studies, presentations and discussions at a stakeholder workshop held on the 27th and 28th of January 2016 in Brussels. A summary of the workshop and the presentations are available here. For the workshop, we would like to thank Roby Biwer, Carsten Brauns, and Martine Lartigue at the Committee of the Regions and the contributing participants. -
Planets of the Solar System
Chapter Planets of the 27 Solar System Chapter OutlineOutline 1 ● Formation of the Solar System The Nebular Hypothesis Formation of the Planets Formation of Solid Earth Formation of Earth’s Atmosphere Formation of Earth’s Oceans 2 ● Models of the Solar System Early Models Kepler’s Laws Newton’s Explanation of Kepler’s Laws 3 ● The Inner Planets Mercury Venus Earth Mars 4 ● The Outer Planets Gas Giants Jupiter Saturn Uranus Neptune Objects Beyond Neptune Why It Matters Exoplanets UnderstandingU d t di theth formationf ti and the characteristics of our solar system and its planets can help scientists plan missions to study planets and solar systems around other stars in the universe. 746 Chapter 27 hhq10sena_psscho.inddq10sena_psscho.indd 774646 PDF 88/15/08/15/08 88:43:46:43:46 AAMM Inquiry Lab Planetary Distances 20 min Turn to Appendix E and find the table entitled Question to Get You Started “Solar System Data.” Use the data from the How would the distance of a planet from the sun “semimajor axis” row of planetary distances to affect the time it takes for the planet to complete devise an appropriate scale to model the distances one orbit? between planets. Then find an indoor or outdoor space that will accommodate the farthest distance. Mark some index cards with the name of each planet, use a measuring tape to measure the distances according to your scale, and place each index card at its correct location. 747 hhq10sena_psscho.inddq10sena_psscho.indd 774747 22/26/09/26/09 111:42:301:42:30 AAMM These reading tools will help you learn the material in this chapter. -
Earth's Structure and Processes 8-3 the Student Will Demonstrate An
Earth’s Structure and Processes 8-3 The student will demonstrate an understanding of materials that determine the structure of Earth and the processes that have altered this structure. (Earth Science) 8-3.1 Summarize the three layers of Earth – crust, mantle, and core – on the basis of relative position, density, and composition. Taxonomy level: 2.4-B Understand Conceptual Knowledge Previous/future knowledge: Students in 3rd grade (3-3.5, 3-3.6) focused on Earth’s surface features, water, and land. In 5th grade (5-3.2), students illustrated Earth’s ocean floor. The physical property of density was introduced in 7th grade (7-5.9). Students have not been introduced to areas of Earth below the surface. Further study into Earth’s internal structure based on internal heat and gravitational energy is part of the content of high school Earth Science (ES-3.2). It is essential for students to know that Earth has layers that have specific conditions and composition. Layer Relative Position Density Composition Crust Outermost layer; thinnest Least dense layer overall; Solid rock – mostly under the ocean, thickest Oceanic crust (basalt) is silicon and oxygen under continents; crust & more dense than Oceanic crust - basalt; top of mantle called the continental crust (granite) Continental crust - granite lithosphere Mantle Middle layer, thickest Density increases with Hot softened rock; layer; top portion called depth because of contains iron and the asthenosphere increasing pressure magnesium Core Inner layer; consists of Heaviest material; most Mostly iron and nickel; two parts – outer core and dense layer outer core – slow flowing inner core liquid, inner core - solid It is not essential for students to know specific depths or temperatures of the layers. -
Students' Understanding of Connections Between Human
International Journal Journal of Environmental of Environmental & Science & Educat Scienceion Education Vol. 5, No. 4, October 2010, 407-433 Vol. 3, No. 3, July 2008, xx-xx Students’ understanding of connections between human engineered and natural environmental systems Blakely K. Tsurusaki, Charles W. Anderson Received 23 July 2009; Accepted 30 April 2010 This research draws on developments in educational research where learning progressions are emerging as a strategy for synthesizing research on science learning and applying that research to policy and practice, and advances in the natural sciences, where interdisciplinary research on coupled human and natural systems has become increasingly important. It focuses on the human systems that supply all of our essential goods and services (i.e., food, water, transportation), which begin and end in the earth‘s natural systems. In order to investigate what students know about how human actions affect environmental systems, we developed assessments focusing on supply and waste disposal chains. In addition, students were asked about a major environmental issue – global warming. Assessments were administered to elementary, middle, and high school students from rural, suburban, and urban schools. Results from this study provide insight into how student knowledge of connections between human-engineered and natural systems varies across grade level and context, which is essential if we are to teach students to be responsible citizens and stewards of our environment. Keywords: connected natural -
Earth Science SCIH 041 055 Credits: 0.5 Units / 5 Hours / NCAA
UNIVERSITY OF NEBRASKA HIGH SCHOOL Earth Science SCIH 041 055 Credits: 0.5 units / 5 hours / NCAA Course Description Have you ever wondered where marble comes from? or how deep the ocean is? or why it rains more in areas near the Equator than in other places? In this course students will study a variety of topics designed to give them a better understanding of the planet on which we live. They will study the composition of Earth including minerals and different rock types, weathering and erosion processes, mass movements, and surface and groundwater. They will also explore Earth's atmosphere and oceans, including storms, climate and ocean movements, plate tectonics, volcanism, earthquakes, mountain building, and geologic time. This course concludes with an in-depth look at the connections between our Earth's vast resources and the human population's dependence and impact on them. Graded Assessments: 5 Unit Evaluations; 2 Projects; 2 Proctored Progress Tests, 5 Teacher Connect Activities Course Objectives When you have completed the materials in this course, you should be able to: 1. Describe how Earth materials move through geochemical cycles (carbon, nitrogen, oxygen) resulting in chemical and physical changes in matter. 2. Understand the relationships among Earth’s structure, systems, and processes. 3. Describe how heat convection in the mantle propels the plates comprising Earth’s surface across the face of the globe (plate tectonics). 4. Evaluate the impact of human activity and natural causes on Earth’s resources (groundwater, rivers, land, fossil fuels). 5. Describe the relationships among the sources of energy and their effects on Earth’s systems. -
New Research Opportunities in the Earth Sciences
New Research Opportunities in the Earth Sciences A national strategy to sustain basic research and training across all areas of the Earth sciences would help inform the response to many of the major challenges that will face the planet in coming years. Issues including fossil fuel and water resources, earthquake and tsunami hazards, and profound environmental changes due to shifts in the climate system could all be informed by new research in the Earth sciences. The National Science Foundation’s Division of Earth Sciences, as the only federal agency that maintains significant funding of both exploratory and problem-driven research in the Earth sciences, is central to these efforts, and coordinated research priorities are needed to fully capitalize on the contributions that the Earth sciences can make. ith Earth’s planet. However, it’s population important to note that this Wexpected to collaborative work builds reach 7 billion by the end on basic research in of 2011, and about 9.2 specific disciplines. Core billion by 2050, demand Earth science research for resources such as food, carried out by individual fuel, and water is investigators, or small increasing rapidly. At the groups of scientists, same time, humans are remains the most creative changing the landscape and effective way to and the temperature of the enhance the knowledge atmosphere is increasing. base upon which integra- Expanding basic research tive efforts can build. in the Earth sciences—the study of Earth’s solid Key Research surface, crust, mantle and Opportunities core, and the interactions Figure 1. Combining LiDAR data with geological Conceptual advances in observations helps determine how erosional processes between Earth and the basic Earth science theory respond to rock uplift at Dragon’s Back pressure ridge and technological improve- atmosphere, hydrosphere, along the San Andreas Fault. -
Chapter 11: Atmosphere
The Atmosphere and the Oceans ff the Na Pali coast in Hawaii, clouds stretch toward O the horizon. In this unit, you’ll learn how the atmo- sphere and the oceans interact to produce clouds and crashing waves. You’ll come away from your studies with a deeper understanding of the common characteristics shared by Earth’s oceans and its atmosphere. Unit Contents 11 Atmosphere14 Climate 12 Meteorology15 Physical Oceanography 13 The Nature 16 The Marine Environment of Storms Go to the National Geographic Expedition on page 880 to learn more about topics that are con- nected to this unit. 268 Kauai, Hawaii 269 1111 AAtmospheretmosphere What You’ll Learn • The composition, struc- ture, and properties that make up Earth’s atmos- phere. • How solar energy, which fuels weather and climate, is distrib- uted throughout the atmosphere. • How water continually moves between Earth’s surface and the atmo- sphere in the water cycle. Why It’s Important Understanding Earth’s atmosphere and its interactions with solar energy is the key to understanding weather and climate, which con- trol so many different aspects of our lives. To find out more about the atmosphere, visit the Earth Science Web Site at earthgeu.com 270 DDiscoveryiscovery LLabab Dew Formation Dew forms when moist air near 4. Repeat the experiment outside. the ground cools and the water vapor Record the temperature of the in the air changes into water droplets. water and the air outside. In this activity, you will model the Observe In your science journal, formation of dew. describe what happened to the out- 1. -
Vplanet: the Virtual Planet Simulator
VPLanet: The Virtual Planet Simulator Rory Barnes1,2, Rodrigo Luger2,3, Russell Deitrick2,4, Peter Driscoll2,5, David Fleming1,2, Hayden Smotherman1,2, Thomas R. Quinn1,2, Diego McDonald1,2, Caitlyn Wilhelm1,2, Benjamin Guyer1,2, Victoria S. Meadows1,2, Patrick Barth6, Rodolfo Garcia1,2, Shawn D. Domagal-Goldman2,7, John Armstrong2,8, Pramod Gupta1,2, and The NASA Virtual Planetary Laboratory 1Astronomy Dept., U. of Washington, Box 351580, Seattle, WA 98195 2NASA Virtual Planetary Laboratory 3Center for Computational Astrophysics, 6th Floor, 162 5th Ave, New York, NY 10010 4Astronomisches Institut, University of Bern, Sidlerstrasse 5, 3012 Bern, Switzerland 5Department of Terrestrial Magnetism, Carnegie Institute for Science, 5241 Broad Branch Road, NW, Washington, DC 20015 6Max Planck Institute for Astronomy, Heidelberg, Germany 7NASA Goddard Space Flight Center, Mail Code 699, Greenbelt, MD, 20771 8Department of Physics, Weber State University, 1415 Edvaldson Drive, Dept. 2508, Ogden, UT 84408-2508 Overview. VPLanet is software to simulate the • BINARY: Orbital evolution of a circumbinary planet evolution of an arbitrary planetary system for billions of from Leung & Lee (2013). years. Since planetary systems evolve due to a myriad • GalHabit: Evolution of wide binaries due to the of processes, VPLanet unites theories developed in galactic tide and passing stars (Heisler & Tremaine Earth science, stellar astrophysics, planetary science, 1986; Rickman et al. 2008; Kaib et al. 2013). and galactic astronomy. VPLanet can simulate a generic • SpiNBody: N-body integrator. planetary system, but is optimized for those with • DistOrb: 2nd and 4th order secular models of orbital potentially habitable worlds. VPLanet is open source evolution (Murray & Dermott 1999). -
Earth Science Standards of Learning for Virginia Public Schools – January 2010
Earth Science Standards of Learning for Virginia Public Schools – January 2010 Introduction The Science Standards of Learning for Virginia Public Schools identify academic content for essential components of the science curriculum at different grade levels. Standards are identified for kindergarten through grade five, for middle school, and for a core set of high school courses — Earth Science, Biology, Chemistry, and Physics. Throughout a student’s science schooling from kindergarten through grade six, content strands, or topics are included. The Standards of Learning in each strand progress in complexity as they are studied at various grade levels in grades K-6, and are represented indirectly throughout the high school courses. These strands are Scientific Investigation, Reasoning, and Logic; Force, Motion, and Energy; Matter; Life Processes; Living Systems; Interrelationships in Earth/Space Systems; Earth Patterns, Cycles, and Change; and Earth Resources. Five key components of the science standards that are critical to implementation and necessary for student success in achieving science literacy are 1) Goals; 2) K-12 Safety; 3) Instructional Technology; 4) Investigate and Understand; and 5) Application. It is imperative to science instruction that the local curriculum consider and address how these components are incorporated in the design of the kindergarten through high school science program. Goals The purposes of scientific investigation and discovery are to satisfy humankind’s quest for knowledge and understanding and to preserve and enhance the quality of the human experience. Therefore, as a result of science instruction, students will be able to achieve the following objectives: 1. Develop and use an experimental design in scientific inquiry.