PPT-Features on Earth’s Surface

Pages 159172 Constructive Forces earthquakes crustal deformations volcanic eruptions sediment depostion Watch Destructive Forces Wear down landforms carry bits and pieces of land to other places like the sea . superweak. angular ground motions. JINR: J. Budagov, M. Lyablin., G. Shirkov.. CERN: J-Ch. Gayde, D. Mergelkuhl. Main principle : use reflected laser beam from horizontal surface liquid . θ. ψ. Laser. The Moon and Mercury. 8.1 Orbital Properties. 8.2 Physical Properties. 8.3 Surface Features on the Moon and Mercury. 8.4 Rotation Rates. Lunar Exploration. Why Air Sticks Around. 8.5 Lunar Cratering and Surface Composition. The Terrestrial Planets. Units of Chapter 6. Orbital and Physical Properties. Rotation Rates. Atmospheres. The Surface of Mercury. The Surface of Venus. The Surface of Mars. Internal Structure and Geological History. 9.1 Orbital Properties. 9.2 Physical Properties. 9.3 Long-Distance Observations of Venus. 9.4 The Surface of Venus. 9.5 The Atmosphere of Venus. 9.6 Venus’s Magnetic Field and Internal Structure. Units of Chapter 9. The National Weather Service counts on two sources for information:. Radar. Weather Balloon. Data collected from the atmosphere. Data collected from the Earth’s surface . In order to forecast the weather, meteorologists make measurements of:. How does the Earth Change?. Geology. In your Science journal record the UEQ. How does the Earth Change?. Activating Strategy:. Your lab group will have the opportunity to use your observation skills and inferring skills to predict the contents of three film canisters.. This work is protected by U.S. copyright laws and is provided solely for the use of instructors in teaching their courses and assessing student learning. Dissemination or sale of any part of this work (including on the World Wide Web) will destroy the integrity of the work and is not permitted. The work and materials from it should never be made available to students except by instructors using the accompanying text in their classes. All recipients of this work are expected to abide by these restrictions and to honor the intended pedagogical purposes and the needs of other instructors who rely on these materials.. The orbits of Venus and Mercury show that these planets never appear far from the Sun.. Orbital and Physical Properties. The . terrestrial planets have similar densities and roughly similar sizes. , but their rotation periods, surface temperatures, and atmospheric pressures vary widely.. Learning Target:. What is necessary for life to be present in our solar system?. Science Starter:. Pg. 2 Life on Earth Workbook…Answer question 1. Supplies: Life on Earth Workbook. 1. Heartbeat. 2. Return Papers. The Sun. What physical features do you notice?. How does the Sun compare to the Earth and Moon?. What does the Sun provide for the Earth?. Physical Characteristics of the Sun. Sunspots. Solar Flare. Contents. Introduction. General . information. Structure. Formation. Life and Death. Features. Observation. introduction. Great ball of hydrogen plasma. Gravitational centre of . system. 99.8% the mass of the entire solar system. Jase. Love, Gilbert Espinoza, Oscar . Pedroza. Planet Profile. Mass: 4,867,320,000,000,000 billion kg (0.815 x Earth). Equatorial Diameter: 12,104 km. Polar Diameter: 12,104 km. Equatorial Circumference: 38,025 km. LAYERS of the Interior. THE CORE- . Nuclear Fusion occurs. Diameter- 400,000 km. The Radiation Zone- . region of compressed gas and energy is transferred by electromagnetic waves.. Thickness- 300,000 km . US Topo Federal Highway Administration Planning Glossary - http//wwwfhwadotgov/planning/glossary/glossarylistingcfmLock Chamber/SpillwayRock XWaterfallWellEarthen DamNonearthen DamLeveeRapidsHYDROGR