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WOODLAND HILLS HIGH SCHOOL LESSON PLAN SAS and Understanding By Design Template Name Kowinsky Date 4/07/2014 Length of Lesson 15 daysContent Area Astronomy Edline has been updated: _X__ Webpage has been updated: __X__ STAGE I – DESIRED RESULTS LESSON TOPIC:Outer Planets BIG IDEAS: (Content standards, assessment anchors, eligible content) objectives, and skill focus) Stars have life cycle ESSential Questions.- Where did all the material on earth come from? S11.A.1.3.2, S11.A.3.1.1, S11.A.3.3.3, S11.D.1.2.1, S11.D.3.1.1, S11.D.3.1.3 UNDERSTANDING GOALS (CONCEPTS): Groups of stars that move in unison in the night sky form constellations. Direct and remote sensing provide evidence that billions of stars cluster into galaxies Direct and remote sensing provide evidence that the universe contains billions of galaxies Students will understand: s ESSENTIAL QUESTIONS: VOCABULARY: Roche Limit, Shephard Moon, Ring, Galilean Moon, Molecular and Metallic Hydrogen, Tidal Heating STUDENT OBJECTIVES (COMPETENCIES/OUTCOMES): S General Properties of Jovial Planets: Compare and contrast gas giants from terrestrial planets. List the Gas giants from closest to the Sun to farthest. Define & Discuss the following terms/Concepts: Atmosphere: Belts Zones Belt-Zone Circulation Molecular Hydrogen Storms Why do storms last so long? What gives storms their energies? Compare and contrast the atmospheres on Jupiter and Saturn vs. Uranus and Neptune. Interior: Liquid Metallic Hydrogen Rings: Roche Limit Shepherd Moon. Ring compositions and size Be sure to explain how old ring systems are, what causes the dust in the ring systems to be destroyed, and what shepherd moons do to sustain ring systems. Satellites: Identify key properties and features of the following moons: Jupiter’s Galilean satellites: Io, Europa, Ganymede, Callisto Saturn: Titan Neptune: Triton Define Tidal Heating. Discuss which moons undergo tidal heating and why. Explain why tidal heating causes Io and Europa to be very different from Ganymede and Callisto. Name the 4 Galilean moons from closest to farthest from Jupiter. Discuss why Titan is a unique moon in the solar system. Explain why astronomers believe Europa is the best place in the Solar system to search for life. Compare Titans atmosphere to early Earths atmosphere. Space missions: Know which planet Cassini is studying, know which planet Galileo studied, and know what the Voyager I & II spacecraft studied. Students will be able to: STAGE II – ASSESSMENT EVIDENCE PERFORMANCE TASK:Classwork Homework Tests/Quizzes Labs Warm-ups/Exit Slips Formative assessments OTHER EVIDENCE: STAGE III: LEARNING PLAN INSTRUCTIONAL PROCEDURES: (Active Engagement, Explicit Instruction, Metacognition, Modeling, Scaffolding) Presentation, discussion, pre-lab, laboratory experiments, actvities MINI LESSON: M: Planets Project T: Planets Project W: Planets Project MATERIALS AND RESOURCES: Overhead/Board/Promethean board Lab material/equipment Power of Ten video Challenger Video Moon Landing Video Math Worksheets 1-4 Scale Activity Worksheet Scientific Notation Quiz INTERVENTIONS: ASSIGNMENTS: Preferential seating Cooperative work Guided notes Modified tests Classwork Homework Tests/Quizzes Labs Warm-ups/Exit Slips Formative assessments