ISP 205, Section 3, Spring 2003, Prof. Stein

UNIT III: SKY & PLANETS
SYLLABUS


DATE                             TOPIC               READING ASSIGNMENT

Monday, March 24 Review Midterm Exam #2 The Solar System Chapter 6 Terrestrial Planets section 6.2 Jovian Planets section 6.2 Wednesday, March 26 Formation of Planets Chapter 13 Characteristic Properties Astroids & comets sections 12.4, 13.2 Formation Scenarios sections 6.3, 13.3 Extra-solar Planets sections 20.3, 20.4 Homework #6, due Wednesday, April 2 Moon Project begins, due Wednesday, April 23 Monday, March 31 The Earth Chapter 7 Atmosphere: Composition, Heating & Cooling Greenhouse effect Evolution Surface: plate tectonics, impact cratering, erosion Interior: core, mantle, crust, differentiation Wednesday, April 2 Scientific Models and Theories prologue Science is Problem Solving Process of scientific problem solving and model building Homework #6, due NOW Monday, April 7 Appearance of the Sky Chapter 3 A-K: In Planetarium Locating bright stars & constellations Motion of the Sun, Moon, Stars, Planets Geocentric vs. Heliocentric models L-Z: In Class The Seasons Moon phases & eclipses Wednesday, April 9 Appearance of the Sky (continued) L-Z: In Planetarium Locating bright stars & constellations Motion of the Sun, Moon, Stars, Planets Geocentric vs. Heliocentric models A-K: In Class The Seasons Moon phases & eclipses Homework #7, due Wednesday, April 16 Monday, April 14 Models of the Solar System section 1.4 Ptolemaic Geocentric model Copernican Heliocentric model Testing the models: Galileo, Tycho Brahe Kepler's model Wednesday, April 16 Motion and Gravity Chapter 2 Motion, Velocity and Acceleration Force and mass Newton's Law of Motion: Acceleration = Force / Mass Newton's Law of Gravity (again): Force of Gravity = G M m / R2 Orbital motion Kepler's laws explained Homework #7, due NOW Quiz 3: (Warm-up for Exam 3) Chapters 1-3, 6, 7, 13 Monday, April 21 Review: Chapters 1-3, 6, 7, 13 Wednesday, April 23 Mid-Term Exam #3, Unit III: Sky & Planets Chapters 1-3, 6, 7, 13 Moon Project Due NOW Wednesday, April 30 Final Exam, 8-10 pm, Eli Broad Business College room N100 Entire course

















UNIT III: THE SKY & PLANETS  -   OBJECTIVES

  1. Become familiar with the night sky: the bright stars and their constellations, the planets and the Moon.
  2. Describe the stages in the development of a new scientific model. Identify these stages in the development of the different models of planetary motion.
  3. Describe and explain the apparent daily motions of the sun, moon, planets and stars relative to the horizon.
  4. Describe and explain the apparent and real motions of the sun, moon and planets with respect to the stars.
  5. Use the celestial globe and celestial coordinates to locate stars and the Sun.
  6. Tell what astronomical cycles set the time intervals of day, month and year.
  7. Relate the appearance, location and motion of the moon and planets in the sky to their position and motion with respect to the sun and earth in a model of the solar system. Specifically, explain: daily motions, the seasons and annual motions, eclipses and phases of the Moon.
  8. Describe the development of the Copernican, Keplerian and Newtonian models of the solar system.
  9. Explain retrograde motion in the Ptolemaic, Copernican and Keplerian models of the solar system.
  10. Identify the concepts: velocity, acceleration, momentum, force, mass, and energy.
  11. Describe the cause-effect relation between force and motion (Newton's law of motion). Illustrate it by simple concrete examples.
  12. Describe the relation between matter (mass), distance and gravity (Newton's law of gravity).
  13. Describe the observational evidence for and against the Ptolemaic, Copernican, Keplerian and Newtonian models of the solar system.
  14. Compare and contrast the Ptolemaic, Copernican, Keplerian, and Newtonian models of planetary motion in terms of geometry, physics, simplicity and prediction.
  15. Evaluate the impact of the Ptolemaic, Copernican, Keplerian and Newtonian models of the solar system on our concept of the universe.
  16. Apply the theories of motion and gravity to explain astronomical and everyday phenomena.
  17. Compare and contrast the Jovian and Terrestrial planets as groups.
  18. Describe the structure of the Earth: its interior, surface and atmosphere. Describe how the internal structure of the Earth is determined. Describe the development of the theory of plate tectonics. Describe the energy balance on Earth: how it is heated and cooled, how heat is distributed from the tropics to the arctic. Describe how the Earth has evolved: differentiation of the interior, outgassing of the atmosphere, evolution of the surface.
  19. Describe the Greenhouse Effect. Describe the processes contributing to global warming of Earth.
  20. Identify 3 characteristic properties of the solar system that any theory of its origin must explain.
  21. Describe the Solar Nebula Theory of planet formation. Evaluate how well it explains the 3 characteristic properties of the solar system.
    Evaluate how well it explains recent observations of planets around other stars ("extrasolar" planets).
  22. Apply the paradigm of scientific model building to theories of the structure of the planets, their origin and evolution.


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Updated: 2003.04.09 (Wednesday) 18:28:49 EDT
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Bob Stein's home page, email: steinr@msu.edu