ISP 205, Section 3, Spring 1997, Hufnagel & Stein

UNIT I: THE SKY

SYLLABUS


Date                             Topic                   Reading Assignment

Thursday, Jan. 9 Introduction Chapter 1 Tour through the Universe Activity: The Vast Distance Between Stars Tuesday, Jan. 14 Scientific Models and Theories Chapter 2 Science is Problem Solving Process of scientific problem sections 2.2, 2.3 solving or model building Appearance of the sky Chapters 3, 4 The Celestial Sphere Analog: maps, globe of the Earth Locations in the sky: Coordinates sections 3.1-3.3 Homework #1, due Tuesday 21 Jan. Thursday, Jan. 16 Appearance of the sky (cont'd) Seasons section 4.5 The Moon, its phases and eclipses section 4.7 Tuesday, Jan. 21 Models of the Solar System Chapter 5 Ptolemaic Geocentric model sections 5.1, 5.2 Copernican Heliocentric model sections 5.3, 5.6, 5.7 Testing the models: parallax section 5.4 Galileo, Tycho Brahe Kepler's model sections 5.3, 5.4 Homework #1, due NOW Homework #2, due Tuesday 27 Jan. Thursday, Jan. 23 Planetarium (A-L): Visit #1 Appearance of the sky (continued) Motions of the stars, Sun, Moon, and planets - daily, monthly and annual Orrery: geocentric vs. heliocentric Classroom (M-Z): Motion and Gravity Motion, Velocity and Acceleration Force and mass Newton's Law of Motion: section 5.5 Acceleration = Force / Mass Tuesday, Jan. 27 Planetarium (M-Z): Visit #1 Classroom (A-L): Motion and Gravity Homework #2, due NOW Homework #3, due Tuesday 4 Feb. Thursday, Jan. 29 Planetarium (A-L): Visit #2 Appearance of the sky (cont'd) Chapter 4 Locating bright stars sections 4.3, 4.6, 4.9, and constellations using star maps Appendix Ch. 4 Coordinate systems Classroom (M-Z): Motion & Gravity (cont'd) Newton's Law of Gravity: section 5.5 Force of Gravity = G M m / R2 Kepler's laws explained Energy section 6.5 (pg. 107) Tuesday, Feb. 4 Planetarium (M-Z): Visit #2 Appearance of the sky, cont'd Classroom (A-L): Motion and Gravity (continued) Homework #3, due NOW Homework #4, due Tuesday 11 Feb. Thursday, Feb. 6 The Planets (Optional reading) movie: Travelers Through (Chapters 9, 10) the Solar System Quiz 1: (Warm-up for Exam 1) Chapters 1-5 Moon Project begins, due Thursday 27 February Tuesday, Feb. 11 Review Chapters 1-5 return and review quiz #1 Homework #4, due NOW Thursday, Feb. 13 Mid Term Exam #1 Chapters 1-5

UNIT I: THE SKY

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 the apparent daily motions of the sun, moon, planets and stars relative to the horizon.
  4. Describe 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 and annual motions, eclipses and phases of the Moon.
  8. Explain the cause of the seasons.
  9. Describe the development of the Copernican, Keplerian and Newtonian models of the solar system.
  10. Describe the observational evidence for and against the Ptolemaic, Copernican, Keplerian and Newtonian models of the solar system.
  11. Explain retrograde motion in the Ptolemaic, Copernican and Keplerian models of the solar system.
  12. Compare and contrast the Ptolemaic, Copernican, Keplerian, and Newtonian models of planetary motion in terms of geometry, physics, simplicity and prediction.
  13. Evaluate the impact of the Ptolemaic, Copernican and Keplerian models of the solar system on our concept of the universe.
  14. Identify the concepts: velocity, acceleration, force, and mass.
  15. Describe the cause-effect relation between force and motion (Newton's law of motion). Illustrate it by simple concrete examples.
  16. Describe the relation between matter (mass), distance and gravity (Newton's law of gravity).
  17. Apply the theories of motion and gravity to explain astronomical and everyday phenomena.
Summary of changes to the Objectives during the unit:
  1. "Explaining the seasons" has been split out separately from Number 7, and is now Number 8.
  2. There is an addition to Number 9. to add the Newtonian model of the Solar System.
  3. Delete the momentum and energy objectives within Number 13.
  4. Delete the objective about conservation of energy (old Number 14).
    Updated: 1997.02.10 (Monday) 14:45:57 EST
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    Visions of the Universe

    Beth Hufnagel's home page, email: bhufnage4@pilot.msu.edu
    Bob Stein's home page, email: steinr@pilot.msu.edu