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
- Become familiar with the night sky: the bright stars and their
constellations, the planets and the Moon.
- Describe the stages in the development of a new scientific
model. Identify these stages in the development of the different
models of planetary motion.
- Describe the apparent daily motions of the sun, moon, planets
and stars relative to the horizon.
- Describe the apparent and real motions of the sun, moon and
planets with respect to the stars.
- Use the celestial globe and celestial coordinates to locate stars and
the Sun.
- Tell what astronomical cycles set the time intervals of day,
month and year.
- 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.
- Explain the cause of the seasons.
- Describe the development of the Copernican, Keplerian and
Newtonian models of the solar system.
- Describe the observational evidence for and against the
Ptolemaic, Copernican, Keplerian and Newtonian models of the solar system.
- Explain retrograde motion in the Ptolemaic,
Copernican and Keplerian models of the solar system.
- Compare and contrast the Ptolemaic, Copernican, Keplerian, and
Newtonian models of planetary motion in terms of geometry, physics,
simplicity and prediction.
- Evaluate the impact of the Ptolemaic, Copernican and Keplerian
models of the solar system on our concept of the universe.
- Identify the concepts: velocity, acceleration, force, and mass.
- Describe the cause-effect relation between force and motion
(Newton's law of motion). Illustrate it by simple concrete examples.
- Describe the relation between matter (mass), distance and
gravity (Newton's law of gravity).
- Apply the theories of motion and gravity to explain
astronomical and everyday phenomena.
Summary of changes to the Objectives during the unit:
- "Explaining the seasons" has been split out separately from Number 7,
and is now Number 8.
- There is an addition to Number 9. to add the Newtonian model of the
Solar System.
- Delete the momentum and energy objectives within Number 13.
- Delete the objective about conservation of energy (old Number 14).
Updated: 1997.02.10 (Monday) 14:45:57 EST
This page has been accessed
times.
Visions of the Universe
Beth Hufnagel's home page, email:
bhufnage4@pilot.msu.edu
Bob Stein's home page, email:
steinr@pilot.msu.edu