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
- 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 and explain the apparent daily motions of the sun, moon,
planets and stars relative to the horizon.
- Describe and explain 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, the seasons and annual motions, eclipses and phases of the
Moon.
- Describe the development of the Copernican, Keplerian and
Newtonian models of the solar system.
- Explain retrograde motion in the Ptolemaic,
Copernican and Keplerian models of the solar system.
- Identify the concepts: velocity, acceleration, momentum, force,
mass, and energy.
- 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).
- Describe the observational evidence for and against the
Ptolemaic, Copernican, Keplerian and Newtonian 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, Keplerian
and Newtonian models of the solar system on our concept of the universe.
- Apply the theories of motion and gravity to explain astronomical
and everyday phenomena.
- Compare and contrast the Jovian and Terrestrial planets as groups.
- 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.
- Describe the Greenhouse Effect.
Describe the processes contributing to global warming of Earth.
- Identify 3 characteristic properties of the solar system
that any theory of its origin must explain.
- 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).
- Apply the paradigm of scientific model building to theories
of the structure of the planets, their origin and evolution.
This page will be updated continually throughout the course.
Updated:
2003.04.09 (Wednesday) 18:28:49 EDT
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Visions of the Universe
Bob Stein's
home page, email:
steinr@msu.edu