ENGR (ASTR) 4190/6190
Planetary Atmospheres, Dynamics, and Magnetospheres The University of Georgia
Fall Semester 2012
Professor: David Emory Stooksbury Office: 603 Driftmier Engineering Center Phone: 583-‐0156 (3-‐0156 on campus)
E-‐mail: [email protected]
UGA Bulletin Course Description
The composition and structure of planetary atmospheres; heating and energy
transport; atmospheric dynamics and thermodynamics; orbital dynamics of planets; magnetospheres; and extrasolar planets.
Credits: 3 hours.
Weekly Class Meeting Pattern: Tu/Th lecture (2:00 – 3:15 pm) and Wednesday observing/discussion session (7:55 – 9:50 pm) weekly. Because labs are at the mercy of the weather, we will have to remain flexible. Cloudy nights are built into the schedule. We also have to be flexible since the planets do not follow the academic calendar.
Level: Undergraduate/Graduate
Undergraduate Prerequisite: (MATH 2500 or MATH 2700) and (PHYS 1212-‐ 1212L or PHYS 1312-‐1312L)
Undergraduate Prerequisite or Corequisite: None
Courses that Require this Course as a Prerequisite: None.
Texts:
Planetary Sciences, 2nd ed. Imke de Pater and Jack J. Lissauer. 2010. Cambridge
University Press.
The Copernican Revolution: Planetary Astronomy in the Development of Western Thought. Thomas S. Kuhn. 1957. Harvard University Press.
Topical Outline
Week 1: August 13 -‐ 17 Introduction to the Planets
Lecture Readings:
de Pater and Lissauer: Chapter 1, pp. 1 – 19
Kuhn’s Preface and Forward, pp. VII -‐ XVIII
Homework Problems: 1.2, 1.3, and1.4
Kuhn Discussion: None this week
Observing Session: Taking CCD images
Topic
Introduction to the course
PART I: ORBITAL DYNAMICS
Week 2: August 20 -‐ 24 Newton’s Laws of Motion
Lecture Readings:
Review the chapters in your introductory physics book covering Newton’s laws and their applications in rectilinear and two-‐
dimensions with special attention given to uniform circular motion.
Kuhn’s Chapter 1: The Ancient Two-‐Sphere Universe, pp. 1 -‐ 44
Homework Problems: 1.5 and 1.6
Kuhn Discussion: Preface and Forward
Observing Session: Mars and Jupiter
Topics
Classical Mechanics Space and Time Mass and Force
Newton’s First and Second Laws; Inertial Frames The Third Law and the Conservation of Momentum Newton’s Second Law in Cartesian Coordinates Two-‐dimensional Polar Coordinates
Week 3: August 27 – 31 Momentum and Angular Momentum
Lecture Readings:
Review the chapters in your introductory physics book covering momentum and angular momentum with special emphasis on the conservation of momentum
Kuhn’s Chapter 2: The Problem of the Planets, pp. 45 -‐ 77
Homework Problems: Handout problems, Classical Mechanics I
Kuhn Discussion: Chapter 1: The Ancient Two-‐Sphere Universe, pp. 1 -‐ 44
Observing Session: Mars and Jupiter
Topics
Conservation of Momentum Rockets
The Center of Mass
Angular Momentum for a Single Particle Angular Momentum for Several Particles
Week 4: September 3 -‐ 7 Energy
Monday 3 September is Labor Day
Lecture Readings:
Review the chapters in your introductory physics book covering kinetic energy, potential energy (with special emphasis on potential energy being a function of location), and the conservation of energy.
Kuhn’s Chapter 3: The Two-‐Sphere Universe in Aristotelian Thought, pp. 78 -‐ 99
Homework Problems: Handout problems, Classical Mechanics II
Kuhn Discussion: Chapter 2: The Problem of the Planets, pp. 45 -‐ 77
Observing Session: The Moon
Topics
Kinetic Energy and Work
Potential Energy and Conservative Forces Forces as the Gradient of Potential Energy
The Second Condition for Force to be Conservative Time-‐Dependent Potential Energy
Energy for Linear One-‐Dimensional Systems Curvilinear One-‐Dimensional Systems Central Forces
Energy of Interaction of Two Particles Energy of a Multiparticle System
Week 5: September 10 -‐ 14 Kepler’s Laws
Lecture Readings:
de Pater and Lissauer pp. 22 -‐ 26
Kuhn’s Chapter 4: Recasting the Tradition: Aristotle to Copernicus, pp. 100 -‐133
Homework Problems: Handout problems, Classical Mechanics III
Kuhn Discussion: Chapter 3: The Two-‐Sphere Universe in Aristotelian Thought, pp. 78 -‐ 99
Observing Session: The Moon
Topics
Kepler’s Laws
Center of Mass and Relative Coordinates; Reduced Mass The Equations of Motion
The Equivalent One-‐Dimensional Problem The Equation of the Orbit
The Bounded and Unbounded Kepler Orbits Changes of Orbits
Week 6: September 17 – 21 The Three-‐Body Problem, Perturbation and
Resonances
Lecture Readings:
de Pater and Lissauer pp.26 -‐ 34
Kuhn’s Chapter 5: Copernicus’s Innovation, pp. 134 -‐ 184
Homework Problems: 2.1, 2.3, 2.4, 2.5, and 2.8
Kuhn Discussion: Chapter 4: Recasting the Tradition: Aristotle to Copernicus, pp. 100 -‐133
Observing Session: Asteroids
Topics
Jacobi Constant, Lagrangian Points Horseshoe and Tadpole Orbits Hill Sphere
Distant Planetary Satellites and Quasi-‐Satellites Regular and Chaotic Motion
Resonance
Examples of Orbital Resonance Resonance in the Asteroid Belt
The Resonance Overlap Criterion and Jacobi-‐Hill Stability
Week 7: September 24 – 28 Stability of the Solar System
Lecture Readings:
de Pater and Lissauer pp. 34 -‐ 39
Kuhn’s Chapter 6: The Assimilation of Copernican Astronomy, pp. 185 -‐ 228
Homework Problems: 2.12, 2.14, 2.15, 2.17, and 2.18
Kuhn Discussion: Chapter 5: Copernicus’s Innovation, pp. 134 -‐ 184
Observing Session: Cloudy night make-‐up
Topics
Secular Perturbation Theory Chaos and Planetary Motions
Survival Lifetimes of Smaller Bodies Orbits About an Oblate Planet Gravitational Potential
Precession of Particle Orbits Torque Upon an Oblate Planet
Week 8: October 1 – 5 Tides; The Orbits of Small Bodies
Lecture Readings:
de Pater and Lissauer pp. 39 -‐ 49
Kuhn’s Chapter 7: The New Universe, pp. 229 -‐ 278
Homework Problems: 2.19, 2.21, 2.22, 2.24, and 2.35
Kuhn Discussion: Chapter 6: The Assimilation of Copernican Astronomy, pp. 185 -‐ 228
Observing Session: Cloudy night make-‐up
Topics
Tides
The Tidal Force and the Tidal Bulges Tidal Torque
Tidal Heating
Dissipative Forces and the Orbits of Small Bodies
Week 9: October 8 -‐ 12 Catch Up Week
Lecture Readings:
de Pater and Lissauer pp. 1 -‐ 49
Homework Problems: 2.27, 2.30, and 2.33
Kuhn Discussion: Chapter 7: The New Universe, pp. 229 -‐ 278
Observing Session: Cloudy night make-‐up
Topics
Orbital Dynamics Catch-‐Up and Review
Part II: Planetary Atmospheres
Week 10: October 15 – 19 Solar Heating and Energy Transport
MIDTERM EXAMINATION IS ON THURSDAY 18 OCTOBER. The midterm
examination will cover the lecture material through week 9 – classical mechanics and orbital dynamics.
Lecture Readings:
de Pater and Lissauer pp. 56 -‐ 64
Homework Problems: 3.1, 3.2, 3.3, 3.5, and 3.8
Observing Session: None this week
Topics
Energy Balance and Temperature Thermal (Blackbody) Radiation Albedo and Emissivity
Equilibrium Temperature Conduction
Convection
Hydrostatic Equilibrium Thermodynamics: 1st Law Adiabatic Lapse Rate
Week 11: October 22 – 26 Radiation and Energy Transport
Lecture Readings:
de Pater and Lissauer pp. 64 – 72
Homework Problems: 3.11, 3.12, 3.13, 3.17, and 3.21
Observing Session: TBD
Topics
Radiation Definitions
Energy Transitions (electron transitions) Einstein A and B Coefficients
Equations of Radiative Transfer Thermal Profile
Greenhouse Effect
Radiative Transfer in a Surface
Week 12: October 29 – November 2 – Radiation Catch-‐up Week
Lecture Readings:
de Pater and Lissauer pp. 56 -‐ 72
Homework Problems: 3.22, 3.23, 3.27, 3.28, and 3.29
Observing Session: TBD
Topics
Radiation Catch-‐Up and Review
Week 13: November 5 – 9 Structure & Composition of Planetary Atmospheres
Lecture Readings:
de Pater and Lissauer pp. 76 -‐ 100
Homework Problems: 4.1, 4.3, 4.7, 4.8, and 4.9
Observing Session: Saturn
Topics
Density and Scale Height
Thermal Structure of Planetary Atmospheres Sources and Transport of Energy
Atmospheric Composition Spectra of Planetary Atmospheres Line Profiles
Natural Damping: Lorentz Profile Pressure or Collisional Broadening
Observations of Selected Planets and Satellites
Week 14: November 12 – 16 Planetary Clouds and Circulation
Lecture Readings:
de Pater and Lissauer pp. 100 – 126
Homework Problems: 4.12, 4.13, 4.14, 4.16, and 4.17
Observing Session: Saturn
Topics
Clouds
Formation of Precipitation Clouds on Selected Planets Winds Forced by Solar Heating Hadley Circulation
Thermal Tides Condensation Flows Wind Equations Coriolis Effect
Thermal Wind Equation Convection
Eddies and Vortices Waves
Lightning
Observations from Selected Planets
Week 15: November 19 -‐ 23 Thanksgiving Holiday Break
Lecture Readings:
Review for Final Examination
Homework Exercises: Review for Final Examination
Observing Session: Work on Project Presentation
Topics
Review for Final Examination
Week 16: November 26 – November 30 Planetary Photochemistry; History of
Secondary Atmospheres
Lecture Readings:
de Pater and Lissauer pp. 126 -‐ 147
Homework Problems: 4.20, 4.25, 4.26, 4.27, 4.29, 4.33, 4.34, 4.35 and 4.36 (Note: These homework problems will NOT be collected but will help you on your final examination.)
Presentations: Project Presentations
Topics
Photolysis and Recombination Oxygen Chemistry on the Earth
Photochemistry of Selected Planets and Satellites Electric Currents
Airglow and Aurora
Molecular and Eddy Diffusion Atmospheric Escape
History of Secondary Atmospheres
Week 17: December 3 – 7
Tuesday 4 December is the last day of fall semester. Tuesday 4 December will be running on a Friday class schedule.
Final Examination
Tuesday 11 December 2012, 3:30 -‐ 6:30 pm
Course Learning Objectives Matrix Course Learning Objectives Course Assessment Methods* Extent of Coverage of Program Outcomes** (ABET Criterion 3)
Upon successful completion of this course, the student will be able to:
1. Apply elementary classical mechanics to planetary orbits with an emphasis on Kepler’s Laws, perturbations and resonances.
A, B, C, E a-xxx, j-x
2. Demonstrate an understanding of Newtonian gravitational theory to orbital motion and tides.
A, B, C, E
a-xxx, j-x 3. Explain applied and theoretical aspects of
atmospheric dynamics to planetary atmospheres.
A, B, C, E
a-xxx, j-x
4. Explain applied and theoretical aspects of atmospheric thermodynamics to planetary atmospheres.
A, B, C, E a-xxx
5. Explain and apply simple energy transport models to planetary atmospheres
A, B, C, E
a-x 6. Explain and demonstrate an understanding of the
physics of electromagnetic phenomenon in the solar system.
A, B, C, D, E
a-xx, d-x, g-x, j-xx, k-x 7. Compare and contrast terrestrial and Jovian
planetary atmospheres.
A, B, C, E
a-xxx 8. Demonstrate an understanding of the
relationships among giant planets, brown dwarfs and low-mass stars.
A, E
a-xxx, d-xx, f-xxxx, g-xx * Course Assessment Methods: A – Homework; B – Hourly Exams; C – Final Exam; D – Computer based project; E – Student Evaluation
** Extent of Coverage: x – some, xx – moderate, xxx - extensive ABET EC-2000 Criterion 3 Program Outcomes
a) an ability to apply knowledge of mathematics, science, and engineering: xxx - extensive b) an ability to design and conduct experiments, as well as to analyze and interpret data: x - some c) an ability to design a system, component, or process to meet desired needs: none
d) an ability to function on multi-disciplinary teams: x - some
e) an ability to identify, formulate, and solve engineering problems: none f) an understanding of professional and ethical responsibility: x - some g) an ability to communicate effectively: xx - moderate
h) the broad educational necessary to understand the impact of engineering solutions in a global and societal context: none
i) a recognition of the need for, and an ability to engage in life-long learning: x - some j) a knowledge of contemporary issues: xx - moderate
k) an ability to use techniques, skills, and modern engineering tools necessary for engineering practice: none
Overall Course Contribution to the Program Outcome
This is designed for atmospheric sciences, physics & astronomy, and engineering students. The course will use a multidisciplinary approach to study the comparative study of planetary atmospheres. Special emphasis will be placed on the fundamental physics.
Method of Grading Midterm Exam 15% Final Exam 15% Final Project 25% Observing Sessions 10 % Weekly Write-‐ups 10% Homework 20 % Project Presentation 5% Revision 17 July 2012 Additional Information
The course syllabus is a general plan for the course; deviations announced to the class by the instructor may be necessary. The instructor reserves to right to make changes to the syllabus as necessary.
Academic Honesty
All academic work must meet the standards contained in "A Culture of Honesty." Students are responsible for informing themselves about those standards before performing any academic work.
The link to more detailed information about academic honesty can be found at: www.uga.edu/ovpi/honesty/acadhon.htm.
Engineering Professional Policy
Engineers make great contributions to society. Engineering is a very satisfying profession that provides many rewards but is demanding and requires hard work. The engineering profession is governed by a code of ethics. Engineering faculty at UGA expect students to act in a professional manner at all times and develop the work ethics required for a successful engineering career. Engineering students at UGA are responsible for maintaining the highest standards of professionalism and professional practice.
Engineering Grading Policy Regarding Communication Skills
Thirty percent of the grade on all written assignments (lab reports and papers) and oral presentations will be based on quality of communication. Spelling, grammar, punctuation, and clarity of writing are evidence of written communication quality. Enunciation, voice projection, clarity and logical order of the presentation and effective use of visual aids are evidence of oral communication quality.
Homework Policy
Homework problems are due at the beginning of class on the Thursday following the week assigned.
Class Attendance Policy
Lecture attendance is encouraged. Material will be covered in class that is not in the book. Attendance is required for all observing and discussion sessions.
Discussion Write-‐ups
Two page typed (10 or 12 point with one inch margins) discussion write-‐ups are due at the beginning of Tuesday ‘s lecture. Each write-‐up should include a summary of Larson’s main points and your thoughts on his points.
Literature Presentations
Students are required to give a presentation based on their project. The presenter will be responsible for choosing the research problem, finding the appropriate literature, presenting the findings, and leading a class discussion on the research problem.
Final Project
Undergraduates are to write a 9 to 11 pages term paper on a planetary sciences topic. Undergraduates should include a minimum of 15 references from referred science journals.
Graduates are to write a 12 to 15 pages term paper on a planetary sciences topic. Graduate students should include a minimum of 25 references from referred science journals
A copy of the abstract of each reference should be submitted with the final paper. Use 12-‐point type with one-‐inch borders.
Make sure to adequately define a narrow planetary science topic. The paper must go into the detail physics of the topic.