Physics 427 Syllabus Fall 2009
I. General
information
II. BYU Standards and Policies
III. CONFIDENTIAL
IDENTIFICATION NUMBER (CID#)
IV.
Homework
V. EXTRA CREDIT
VI. Grades
VII.
Semester Schedule
VIII. Figures, Tables and Images
Disclaimer: Normally we waive deadlines, modify grade requirements, or otherwise accommodate those occasional students who suffer injuries, severe illnesses or other unforeseen problems, without disrupting the flow of coursework for the remainder of class members. Because of the greater than normal possibility of a disruption this year of unknown magnitude, ranging from a slightly elevated class absence rate to a temporary closure of the entire university, due to the H1N1 (swine) flu virus, we reserve the right to modify any of the class policies, schedules and requirements stated in this syllabus. Our hope is that no changes will be necessary. For your information you may access the letters sent by Academic President John Tanner to faculty and by an unnamed university spokesperson to students regarding this matter. In response to item #3 in President Tanner's letter, we have inserted boxes for you to submit your email address and your cell (or other) phone number with your CID# request. Out intent is to make those two information items available to all class members. (This will be done via an emailed list.) If you do not want to make your email address and/or cell number available to other class members, then leave those boxes blank when you specify your CID#.
Course Number, Section and Title
: Physics 427, Section 1, Introduction to AstrophysicsClass Time and Place: Fall Semester 2009, MWF 1:00-1:50 pm, 247 ESC
Instructor: Dr. Clark G. Christensen
Office: N482 ESC
Office Hours: MWF 2:00 - 3:00 pm, other hours by appointment. Please feel free to call or come by whenever
you need. However, unless you have an appointment, I may not be in except during my scheduled office
hours.Phone: 422-2207 (office), 375-5951 (home) Email: cgchristensen@byu.edu
Grader: Christian Draper. Phone: 801-836-1724 Email: christiandraper@gmail.com
Credit: 3 hours
Prerequisites: Physics 227 and 228.
Texts: Modern Astrophysics
by Bradley W. Carroll and
Dale A. Ostlie 1996 ( Reading, Massachusetts & other
locations: Addison-Wesley Publishing
Company, Inc.)
II. BYU STANDARDS AND POLICIES
Standards: Each of you has signed a pledge to maintain BYU standards including those of honesty, respectful treatment of others, and modesty and dignity in dress and grooming. Your instructor is also fully committed to those standards and expects, as a matter of honor, that the conduct of all class members will be in conformity with those standards.
Sexual Harassment: BYU's policy against sexual harassment extends not only to employees of the university but to students as well. If you encounter sexual harassment or gender-based discrimination, please talk to your instructor, contact the Equal Employment Office at 422-5895, or contact the Honor Code Office at 422-2847.
Student with Disabilities: BYU is committed to providing reasonable accommodation to qualified persons with disabilities. If you have any disability that may adversely affect your success in this course, please contact the Services for Students with Disabilities Office at 422-2767. Services deemed appropriate will be coordinated with you and your instructor by that office.
III. CONFIDENTIAL IDENTIFICATION NUMBER (CID#)
To enable us to identify
you on postings of scores, class rankings and grades, in conformity with federal privacy laws, we ask that you assign
yourself a confidential four-digit identification number (CID#). (If you fail
to do so, your scores will still be known to your instructor but will not appear
on posted lists.) If more than one student selects the same CID#, that number
will be assigned to the first person making the selection. Later selectors will
be invited to choose different numbers. Please fill in the yellow boxes
below, then click the "Submit" button. If
you discover an error in any box after you have exited it, please hit the
"Reset" button and start over. Be sure to read the comment regarding
your email address and cell number in the disclaimer above before you fill in and submit the form.
There will be a number of homework assignments during the semester. You may collaborate in doing the homework insofar as finding the correct procedure for working problems. However, each student should do his/her own calculations, plot his/her own graphs, etc. You may compare final results and redo your work if you feel so inclined.Policy:
Homework is due at the beginning of the class periods on the dates indicated on the semester schedule. Late homework will be penalized using the relation
s = so e-(t-to)/20 ,
where s is the earned score rounded to the nearest tenth of a point, so is the "on-time score," to is the date on which the homework is due and t is the date on which the homework is submitted plus 1 if the homework is submitted after the time at which class begins. Therefore an assignment submitted 2 minutes late is worth e-1/20 = 0.951 of its on-time value. (The score value of homework exponentially decays with a 20-day time constant [13.86-day half-life].)
Assignments: Homework assignments can be obtained by clicking the assignment numbers posted on the semester schedule. Your instructor may modify, add to, or cancel some of the posted homework problems at any time during the semester.
Occasionally an opportunity to
earn extra credit will arise. Points earned as extra credit will
be added to your total homework score. Thus, when there are
extra-credit opportunities, it will be possible to earn in excess of a
100-percent total score for the semester.
Grades will be based on your total percentage score entered into a curve based on the performances of the classes of several semesters (because of the small number of students enrolled in a single semester). Your percentage score will be determined using the weights in the following table.
| Item | Maximum Raw Score | Weight [%] |
| Homework | ? | 40 |
| Midterm Examination | ? | 20 |
| Final Examination | ? | 40 |
| Total | 100 |
Class meets at 1:00-1:50 pm in C247 ESC
|
WK# |
DATE |
TOPIC |
Figures, Tables, Images |
SUPPL RDG (pp.) | HW ASSGN DUE1 | |||||
|---|---|---|---|---|---|---|---|---|---|---|
| 1 | M Aug 31 |
Nomenclature, Data Sources, Catalogs, Astronomical Literature, Simbad |
0-7 |
- |
||||||
| W Sep 2 |
Simbad, Astronomical Literature, Coordinate Systems |
8-14 |
3-21 |
|||||||
| F Sep 4 |
Spherical Trigonometry |
15 | ||||||||
| 2 | M Sep 7 | L A B O R D A Y H O L I D A Y | ||||||||
| W Sep 9 | Stellar Positions |
Time Systems and Seasons |
16-26 | |||||||
| F Sep 11 |
Coordinate Precession: Exact Method and Approximate Methods |
27-33 |
15-16 |
|||||||
| 3 | M Sep 14 | |||||||||
| W Sep 16 | ||||||||||
| F Sep 18 |
Chandler Wobble, Refraction |
34-41 | ||||||||
| 4 | M Sep 21 |
Stellar Aberration |
42 | |||||||
| T Sep 22 | 11:00 am, Neil deGrasse Tyson Forum (extra-credit opportunity)2 | |||||||||
| W Sep 23 | Stellar Positions |
Trigonometric Parallaxes, Parallactic and Proper Motion |
43-50 |
63-65 |
||||||
| F Sep 25 | Stellar Motions: Radial, Transverse & Space Velocities, Moving-Cluster π |
46-51 |
18-21, 126-130, 960-964 |
|||||||
| 5 | M Sep 28 | Statistical Parallaxes, Luminosities: Apparent & Absolute Magnitudes |
52-58 |
65-69 |
||||||
| W Sep 30 | Magnitudes, Flux Densities, Luminosities, Color Indices |
59-62 |
82-87 |
|||||||
| F Oct 2 | Effects of Interstellar Absorption: Extinction and Reddening |
63-64 |
265-268, 437-442 |
|||||||
| 6 | M Oct 5 | Stellar Spectral Classification |
65-77 |
223-240 |
|
|||||
| W Oct 7 | The H-R Diagram, Measures of Stellar Temperature |
78-87 |
223-250 |
|||||||
| F Oct 9 |
|
|||||||||
| 7 | M Oct 12 |
The Stellar Luminosity Function |
88-95 |
1044-1046 |
||||||
| W Oct 14 | ||||||||||
| F Oct 16 |
|
|||||||||
| 8 | M Oct 19 |
Telescopes |
Primary Functions, Light-Gathering Power |
96-100 |
||||||
| Tu Oct 20 |
M I D T E R M E X A M I N A T I O N ( in Testing Center) |
Midterm |
||||||||
| W Oct 21 |
Telescopes |
Image and Apparent Surface Brightness, Plate Scale | 159-197 | |||||||
| F Oct 23 |
Angular Resolution, Seeing |
101-104 |
||||||||
| 9 | M Oct 26 |
Magnification, Refractors, Aberrations |
105-109 |
|||||||
| W Oct 28 | Reflector Designs, Aberrations, Observatory Sites |
110-126 |
||||||||
| F Oct 30 | Schmidt Telescopes, Radio Telescopes |
127-136 |
||||||||
| 10 | M Nov 2 | Spectrographs | Basic Designs, Performance Characteristics |
137-141 |
129 |
|
||||
| W Nov 4 | Speed |
142-144 |
||||||||
| F Nov 6 | Diffraction Gratings |
145-149 |
||||||||
| 11 | M Nov 9 | |||||||||
| W Nov 11 | ||||||||||
| F Nov 13 |
Detectors |
The Eye, Photographic Emulsions |
150-157 |
|||||||
| 12 | M Nov 16 | Photon-Counting Statistics |
158-161 |
|||||||
| W Nov 18 | CCDs |
162 |
||||||||
| F Nov 20 |
Basic Equations of |
Introduction, Black-body Radiation |
163-164 |
223-240 |
|
|||||
| 13 | M Nov 23 | The Boltzmann Equation |
165-166 |
|||||||
| T Nov 243 | ||||||||||
| W Nov 25 - F Nov 27 |
T H A N K S G I V I N G H O L I D A Y |
|
||||||||
| 14 | M Nov 30 |
Basic
Equations of |
The Maxwellian Kinematic Distributions | 167-169 | 14 | |||||
| W Dec 2 |
The Saha Equation Applications of the Boltzmann & Saha Equations |
170 | ||||||||
| F Dec 4 | ||||||||||
| 15 | M Dec 7 | Calculations of Pe(Pg,T ) | 171-172 | 15 | ||||||
| W Dec 9 | Semester Review | 0-172 | ||||||||
| F Dec 12 - S Dec 13 |
E X A M P R E P A R A T I O N D A Y S |
|||||||||
| 16 | T Dec 15 | F I N A L E X A M I N A T I O N (in classroom, 3:00 pm - 6:00 pm) | Final | |||||||
1Additional problem assignments may be added to this schedule as the semester progresses.
3By university policy, Friday classes are held on Tuesday, November 24.
2You may earn 5 points of extra credit by (1) attending the Neil deGrasse Tyson forum, (2) submitting to your instructor in class on September
23 a signed statement that you were in attendance, and (3) on your statement recounting at least three things you learned from Tyson's
presentation.
V
III. figures, tables and imagesThese are found on a separate webpage. Please click here.