Course Web Site and Preliminary Syllabus

Introductory Astronomy: Solar System/Cosmology

Astronomy 102A, 101A and 101EA: Washburn University: 2005 Spring

Don't Panic

The course motto: very reassuring I think.


Instructor: Dr. David Jeffery, Stoffer Science Hall (ST), Rm 108a, Tel: 785-231-1010, ext 2144, Email: jeffery@physics.unlv.edu, Office hours: MTWRF 2:30--3:30 p.m., MW 6:00--6:30 pm (If you need to see the instructor for sure, make an appointment. I'm usually happy to see students at any time that I'm relatively free.)

Classes: Places and times.

  1. Stoffer 103, TR 1:00--2:15 pm (102A)
  2. Stoffer 101, TR 9:30--10:45 am (101A), MW 7:00--8:15 pm (101EA)
Warning: This syllabus is subject to change at the discretion of the instructor. Any changes will be announced in class as well a made on this page.

M31 (Andromeda Galaxy) and Moon










Current Course Sites
  1. Introductory Astronomy Web Lectures (IAWL) for the Solar System/Cosmology courses.
  2. Astronomy David Jeffery astronomy encyclopedia site: general physics, science, and technology are included too.
  3. Astronomy Links
  4. Marks and Grades Section 102A
  5. Marks and Grades Section 102A 2004 Fall
  6. Marks and Grades Section 101A
  7. Marks and Grades Section 101A 2004 Fall
  8. Marks and Grades Section 101EA
  9. Marks and Grades Section 101EA 2004 Fall
  10. Physics Links Look-up pages mainly.

University Sites
  1. Washburn University
  2. Washburn course catalogs past
  3. Washburn academic calendars
  4. Washburn academic calendar 2005 Spring
  5. mywashburn
  6. Student Services including Learning Disability Services
  7. Washburn EOP (Educational Opportunity Program Tutoring and mentoring help.
  8. Washburn University Netstation and Computer Lab Information for Students Fall 2004
  9. Washburn University Faculty Handbook
  10. Washburn University Policy on grades and grade points.
  11. Washburn Physics
  12. Washburn Physics, Crane Observatory



Syllabus Items

    Jump in with Questions? at any time, of course.

    Wait 15 seconds at least. (A self-note to the instructor.)

  1. Prerequisites: None.

  2. Breaks: These 75 minute classes are awful. So we will usually take a 5 minute---and only 5 minute---break at about the 40 minute mark.

  3. Web-Based Course: This is web-based course both for material and homeworks.

    But it is NOT a recognized Washburn on-line course.

    Students are TASKED with using/learning how to use campus computer resources if they don't yet know or have no home or other computer resources.

    Washburn's Information Technology Services (ITS) provides many facilities including computer labs and printers and assistance.

    If you do NOT have UNIX account you may need one. You can apply at the Bennett 104 dispatch window for login name and password: see ITS Quickfacts for more information---much more information---more than you ever wanted to know.

    Students can set up their own unofficial Washburn webpages. See Student Webpages. The URLs are all http://students.washburn.edu/studentusername I think.

    The instructor can also help people get started.

  4. Course Web Site: The course web site and preliminary syllabus URL is http://www.physics.unlv.edu/~jeffery/course/c_astint/index.html which is the page you are viewing right now.

    This page is linked from the official Washburn AS 102A/101A/101EA course page.

  5. Introductory Astronomy Web Lectures: These are a set of web lectures prepared by the instructor. They will be used as a lecturing tool and the substitute for a course TEXTBOOK, and are meant to be a replacement for student notes.

    Real TEXTBOOKS are always more material and more detail than a course can actually cover. That makes them a good resource, but a poor substitute for course notes for either the students or the instructor.

    The appropriate sequence of web lectures for the solar system/cosmology course are meant to be almost exactly the course and the course notes

    How much of the sequence of lectures for your course do you need to know?

    The short answer is all of it. The subject (see below) is extensive.

    Students do NOT need to take notes and, in fact, you CANNOT take complete notes though you may want to take some for staying-awake purposes.

    There is usually more on the screen than anyone can write down and still have the lecture flow along.

    In order for the lectures to replace a text, they have to be in full sentences and be wordier than ordinary lecture headings and points.

    Try not to be mesmerized by all the words on the screen---resist, RESIST.

    Alien mesmerized by words Alien mesmerized by words.

    In lecturing, the instructor will often focus on only images, any calculation, and key sentences. Often the instructor will skip over INDENTED or LINKED digressions.

    Some lectures or lecture sections might be omitted from a sequence. This depends on time and also relevance to the respective course.

    Students can download the lectures in text or some other format.

    It is recommended that you do NOT download them all at once.

    The web lectures have a tendency to SEEM perfected and that tends to inhibit questions from the students---we all have to work against that inhibition.

    Questions? 15 second wait at least.

  6. Optional Text for the Solar System/Cosmology Course: Discovering the Universe, 2003 edition, by Neil F. Comins & William J. Kaufmann III.

    This is a good book which covers the topics of both courses.

    Compared to the web lectures, sometimes its discussion is longer, sometimes shorter.

    Readings from the text that are comparable to the web lectures are specified. The text is closer to the web lectures for the Cosmology course.

    The web lectures are a bit more closely keyed to the questions I ask on tests, but I think comparable marks can be obtained either reading the web lectures or doing the textbook readings.

    The text can be recommended to students for whom downloading the homeworks is a sufficiency of downloading. The web lectures downloaded are just a messy sheaf of paper after all.

    Sometimes it's just a lot more convenient to have a compact, bound book in hand.

    The University Bookstore and Textbook Team (at 21st and Washburn Avenue, Suite 205) have lots of used copies to sell.

    But text has NO resale value since a new edition is coming out soon.

  7. Nature of the Course: This is an introductory astronomy course covering the solar system (102A)/the stars, galaxies, and cosmology (101EA/A).

    Great stuff if I say so myself.

    And to learn the course, it helps to appreciate the stuff.

    Physically, humankind is pretty minute in the universe. But amazingly we can look out from our little platform and see what certainly seems to be INFINITY and ETERNITY.

    ../../astro/astro1/lec000/infinity_eternity.png But as Dorothy said, there's no place like home.

    Earthrise Earthrise from Apollo 11, 1969jul16. Credit: NASA.

    Some general astronomy (e.g., the celestial sphere, lunar phases, etc.), BACKGROUND PHYSICS, and other material is also included.

    The BACKGROUND PHYSICS is essential: astronomy is based on physics. Our approach to the physics is largely qualitative. Concepts, including force, energy, and light, are introduced/reviewed.

    Alien consigning math to the flames Well not quite.

    There is a MATH COMPONENT to this course. Up to about 20 % of questions on tests may involve math. The rationale for this is to give some appreciation of the mathematical nature of astronomy.

    The math is multiplication and division with the odd square root or bit of algebra.

    For students who are unrefreshed in math, the math component may seem challenging.

    A math refresher is given for that reason as IAWL Lecture 1: Scientific Notation, Units, Math, Angles, Plots, Motion, Orbits

    The solar system and cosmology courses are very similar through the first three weeks or so.

    It is hoped that students will make progress in achieving some of skills in Washburn's General Educational Statement: The ability to

    1. read intelligently,
    2. reason mathematically and understand numerical data,
    3. process information both in terms of synthesis and analysis,
    4. solve problems using the methods of analysis considering evidence, relevance and validity.

    Is this a hard or an easy course?

    Somewhere in between in the instructor's view.

    There are NO course projects or essays and all tests and homeworks are multiple-choice questions.

    But there ARE a lot of things to learn: facts and concepts.

    Astronomy lore is EXTENSIVE: it goes on and on.

    It is hoped that the facts and concepts cohere into stories that are memorable, and so one knows the answer to a question because one knows the story into which the answer fits.

  8. Homeworks: Every lecture has an associated homework and set of homework solutions. See the Introductory Astronomy Web Lectures:

    Typically a homework is 5 to 30 multiple-choice questions.

    Homeworks are NOT handed in or marked.

    They are learning aids.

    Typically about 50 to 70 % of test questions will be drawn from the homeworks or, in the case of the FINAL, past tests also. The questions might be tweeked a bit.

  9. Exams: There will be 3 in-class exams and a 2-hour COMPREHENSIVE FINAL.

    The in-class exams cover the material up to some cut-off point that will be announced in class.

    The final is about 50% weighted on material since the 3rd in-class exam and about 50% weighted on all the material that came before the 3rd in-class exam.

    The tentative dates for the exams are:

          _________________________________________________________________
    
          Exam        101EA           101A            102A
          _________________________________________________________________
    
          Exam 1      Feb07 M         Feb08 T         Feb10 R  (tentative) 
          Exam 2      Mar07 M         Mar08 T         Mar10 R  (tentative)
          Exam 3:     Apr11 M         Apr12 T         Apr14 R  (tentative)
          Final Exam  May09 M 7:00pm  May10 T 9:00am  May10 T 1:30 pm 
          _________________________________________________________________
          

          _________________________________________________________________
          
    The in-class tests are worth 60 % of the final grade.

    Thus, they are worth 20 % each.

    The final is worth 40% of the final grade.

    The tests are all multiple-choice questions and scantrons are NOT used. An answer table will be provided. They are closed book; calculators are allowed.

    Students are asked to show a PHOTO ID when handing in tests.

    Make-up tests are possible, but students must ask for them promptly and avoid knowing anything about given tests in any section.

    In general, students who have not taken a given test must avoid knowing anything about that test given in other sections or to other people.

  10. Extra Credit: We have NO astronomy lab associated with this course.

    But it is good that students visit an observatory at some time during the course. It is just a good educational thing to do. It is good for your souls.

    I will give ONE EXTRA POINT on a test if a student visits an observatory DURING the semester and takes advantage of what is there to be seen.

    There are NO seconds: you only get ONE extra point.

    But that ONE could help if you end up near a grade boundary on the wrong side.

    The easiest observatory to visit is Washburn's Crane Observatory on the roof of Stoffer Science Hall.

    The Crane Observatory's schedule of open houses gives the times and dates. All days are thursdays.

    The Crane open houses are canceled if weather does NOT allow viewing.

    Other available observatories are the Clyde W. Tombaugh Observatory of the University of Kansas in Lawrence and the Farpoint Observatory in Wabaunsee County, Kansas run by the Northeast Kansas Amateur Astronomers League (NEKAAL). Public viewing is available at scheduled times.

    There may be observatories around or you may have a chance to visit one on a trip.

    Just inform the instructor that you have made an observatory visit and you will be given the extra credit point.

    If work or distance always precludes visiting Crane or any other observatory, I will just give you the extra credit.

    There is NO other extra credit with this course.

  11. Evaluation and Grading: The 2 grading categories, their weightings, and their drops are:
    
          3 in-class tests        60 %      no drop
          1 comprehensive final   40 %      no drop
    
          
    Letter grades will be assigned following the Washburn Faculty Handbook grade rules.

    The rules say the average grade is to be a C and that's the way it will be.

    But the rules permit some freedom since ``excellent,'' ``well above average,'' ``below average but passing,'' and ``failure'' are not precisely defined.

    During the semester current letter grades are assigned in an automated fashion according the BELL CURVE---which physicists call a Gaussian.

    
          
    Grade Distribution of a Bell Curve
    Grade Percentage of Standard deviations from mean a bell-curve class for each grade bin. in each grade bin A standard deviation is the statistical width of the distribution
    A 10 % 1.28 B 25 % 0.38 C 45 % -0.84 D 15 % -1.64 F 5 % 0. The bell curve grade point average is 2.20.
    The actual class will not usually have exactly this breakdown because the class distribution will not be exactly a bell curve.

    There is for instance NO need for F's at all.

    At the end of the semester the instructor will make a FINAL grade decision.

    The instructor will NOT lower a grade from the BELL CURVE assignment: the instructor might raise it depending on several things including:

    1. Did a student improve on the course final?
    2. Is there a good gap in percentages in which to draw a grade line?

    But students should count on anything.

    Just do your best all along---subject to all the other constraints in life.

    Aliens and Grades Beware of aliens bearing grades.

  12. Posting Grades: Student marks and grades will be posted at the course web site (i.e., above) under an anonymous alias only if the student requests this.

    If you desire a web posting of marks and grades, give an anonymous alias on the fun quiz: you only need to hand it in if you want GRADE POSTING. Follow the given alias rules.

    The alias is ONLY for grade posting. You don't put it on things you hand in and I won't recognize you by it.

    You can, of course, give an alias at any time.

    I do recommend that you ask for GRADE POSTING since experience shows students, particularly as the semester nears the end, do want to know what they've gotten.

  13. Disability Services: The Student Services/Services for Students with Disabilities Office (SSWDO) is responsible for assisting in arranging accommodations and for identifying resources on campus for persons with disabilities. Qualified students with disabilities must register with the office to be eligible for services. SSWDO MUST have documentation on file in order to provide services. Accommodations may include in-class notetakers, test readers and/or scribes, adaptive computer technology, brailled materials. New requests for accommodations should be submitted two months or more prior to the date services should begin; however, contact SSWDO as soon as a need may arise.

    1. Location: Student Services, Morgan Hall-Room 150
    2. Phone: 785-231-1010, ext 1629 (may leave voice mail 24 hrs/day) or TDD: 785-231-1025
    3. Web Site: Student Services including Learning Disability Services

    Students may voluntarily identify themselves to the instructor for a referral to SSWDO.

  14. Sequence of Lectures: No dated schedule has ever been adhered to by the instructor.

    Thus we will just look over the sequence of lectures/topics appropriate to the Solar System and Cosmology courses before we dig in.

    Some lectures/topics may be omitted from either sequence in order to complete the most important lectures/topics.

    Questions? 15 second wait at least.

    On with the show: Introductory Astronomy Web Lectures (IAWL) for the Solar System/Cosmology courses.