1. Wednesday 4:00 – 4:55pm Sundquist Science Center E-109 Dr. Spencer Buckner www.apsu.edu/astronomy

2. Office: SSC B – 326 (enter through B-332) Hours: MWF 10:15 – 11:30am and MWThF 1:30 – 2:30pm or by appointment Email: buckners@apsu.edu Phone: 221-6241

3. 21 st Century Astronomy: The Solar System, 4 th Edition, by Kay, Palen, Smith and Blumenthal If you don’t have the book, don’t go buy it since it isn’t required. Mostly we will just use the problems in the back of the chapters. There are old editions in the department library you can borrow.

4. Exams…………45%90 – 100…A Homework…….30%80 – 89…..B Projects………..20%70 – 79…..C Participation…….5%60 – 69…..D <60……….F

5. There will be three one-hour exams during the semester. The exams will be entirely problems similar to the homework problems. A formula sheet will be given out with the exam. Tentative exam dates are Wednesday September 23 Wednesday October 28 Wednesday December 9 A scientific calculator will be required for the exams

6. Homework will be assigned from the Student Questions at the back of each chapter in the 21 st Century Astronomy textbook. Additional problems from other sources will also be assigned to supplement the back-of-chapter questions. They will be due at the beginning of the next class meeting. First Homework set is due next week: Chapter 1 #46 & 50 plus Supplemental Problems Solutions to the homework will be posted in the class D2L shell a day or two after they are turned in.

7. There will be two projects assigned during the semester. The first project will be due September 30. The second project will be due at the final exam period Wednesday December 9. In addition to a written report, you will make a short (10-15 minute) oral presentation on your project.

8. First Project List is posted in Problems in Planetary Astro Stuff on www.apsu.edu/astronomy and in the Content section of the class D2L website.www.apsu.edu/astronomy NO REPEATS! First project presentations will be Wednesday October 21

9. How to work a problem Step 1: What are you trying to solve for? Step 2: What information are you given? Step 3: What equation(s) do you need to solve the problem? Step 4: Plug in the numbers and solve the problem Step 5: Check for reasonableness

10. Most objects viewed through a telescope have diameters measured in arcseconds. To calculate the linear diameter of such an object we can use the Small Angle Approximation applied to the formula for arclength (s = r  ). The result is the formula where the number 206,265 comes from dividing 360° in arcseconds by 2 . If Jupiter is observed to be 31.2 arcseconds wide when it is at a distance of 944 million kilometers, what is the actual diameter of the planet?

11. Answer the first two questions Step 1: What are you trying to solve for? What is the diameter of the planet Jupiter in kilometers? Step 2: What information are you given? Angular size of the planet (31.2”) and distance from Earth to Jupiter ( 944 million kilometers)

12. Step 3: what equation(s) do you need? Look for example problems in the chapter, in the appendix, in other textbooks or online. For this problem, it is given in the statement of the problem

13. Step 4: Plug in numbers and solve r = 944 x10 6 km  = 31.2” Significant figures: the final answer should never have more significant figures that the least number of significant figures in the numbers you start with.

14. Step 5: check for reasonableness In this case we can check the result with the value in the back of the textbook which gives the radius as 71,492 km

15. An Example for You Under excellent seeing conditions a good sized telescope on Earth can resolve angular details as small as 1 arcsecond. What is the greatest distance at which you could resolve a typical person (1.7 meters)?

16. Example for You Solution 1.What are you trying to find? Distance at which 1.7 meters subtends an angle of 1” 2.What information is given? Angle: 1” Linear size: 1.7 m 3.What equation is needed?

17. First rearrange the equation Next, plug and chug