PPT-Chapter 13 : Star Stuff © 2015 Pearson Education, Inc.

131 Star Birth Our goals for learning How do stars form How massive are newborn stars 2015 Pearson Education Inc How do stars form 2015 Pearson Education Inc StarForming Clouds. Syllabus: . http://www.astro.umn.edu/courses/1001/syllabi/. Lecture notes: . http://www.astro.umn.edu/courses/1001/lecnotes/. Exams: . http://www.astro.umn.edu/courses/1001/examsched.html. Everything: http://www.astro.umn.edu/courses/1001/. Grades are posted on course website. Average = . 127/180, . s.d. . = . 26 (Section 1). 132/180, . s.d. . = 24 (Section 4). Highest . 180/. 180. Scores below 100 => “serious concerns”. 001). The First Midterm is Tuesday. , . February 24. The First Midterm will be given . in two rooms. A – J Physics 166 (this room). K – Z Anderson 270 (West Bank). Bring 2 pencils and a photo-id.. Surveying the Stars. © 2015 Pearson Education, Inc.. 12.1 Properties of Stars. Our goals for learning:. How do we measure stellar luminosities?. How do we measure stellar temperatures?. How do we measure stellar masses?. #2 . Grades are posted on course website. Average = . 122/. 180, . s.d. . = . 29 . (Section 1). . 126/. 180, . s.d. . = 24 (Section 4). Highest . 180/. 180. Scores below 100 => “serious concerns”. 001). The Final Exam is. . Thurs. day. ,. . December. 22, 8:. 0. 0 . – . 10:. 0. 0 . a. m. The Final Exam will be given . in. :. Willey 175. Don’t come to Anderson 210. No one will be there. No one.. #2 . Grades are posted on course website. Average = . 126/180, . s.d. . = . 27 (Section 1). 124/180, . s.d. . = 27 (Section 2). Highest . 174/. 180. Scores below 100 => “serious concerns”. Chapter 11 The Interstellar Medium. © 2017 Pearson Education, Inc.. Units of Chapter 11. Interstellar Matter. Star-Forming Regions. Dark Dust Clouds. Formation of Stars Like the Sun. Stars of Other Masses. Systems . The New Science of Distant Worlds. © 2018 Pearson Education, Inc.. 10.1 Detecting Planets Around Other Stars. Our goals for learning:. How do we detect planets around other stars?. © 2018 Pearson Education, Inc.. Chapter 14 Oscillations. Chapter Goal: . To understand systems that oscillate with simple harmonic motion.. © 2015 Pearson Education, Inc.. Chapter 14 Preview. Looking Ahead: Motion that Repeats. . Chapter Goal: To extend the description of motion in one dimension to include changes in velocity. This type of motion is called . acceleration. .. © 2015 Pearson Education, Inc. . Chapter 3: Acceleration. 11.1 A Closer Look at the Sun. Our goals for learning:. Why does the Sun shine?. What is the Sun. '. s structure?. © 2015 Pearson Education, Inc.. Why does the Sun shine?. © 2015 Pearson Education, Inc.. •. . Kendall Martin. Mary Anne Poatsy. Eleventh . Edition. Copyright © 2015 Pearson Education, Inc.. Technology in Action. Chapter 3. Using the Internet: . Making the Most of the Web’s Resources. •. . Kendall Martin. Mary Anne Poatsy. Eleventh . Edition. Copyright © 2015 Pearson Education, Inc.. Technology in Action. Chapter 3. Using the Internet: . Making the Most of the Web’s Resources.