PPT-Chapter 11: Our Star © 2015 Pearson Education, Inc.

111 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. 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”. : Jovian Planet Systems. © 2015 Pearson Education, Inc.. 8.1 A Different Kind of Planet. Our goals for learning:. What are jovian planets made of?. What is the weather like on jovian planets?. © 2015 Pearson Education, Inc.. 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”. in Action. Alan Evans . •. . Kendall Martin. Mary Anne Poatsy. Eleventh . Edition. Copyright © 2015 Pearson Education, Inc.. Technology in Action. Chapter 9. Securing Your System: . Protecting Your Digital Data and Devices. #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. 13.1 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.. Star-Forming Clouds. •. . 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.