Slide 1 ASTR100 (Spring 2006) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106 Slide 2 Celestial Sphere Zenith: Point directly…

Slide 1 UNIT 4 – WEATHER DYNAMICS Slide 2 BOOK SECTIONS Chapter 13 – Getting started, 13.1, 13.2, 13.3, 13.4, 13.6, 13.8, 13.9, 13.1, 13.13, Chapter 14 – Getting started,…

Slide 1 Lecture Outline Chapter 2: Discovering the Universe for Yourself © 2015 Pearson Education, Inc. Slide 2 2.1 Patterns in the Night Sky Our goals for learning: What…

Observing the Universe for Yourself Patterns in the Night Sky What does the universe look like from Earth? Why do stars rise and set? Why do the constellations we see depend…

Planetary Shapes Non-rotating, self-gravating, strength-less objects would be spherical Rotating bodies, because of the centrifugal force of rotation, will be oblate spheres…

Class 3: End of Ch 2 and Ch. 3 Last time: 2.1. Patterns in The Sky: Stars and constellations, TODAY: celestial coordinates 2.2 Seasons,…Precession 2.2 (cont.). 2.3. The…

Chapter 2 Discovering the Universe for Yourself 2.1 Patterns in the Night Sky What does the universe look like from Earth? Why do stars rise and set? Why do the constellations…

Observing the Universe for Yourself Patterns in the Night Sky What does the universe look like from Earth? Why do stars rise and set? Why do the constellations we see depend…

Richard Avis: Mon. 1:30 [email protected] 7274526615 =) Jill Capano: Wed. 2PM [email protected] (845) 417 7605 Brendan Forte: Fri. 11:30 AM [email protected]…