Listed in: Physics and Astronomy, as ASTR-111
Kate Follette (Section 01)
What is the shape of the universe? How do stars die? What happens when galaxies collide? This course will provide an introduction to the nature and evolution of stars, our Milky Way galaxy, other galaxies, and the origin, size, shape and fate of the universe itself. We will explore how the fields of extragalactic astronomy and cosmology emerged and continue to evolve, and will touch on many of the big unanswered questions in these fields. Our investigations of galactic and extragalactic phenomena will focus on understanding proportionalities, relative sizes, and visual representations of data, as well as evaluating the reasonableness of quantitative answers rather than on lengthy calculations.
Limited to 60 students. Fall semester. Professor Follette.
How to handle overenrollment: 25 slots reserved for freshmen. Of the 35 remaining slots, preference given to seniors. All other slots filled by lottery.
Students who enroll in this course will likely encounter and be expected to engage in the following intellectual skills, modes of learning, and assessment: quantitative work and working in groups
Tu 02:30 PM - 03:50 PM SCCE A011
Th 02:30 PM - 03:50 PM SCCE A011
This is preliminary information about books for this course. Please contact your instructor or the Academic Coordinator for the department, before attempting to purchase these books.
|Lecture-Tutorials for Introductory Astronomy, 3rd Edition||Pearson; 3rd Edition||Edward E. Prather, Slater Timothy, Jeff Adams, Gina Brissenden||TBD|