Astrophysical and Dynamical Processes in Planetary Sciences

Astrophysical and Dynamical Processes in Planetary Sciences is a course that challenges students to use physical and geophysical analysis to construct a quantitative understanding of the formation and evolution of the Sun, the solar system’s planets and small bodies, and extrasolar planets. The goal is to provide senior undergraduate and first-year graduate students with core knowledge of facts and current theories in the planetary sciences. Through lectures, problem sets, and exams, the students will construct quantitative framework on which to evaluate, and place into context, hypotheses and theories discussed in upper-level graduate courses. Prerequisites: MATH 0100 ; and one of EEPS 0050 , PHYS 0210, 0220 , or 0270 . APMA 0330 is desirable but not required.