Spacecraft observations have revealed a breathtaking diversity of geologic features in the solar system, such as the giant impact basins on Mars, towering thrust fault scarps on Mercury, coronae structures on Venus, and active volcanoes on Io and Enceladus. From a comparative perspective, this course examines the physical processes that drive the evolution of the planets and small bodies in the solar system. Topics include: planetary shape and internal structure, mechanisms of topographic support, tectonics, impacts, volcanism, and tides. Some class sessions are reserved for seminar-style discussions of journal articles. Students will produce a final project that involves researching a topic of their choosing.

Units: 1

Max Enrollment: 12

Crosslisted Courses: GEOS 313

Prerequisites: Any 100-level course in ASTR or GEOS in addition to at least one of the following - PHYS 107, GEOS 203, GEOS 218. An introductory course in mechanics (e.g., PHYS 104 or PHYS 107) is not required but is strongly recommended.

Distribution Requirements: MM - Mathematical Modeling and Problem Solving; NPS - Natural and Physical Sciences

Typical Periods Offered: Every other year

Semesters Offered this Academic Year: Fall; Not Offered; Spring