Have you wondered what Earth's climate was like 3 billion years ago? What about weather patterns on Titan and climate change on Mars? In this course, we'll explore the structure and evolution of atmospheres and the climate on four worlds: the Earth, Mars, Venus, and Saturn's moon Titan. We'll examine the techniques and tools that geologists use to learn about the history of Earth's climate and that planetary scientists use to learn about the atmospheres and surface environments on other worlds. Students will also gain experience simulating the climate system and computing atmospheric properties. Other topics include: the super-rotation of Venus's atmosphere and its Runaway Greenhouse climate, the destruction of atmospheres on low-gravity worlds, and the future of Earth's climate as the Sun grows steadily brighter.

Units: 1

Max Enrollment: 20

Crosslisted Courses:

Prerequisites: MATH 116 and PHYS 107 and one of the following (ES 101, ASTR 100, ASTR 107, GEOS 101, or GEOS 102), or permission of the instructor.

Instructor: Watters

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

Typical Periods Offered: Every other year

Semesters Offered this Academic Year: Not Offered

Notes: