||Title & Description
Instrumentation and Statistics (3)
Radiant energy; signals and noise; detectors and techniques for imaging, photometry, polarimetry and spectroscopy. Examples from stellar and planetary astronomy in the x-ray, optical, infrared and radio. ASTR is home department. May be convened with: ASTR/PTYS 518.
Course page: PTYS 418 (001) Rieke
Dynamic Meteorology (3)
Thermodynamics and its application to planetary atmospheres, hydrostatics, fundamental concepts and laws of dynamic meteorology. Prerequisite: PHYS 426 or consent of instructor. ATMO is home department.
Planet Earth: Evolution of the Habitable World (3)
This course develops a planetary perspective on the evolutionary processes that shaped Earth throughout history. We will examine why Earth is habitable, that is, why any kind of life can live on it, we will discuss the unique influences that biological processes and atmosphere/ocean systems have on each other, and we will review current notions of climate change, including evidence for the influence of human activities on it. This interdisciplinary treatment of Earth and its sister planets will encourage students to think about how science and engineering must be applied to today's challenges if humankind is to have a promising future on (and off) this planet. PTYS 170A1 is a Tier I Natural Science course in the University's general education curriculum. This course is co-convened (cross-listed) with ASTR 170A1.
Course page: PTYS/ASTR 170A1 (001) Matsuyama
The Universe and Humanity: Origin and Destiny (3)
The Universe And Humanity: Origin And Destiny places Earth and humanity in a broad cosmic context. Topics range from the Big Bang cosmology to human consciousness with emphasis on the events and evolutionary processes that define the physical universe and our place in it. PTYS 170B2 is a Tier I Natural Science course in the University's general education curriculum. This course is co-convened (cross-listed) with ASTR 170B2.
Course page: PTYS/ASTR 170B2 (001) Holberg is D2L
First Year Colloquium (1)
Freshmen and other first year students are encouraged to enroll in one-unit First Year Colloquia that allow for in-depth exploration of a science topic. Colloquia feature lively discussion and class participation. Topics vary by semester (e.g., "The Changing Sun and its Influence on Earth: Does the Sun's natural variability affect climate on Earth?" and "Why do we have a space program?"). For further information, contact the Department of Planetary Sciences.
Course page: PTYS 195A (001) Jokipii The Nature of Time
Our Golden Age of Planetary Exploration (3)
PTYS 206 emphasizes the part of the universe that is within reach of direct human experience and exploration. We will review current understanding of the contents of our Solar System and emphasize the processes that unite all of the planets and smaller bodies, such as tectonics, weathering, cratering, differentiation, and the evolution of oceans and atmospheres. The course will build on this knowledge to understand humankind's motivation to explore beyond our Solar System, especially to search for planets around distant stars and to look or listen for evidence of life elsewhere in the Universe. PTYS 206 is a Tier II Natural Science course in the University's general education curriculum. PTYS 206 is cross-listed with ASTR 206. Course requisites: Two courses from Tier One, Natural Sciences.
Course page: PTYS/ASTR 206 (001) Kortenkamp is D2L
Course page: PTYS/ASTR 206 (002) Hubbard
Chemistry of the Solar System (3)
Abundance, origin, distribution, and chemical behavior of the chemical elements in the Solar System. Emphasis on applications of chemical equilibrium, photochemistry, and mineral phase equilibrium theory. Prerequisites: CHEM 152, MATH 125b, and PHYS 132 or their equivalents. PTYS 407 is required for the PTYS Minor. PTYS 407 is equivalent to CHEM 407 (not cross-listed).
Course page: PTYS 407 (001) Zega
Origin of the Solar System and Other Planetary Systems (3)
This course will review the physical processes related to the formation and evolution of the protosolar nebula and of protoplanetary disks. In doing that, we will discuss the main stages of planet formation and how different disk conditions impact planetary architectures and planet properties. We will confront the theories of disk evolution and planet formation with observations of circumstellar disks, exoplanets, and the planets and minor bodies in our Solar System. This course may be co-convened with PTYS/ASTR 550.
Course page: PTYS 450 (001) Pascucci is D2L