Fall 2025 Graduate Courses

PTYS Graduate Core Course. Quantitative investigation of the physical processes controlling planet formation, the orbital and rotational dynamics of planetary systems, the mechanical and thermal aspects of a planetary interior, and the dynamics of the Earth-Moon and other satellite systems. Course requisites: Classical and quantum mechanics at the level of PHYS 151 and PHYS 242. Sample course syllabus, Matsuyama (PDF)

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. Equivalent to ASTR 518.

Classification; chemical, mineralogical and isotopic composition; cosmic abundances; ages; interaction with solar and cosmic radiation; relation to comets and asteroids. Prerequisite(s): PTYS 510. Identical to: GEOS 520. Usually offered: Spring.

Thermodynamics and its application to planetary atmospheres, hydrostatics, fundamental concepts and laws of dynamic meteorology. Identical to ATMO 541A. ATMO is home department.

This graduate course will focus on the use of radar remote sensing for studies of planetary surfaces, including rocky and icy objects.  It will cover the basics of how radar works including SAR and sounding (ground penetrating) radar, the use of different frequencies, an introduction to electromagnetic wave propagation including polarimetry, radar data processing, and the use of radar field equipment. The course will include a discussion of some of the past, current and future radars included on spacecraft and their design and science results. The course will be focused on geosciences; in particular, applications relevant to planetary processes such as regolith development, volcanism, cratering, fluvial deposits etc. This class includes 3 hours/week lecture plus a lab and fieldwork component. Cross-listed with GEOS 549; may be co-convened. PTYS is home department.

PTYS Graduate Core Course. The geologic processes and evolution of terrestrial planet and satellite surfaces including the Galilean, Saturnian, and Uranian satellites. Course includes one or two field trips to Meteor Crater or other locales. Identical to: GEOS 554. PTYS is home department. Usually offered: Spring. Sample course syllabus, Byrne (PDF)

This course will cover observational and theoretical ideas pertinent to planets orbiting other stars. Discovery and characterization techniques will be emphasized along with associated theory. In-class format will alternate from traditional lectures, guest lectures by local or visiting experts, and student-lead presentations.

This astrochemistry course is the study of gas phase and solid state chemical processes that occur in the universe, including those leading to pre-biotic compounds. Topics include chemical processes in dying stars, circumstellar gas, planetary nebulae, diffuse clouds, star-forming regions and proto-planetary discs, as well as planets, satellites, comets and asteroids. Observational methods and theoretical concepts will be discussed. Graduate-level requirements include a project and an oral exam. Identical to ASTR 588A; may be convened with ASTR 488A. ASTR is home department.

The acquisition of first-hand experience with geologic processes and features, focusing on how those features/processes relate to the surfaces of other planets and how accurately those features/processes can be deduced from remote sensing data. This is a three- to five-day field trip to an area of geologic interest where each student gives a short presentation to the group. This trip typically involves camping and occasional moderate hiking; students need to supply their own camping materials. Students may enroll in the course up to 10 times for credit. Trip is led by a Planetary Sciences faculty member once per semester. Alternative grading (SPF).