2022 Spring

Stars and Planets (3)

This course will explore the physical principles that govern the structure and evolution of stars and planets. Topics covered will include stellar structure, energy generation and transport, and equations of state. Applying physical models and computational methods, fundamental properties of stars and planets will be derived, and compared with observational constraints. Identical to: ASTR 545; ASTR is home department. Usually offered: Fall.

(001) Smith

Core Course

Cosmochemistry (3)

PTYS Graduate Core Course. This course discusses the chemical processes important for the formation of our solar system and that subsequently acted on the objects within the solar system. It also discusses nuclear processes responsible for synthesis of the elements and alteration of isotopic abundances. Sample course syllabus, Zega (PDF)Sample course syllabus, Barnes (PDF)

(001) Barnes, Haenecour | D2L

Meteorites (3)

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.

(001) Reddy | D2L

Planetary Materials (3)

This course discusses chemical thermodynamics and applies it to the origins and history of primitive planetary materials. The types of planetary materials will be discussed together with an overview of the chemical setting of their origins. We will discuss thermodynamic formalism, the various chemical pathways through which planetary materials are believed to have formed, the characterization and numerical methods we use to quantify such origins, and we will consider several case studies. May be co-convened with PTYS 513.

(001) Muralidharan, Zega | D2L

Planetary Materials (3)

This course discusses chemical thermodynamics and applies it to the origins and history of primitive planetary materials. The types of planetary materials will be discussed together with an overview of the chemical setting of their origins. We will discuss thermodynamic formalism, the various chemical pathways through which planetary materials are believed to have formed, the characterization and numerical methods we use to quantify such origins, and we will consider several case studies. Course may be co-convened with PTYS 413.

(001) Muralidharan, Zega | D2L

Core Course

Solar System Dynamics (3)

PTYS Graduate Core Course. Dynamical processes affecting the orbital evolution of planets, asteroids, and satellites, and the rotational evolution of solid bodies. Emphasizes modern nonlinear dynamics and chaos. Identical to ASTR 553. PTYS is home department. Sample course syllabus, Malhotra (PDF)

(001) Malhotra | D2L

Geology and Geophysics of the Solar System (3)

Geologic processes and landforms on satellites and the terrestrial planets, their modification under various planetary environments, and methods of analysis. PTYS 411 is equivalent to GEOS 411 and HWRS 411 (cross-listed). PTYS 411 is required for the PTYS Minor.

(001) Hamilton | D2L

Introduction to Plasma Physics (3)

The purpose of this course is to present an introduction to the physics of plasmas. Topics include fundamental plasma scales and interactions, single particle motion, magnetohydrodynamic and fluid models, linear waves, kinetic theory, plasma stability, magnetic reconnection, and non-linear processes. The roles of these processes are considered in a variety of systems, including the Sun and stars, their extended atmospheres, planetary magnetospheres, and laboratory devices.  The emphasis throughout will be on basic physical processes and the various approximations used in their application to realistic and relevant problems. The graduate course is identical to ASTR/ATMO/PHYS 514, with PTYS as the home department.

(001) Klein | D2L

Introduction to Plasma Physics (3)

The purpose of this course is to present an introduction to the physics of plasmas. Topics include fundamental plasma scales and interactions, single particle motion, magnetohydrodynamic and fluid models, linear waves, kinetic theory, plasma stability, magnetic reconnection, and non-linear processes. The roles of these processes are considered in a variety of systems, including the Sun and stars, their extended atmospheres, planetary magnetospheres, and laboratory devices. The emphasis throughout will be on basic physical processes and the various approximations used in their application to realistic and relevant problems. The graduate course is identical to ASTR/ATMO/PHYS 514, with PTYS as the home department.

(001) Klein | D2L

Special Topics in Planetary Science (2-3)

Course will emphasize emerging and current topical research in Planetary Science; course will be offered as needed or required.  Sample course topics might include an active spacecraft mission, an emerging research area, or new discoveries.  Course may be co-convened with PTYS 595B. Graduate-level requirements may include an additional project for graduate credit and extra questions on exams, depending on the course/topic taught. Course may be repeated for credit 3x (or up to 9 units).

(001) Carter | D2L

Spring 2022, PTYS 495B 3 units, Writing for Science.

Special Topics in Planetary Science (1-4)

Course will emphasize emerging and current topical research in Planetary Science; course will be offered as needed or required.  Sample course topics might include an active spacecraft mission, an emerging research area, or new discoveries.  Course may be co-convened with PTYS 495B. Graduate-level requirements may include an additional project for graduate credit and extra questions on exams, depending on the course/topic taught. Course may be repeated for credit 4x (or up to 12 units). Regular grades assigned (ABC).

(003) McEwen | D2L

Spring 2022, PTYS 595B (003), is 1 unit, Galilean Satellites.

(001) Barnes, Haenecour | D2L

Spring 2022, PTYS 595B (001), is 1 unit, Writing in Planetary Science: Cosmochemistry.

(002) Matsuyama | D2L

Spring 2022, PTYS 595B (002), is 3 units, Statistics.

Planetary Geology Field Studies (1)

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. Altnerative grading (SPF).

(001) Byrne | D2L

Exploring Our Solar System (3)

Our Solar System is filled with an incredible diversity of objects. These include the sun and planets, of course, but also many hundreds of moons—some with exotic oceans, erupting volcanoes, or dynamic atmospheres. Billions of asteroids and comets inhabit the space between and beyond the planets. Each body is unique, and has followed its own evolutionary history. This class will explore our current understanding of the Solar System and emphasize similarities that unite the different bodies as well as the differences between them. We will develop an understanding of physical processes that occur on these bodies, including tectonics, impact cratering, volcanism, and processes operating in their interiors, oceans, and atmospheres. We will also discuss planets around nearby stars and the potential for life beyond Earth. Throughout the class, we will highlight the leading role that the University of Arizona has played in exploring our Solar System.

Course Objectives: Students who engage with this course will develop a broad understanding of many fundamental concepts in planetary science and gain an appreciation for the discoveries and reasoning that leads to this understanding. They will learn to collect their own data as well as gather relevant supporting information from a variety of outside sources. Throughout the semester students will be demonstrating their grasp of course material by composing written assignments at a level their peers outside of the class will understand (a.k.a., Students on the Street, or SOS). During the term project students will be assisted in working with telescopes to obtain astronomical images using their own smart phone cameras. Students will learn during in-class workshops how to use their own images to then construct a time-lapse animation. Expected Learning Outcomes: Upon successful completion of this course students will be able to (1) access and use information and data from a variety of sources, including their own activities, (2) critically evaluate this information and data for reliability in supporting fundamental concepts, (3) effectively communicate an understanding of these concepts to their SOS peers by synthesizing the information and data they have gathered, (4) demonstrate practical skills with a variety of software, including Word, Excel, Keynote, PowerPoint, and image/video editing apps.

PTYS 206 is cross-listed with ASTR 206. Course requisites: Two courses from Tier One, Natural Sciences.

(001) Andrews-Hanna | D2L

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.

(001) Marley | D2L

Physics of High Atmospheres (3)

Physical properties of upper atmospheres, including gaseous composition, temperature and density, ozonosphere, and ionospheres, with emphasis on chemical transformations and eddy transport. Identical to ATMO 544. PTYS is home department.

(001) Koskinen | D2L

Planetary Surface Processes Seminar (1)

This seminar course will focus on discussion of planetary surfaces and their evolution, including geology of rocky planets and moons, icy surfaces and moons, regolith development, surface-atmosphere interactions, sub-surface structure and interiors, and climate change. The course will involve the exchange of scholarly information in a small group setting, including presentations and discussions of student research, reviews of recent science results and discussion of proposal ideas. Students will be expected to lead 1 to 2 presentations and participate in group discussions. This course is intended for graduate students; senior undergraduates may be able to enroll with permission of the instructor. Alternative Grading S, P, F; may be repeated for 10 completions/units.

(001) Carter | D2L

Teaching Teams Professional Development Workshop (3)

Professional development for undergraduates of all disciplines in areas of peer instruction and mentoring, leadership, public speaking, group dynamics, and interview skills; also assists students with preceptorships.

(001) Kortenkamp, Edwards | D2L

Teaching Teams Internship (3)

Internship for students who have completed PTYS 297A (formerly LASC 297A), with at least one semester as a preceptor of a university-level course) to continue their reaching team education. Course covers elements of learning environments, communication skills, providing feedback, performance evaluation, and cooperative learning strategies.

(001) Kortenkamp, Edwards | D2L

Professional Development in a Digital Age (2-3)

Professional development in areas that are affected by transition to digital formats. Students will learn about elevator pitches, communication, utilizing professional technologies, resumes and curriculum vitaes, online resumes and portfolios, professionalism within social media, searching for jobs online, and interviewing.

(001) Kortenkamp, Edwards | D2L

Advanced Teaching Teams Internship (3)

This advanced internship is for students who have completed PTYS 393. Course covers elements of learning environments, communication skills, providing feedback, performance evaluation, and cooperative learning strategies; it requires students to peer lead workshop sections within the Teaching Teams Program alongside a faculty/staff mentor.

(001) Kortenkamp, Edwards | D2L

Planetary Astrobiology (3)

This course will explore the processes related to planet formation, the properties of planets and the planetary conditions required for the emergence of life. We will study the formation of our Solar System and exoplanetary systems, the distribution and properties of exoplanets, and the potential habitability of other planets/moons in our system or extrasolar systems. The course will also review science cases and possible future astrobiology studies, both in site and via remote sensing, of astrobiologically relevant environments. Toward the end of the semester a few guest lectures will highlight particularly exciting and timely topics. This course may be co-convened with ASTR/PTYS 575.

(001) Apai

Planetary Astrobiology (3)

This course will explore the processes related to planet formation, the properties of planets and the planetary conditions required for the emergence of life. We will study the formation of our Solar System and exoplanetary systems, the distribution and properties of exoplanets, and the potential habitability of other planets/moons in our system or extrasolar systems. The course will also review science cases and possible future astrobiology studies, both in site and via remote sensing, of astrobiologically relevant environments. Toward the end of the semester a few guest lectures will highlight particularly exciting and timely topics. This course is identical to ASTR 575; may be co-convened with ASTR 475. ASTR is home department.

(001) Apai

Writing Across the Space Sciences (3)

The purpose of this class is to strengthen the writing skills of the student along the entire range of writing, from technical scientific writing in the space sciences to popular articles about science. It has the secondary purpose of preparing the student for the wide variety of occasions when communication skills, written and verbal, will be required in the professional practice of the space sciences. Typically offered: Fall. ASTR is home department.

(001) Besla

Dynamic Metereology (3)

Thermodynamics and its application to planetary atmospheres, hydrostatics, fundamental concepts and laws of dynamic meteorology. Graduate-level requirements include a more quantitative and thorough understanding of the subject matter. ATMO is home department.

(001) Atallah

Boundary Layer Meteorology & Surface Processes (3)

Designed for students in the atmospheric sciences, hydrology and related fields. It provides a framework for understanding the basic physical processes that govern mass and heat transfer in the atmospheric boundary layer and the vegetated land surface. In addition to the theoretical part of the course, there is a strong focus on modeling and students will be required to program numerical codes to represent these physical processes. Course may be repeated for a maximum of 6 unit(s) or 2 completion(s). Also offered as: ATMO 579, ENVS 579, HWRS 579, WSM 579. ATMO is home department.

(001) Zeng