2021 Spring

Physics of the Solar System (3)

Survey of planetary physics, planetary motions, planetary interiors, geophysics, planetary atmospheres, asteroids, comets, origin of the solar system. Graduate-level requirements include an in-depth research paper on a selected topic and an oral class presentation. This course does not count toward the major requirements in Planetary Sciences. Equivalent to: ASTR 503, GEOS 503, and PHYS 503 (and cross-listed); may be co-convened with PTYS 403. PTYS is home department.

(001) Yelle | D2L | Syllabus

Mars (3)

In-depth class about the planet Mars, including origin and evolution, geophysics, geology, atmospheric science, climate change, the search for life, and the history and future of Mars exploration. There will be guest lectures from professors and research scientists with expertise about aspects of Mars. There will be lots of discussion of recent results and scientific controversies about Mars. Graduate-level requirements include the completion of a research project that will be presented in class as well as a report. The research project could be analysis of Mars datasets, a laboratory experiment, or new theoretical modeling. Regular grades are awarded for this course: A B C D E. Prerequisite(s): PTYS 411, Geology of the Solar System is strongly recommended but not required. Identical to: ASTR 542, GEOS 542. May be convened with: PTYS 442.

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) Kortenkamp | D2L | Syllabus

Core Course

Chemistry of the Solar System (3)

PTYS Graduate Core Course. Provides an overview of the gas and ice chemistry in planetary environments including molecular structure, spectroscopy, kinetics. The course describes how these physical processes are manifest in the diverse solar system environments. The instructional level is aimed at beginning graduate students with an adequate background comparable to that obtained from advance undergraduate courses in physics and chemistry. Knowledge of vector calculus and elementary differential equations is assumed. Successful students will be able to understand current research in planetary chemistry and will be well prepared for more detailed studies.
Sample course syllabus, Pascucci (PDF)

 

(001) Pascucci | D2L | Syllabus

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) Barnes | D2L | Syllabus

Core Course

Atmospheres and Remote Sensing (3)

PTYS Graduate Core Course. Structure, composition, and evolution of atmospheres; atomic and molecular spectroscopy; radiative transfer and spectral line formatting.
Sample course syllabus, Griffith (PDF)
Sample course syllabus, Yelle (PDF)

(001) Griffith | D2L | Syllabus

Mars (3)

In-depth class about the planet Mars, including origin and evolution, geophysics, geology, atmospheric science, climate change, the search for life, and the history and future of Mars exploration. There will be guest lectures from professors and research scientists with expertise about aspects of Mars. There will be lots of discussion of recent results and scientific controversies about Mars. Graduate-level requirements include the completion of a research project that will be presented in class as well as a report. The research project could be analysis of Mars datasets, a laboratory experiment, or new theoretical modeling. Regular grades are awarded for this course: A B C D E. Prerequisite(s): PTYS 411, Geology of the Solar System is strongly recommended but not required. Equivalent to/crosslisted: ASTR 442, GEOS 442. May be convened with: PTYS 542.

Physics of the Solar System (3)

Survey of planetary physics, planetary motions, planetary interiors, geophysics, planetary atmospheres, asteroids, comets, origin of the solar system. Prerequisites: PHYS 142 or 251. PTYS 403 is a required course for the PTYS Minor. Equivalent to ASTR/GEOS/PHYS 403.

(001) Yelle | D2L | Syllabus

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).

(001) Asphaug | Syllabus

Spring 2021, PTYS 595B (001), Asphaug, PLANET-FORMING COLLISIONS, 3 units

(002) Malhotra | D2L | Syllabus

Spring 2021, PTYS 595B (002), Malhotra, ADVANCED DYNAMICS, 3 units

(003) Lauretta | D2L | Syllabus

Spring 2021, PTYS 595B (003), Lauretta, 3 units. Spacecraft Mission Design and Implementation.

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.

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.

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 | Syllabus

Remote Sensing of Planetary Surfaces (4)

This graduate course will focus on the use of remote sensing in the study of rocky and icy planetary surfaces.It is not a science course, but rather intended to provide technical knowledge of how instruments work and practical techniques to deal with their datasets. In this course, we will cover how different types of remote-sensing instruments work in theory and practice along with case studies (student-led) of specific planetary science instruments.  We will discuss what datasets are generated by these instruments, their limitations and where they can be located. Lab sessions will provide experience in how these data are processed, visualized and intercompared. The class consists of two lectures and a 2.5-hour lab session each week. Cross-listed with GEOS, equivalent to GEOS 551.

(001) Byrne | D2L | Syllabus

(01A) Byrne | D2L | Syllabus

Nanoscale Analysis of Materials Using Transmission Electron Microscopy (3)

This course discusses the theory and practice of transmission electron microscopy as applied crystalline solids. Among the topics to be covered include electron scattering and diffraction, image formation, energy-dispersive X-ray spectroscopy and electron energy-loss spectroscopy. Weekly lectures will be accompanied by several laboratory practical sessions. Emphasis will be placed on quantitative analysis of material structure and composition as well as the identification of unknown materials. Equivalent to: MSE 526; PTYS is home department.

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

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

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) Psaltis

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) Ozel

Methods in Computational Astrophysics (3)

The course is a "hands-on" introduction to computer use for research by scientists in astrophysics and related areas. The course begins with a survey of and introduction to tools available on Linux systems, web-based tools, and open-source software widely used in astrophysics. Standard methods for integration, iteration, differential and difference equations, and Monte Carlo simulations, are discussed, in one to four dimensions. Historically important methods of radiative transfer, reaction networks, and hydrodynamics are presented, and contrasted with presently-used methods. Parallel programming is introduced, and discussed in terms of new and future computer systems. Special topics are added to reflect new developments. The course is task-oriented, with individual and team work projects, and class participation determining grades. Most of the work is done on the student's own personal computer (Linux or Mac operating systems are preferred). Identical to ASTR/PHYS 596B. ASTR is home department. Equivalent to ASTR 596B and PHYS 596B; ASTR is home department. Typically Offered Spring. Regular or Alternative Grades: ABCDE or SPF.

(001) Pinto

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) Lauretta | D2L | Syllabus

3 units. Spacecraft Mission Design and Implementation.

Description of Course

This course will provide an overview of NASA and international planetary exploration. The focus is on the development and implementation of planetary robotic exploration missions. The instructor is the Principal Investigator for the NASA OSIRIS-REx mission, which successfully collected a sample from near-Earth asteroid Bennu in October 2020. All aspects of mission development and operations will be covered including political, scientific, engineering, management, and resources.

Course Format and Teaching Methods

The course will be a combination of seminar-style lectures, assigned reading, and group projects. The group projects will focus on the development of science and engineering requirements and design for a planetary exploration mission. Final grades will be calculated based on classroom attendance, participation in in-class discussion, and the quality of the work demonstrated in the group-project reports.

Course Objectives and Expected Learning Outcomes

The primary outcome of this course is for the students to gain an understanding of all aspects of planetary mission design. Spacecraft mission development will be presented as a multi-faceted challenge that involves political processes, scientific investigation, engineering disciplines, and project management.

Astrochemistry (3)

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.

(001) Lucy Ziurys

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 | Course Page

PTYS 297A (001) for Spring 2021 is Flex In-Person.

(002) Kortenkamp, Edwards | Course Page

PTYS 297A for Spring 2021 is online only, iCourse.

(003) Kortenkamp, Edwards | Course Page

PTYS 297A (003) for Spring 2021 is Flex In-Person.

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 | Course Page

PTYS 393 (001) for Spring 2021 is Flex In-Person.

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 | Course Page | Syllabus

PTYS 397A (001) for Spring 2021 is Flex In-Person.