2019 Spring

Life on Mars: Fact and Fiction (3)

Life on Mars is likely to be a scientific "hot topic" for the rest of your life. After this class, you should have a good understanding of what planetary scientists think about the chances of life on Mars, why they think that, and how current and future spacecraft missions plan to address that. In addition, since life on Mars has been the subject of some classic science fiction for more than 100 years, with no signs of letting up, you should understand how that science fiction relates to science. My real goal is that as the current debate resolves itself, and as spacecraft explore Mars during the next few decades, you'll understand what's going on and which claims are important, and that as you read or watch science fiction dealing with Mars, you'll appreciate how it relates to past and present science and sci-fi. PTYS 342 may not be applied toward the PTYS undergraduate minor.

Exoplanets: Discovery and Characterization (3)

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.

(001) Barman | 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, Showman (PDF)
Sample course syllabus, Yelle (PDF)

(001) Showman | 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)

 

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).

Astrobiology: A Planetary Perspective (3)

We will explore questions about the origin, evolution, and future of life on Earth and the possibility of life arising independently elsewhere in the Universe. We will examine what it means for a planet to be habitable, both in terms of basic necessities for living organisms to function and environmental limits to their ability to survive. Finally, we will review different approaches for searching for life within the Solar System and beyond using direct and remote sensing techniques. PTYS 214 is a Tier II Natural Science course in the University general education curriculum. PTYS 214 is cross-listed with ASTR 214 and GEOS 214. Course is equivalent to ASTR 202 (students may not receive credit for both courses).

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.

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.

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.

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. Equivalen to ASTR/GEOS/PHYS 403.

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.

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) McEwen | Course Page | Syllabus

This 1-credit class will be a seminar on the Galilean satellites of Jupiter, four large worlds with complex orbital, tidal, and magnetospheric interactions.  The course objective is for students to gain a first-order understanding of these worlds, and a more detailed understanding of some aspect of these satellites.

(002) Asphaug | Syllabus

PTYS 595B (002), 3 units, Planet-Forming Collisions. The terrestrial planets grew in a series of massive late-stage collisions. Unlike impact cratering there is no impact locus when the colliding bodies are similar-sized, and the process is governed by angular momentum and self-gravity as much as by shocks and equations of state. The first half of the course will be lecture-based providing an essential background leading up to the major current science questions, and the second half will be focused on research projects culminating in final presentations. 

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) Eisner/Apai

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) Castro

High Energy Astrophysics (3)

A study of pulsars, black holes, accretion disks, X-ray binaries, gamma-ray sources, radio galaxies, active galactic nuclei, and the acceleration of charged particles near these objects, together with the radiation mechanisms they employ to produce the high-energy emission we detect at Earth. This course is identical to ASTR/PHYS 582. ASTR is home department.

(001) Ozel

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) Ziurys