CORE
COURSES
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Fall Semester |
Spring Semester |
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Year 1 |
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ASTR 522: Atomic & Molecular Astrophysics |
ASTR 515: Interstellar Medium & Star Formation |
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ASTR 540: Structure & Dynamics of Galaxies |
ASTR 541: Extragalactic Astronomy & Cosmology |
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Year 2 |
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ASTR 545: Stellar Atmospheres |
ASTR 535: Stellar Structure |
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ASTR 518: Instrumentation & Techniques |
ASTR 582: High Energy Astrophysics |
ELECTIVES |
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Fall Semester |
Spring Semester |
| ASTR 589: Theoretical
Astrophysics |
Astr 587: Nuclear Astrophysics |
| ASTR 569: Introduction to
General Relativity |
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| Astro 585: Radio Astronomy | |
518. Modern Astronomical
Instrumentation and Techniques
(3) I 2001-02 For a description of course topics, see 418.
Graduate-level requirements include an in-depth research paper.
(Identical with PTYS 518) May be convened with 418.
Last taught by: George Rieke, Gary Schmidt
Class Web Site
522. Atomic and Molecular
Astrophysics
(3) I 2000-01 Interpretation of astronomical spectra: basic aspects of
atomic and molecular spectra and processes that enable one to infer
physical conditions in astronomical environments from analysis of their
electromagnetic spectra. Familiarity with basic quantum mechanics is
assumed.
Last taught by: Lucy Ziurys, Peter Strittmatter
535. Stellar Structure
(3) II 2001-02 Equations of stellar structure, virial theorem,
energy
transport, equations of state, opacities, nuclear reactions, stellar
models, evolution of low and high mass stars, observational tests,
rotation and magnetic fields, binary evolution.
Last taught by: Dave Arnett, Jim Liebert
Class
web site
540.
Structure and Dynamics of Galaxies (3) I 2000-01 Observational
properties of galaxies; structure, kinematics, star and gas content.
Structure of our own galaxy. Dynamics of stellar systems: equilibria,
instabilities, internally and externally driven evolution.
Last taught by: Dennis Zaritsky, Romeel Dave
Class Web
Site
541.
Extragalactic Astronomy and Cosmology (3) II 2000-01 The
structure,
origin and evolution of the physical universe from theory and
observations of systems outside our own galaxy. Relativistic cosmology;
galaxy evolution and clustering; active galaxies and quasars; the
microwave background; galaxy formation; the hot big bang; and physics
of the early universe. P, 540.
Last taught by: Daniel Eisenstein, Romeel Dave
Class
Web site
545. Stellar Atmospheres
(3) I 2001-02 Radiative transfer, gray atmosphere, opacity, line
formation, non-LTE, curves of growth, stellar hydrodynamics, and
planetary applications. (Identical with PTYS 545)
Last taught by: Ivan Hubeny
Class web
site
582.
High Energy Astrophysics (3) Radiation mechanisms, synchrotron
radiation, charged particle acceleration, pulsars, black holes,
accretion disks, X-ray binaries, gamma-ray sources, radio galaxies,
active galactic nuclei. (Identical with PHYS 582 and PTYS 582)
Last taught by: Fulvio Melia
Class Web
site
Course notes have been published as a book: http://press.princeton.edu/titles/8964.html
ASTR 519 -- Adaptive Optics (1 unit)
Description:
An overview of adaptive optics for astronomy and optical sciences grad
students. Will cover light propagation through atmospheric turbulence
and methods for sensing and correcting wavefront errors. Topics will
include laser beacons, multi-conjugate adaptive optics, and exoplanet
imaging.
Usually offered: Spring.
ASTR 537 -- The Physics of the Sun (3 units)
Description:
The purpose of this course is to present an introduction to the
physics of the Sun. The course begins with a discussion of
the standard solar model, the solar-neutrino problem, and
observational techniques. Long-term variability in the total
irradiance, sunspot number, and diameter, and its effect on Earth's
climate will be addressed in some detail. Other topics include the
physics of the solar interior, solar oscillations, and solar
composition. This course will also introduce the equations of
magnetohydrodynamics and apply them to important solar-physics
problems, such as: the solar magnetic dynamo, stability of prominences,
physics of sunspots and flares, and heating of the solar atmosphere.
The emphasis throughout will be on basic physical processes and the
various approximations used in their application to concrete problems.
Usually offered: Fall.
ASTR 539 -- Methods of Teaching Space Sciences (3
units)
Description:
Planning and assessment in space science teaching, identification and
correction of student misconceptions, management of classroom
discourse, and use of technology for data collection and analysis.
Graduate level requirements include two additional critical review
projects, one of which must be suitable for submission to Astronomy
Education Review as a scholarly review.
Usually offered: Fall.
ASTR 542 -- Mars (3 units)
Description:
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. The
course will include visits to Mars exploration centers at the
University of Arizona and Arizona State University, including the
operations center for the Gamma Ray Spectrometer on the Mars Odyssey
spacecraft, currently orbiting Mars, and an all-day trip to the Mars
Space Flight Facility at Arizona State University, operations center
for experiments on the Mars Global Surveyor, Mars Odyssey, and Mars
Exploration Rovers. 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.
Usually offered: Spring.
ASTR 553 -- Solar System Dynamics (3 units)
Description:
Dynamical processes affecting the orbital evolution of planets,
asteroids, and satellites, and the rotational evolution of solid
bodies. Emphasizes modern nonlinear dynamics and chaos.
Usually offered: Spring.
ASTR 555 -- Teaching College-Level Astronomy and Planetary
Science (1-3 units)
Description:
Students will discuss their current or recent experiences as a student.
They will also learn how to create productive learning environments by
reviewing research on the nature of teaching and learning; setting
course goals and objectives; using interactive lectures, peer
instruction, engaging demonstrations, collaborative groups, tutorials,
and ranking tasks; and observing other instructors. Students will
conduct a collaborative research project of their choosing related to
astronomy and space science. The course will culminate with students
presenting mock lectures using these techniques. Graduate-level
requirements are based a higher level of
Usually offered: Fall, Spring.
ASTR 556 -- Teaching College-Level Astronomy & Planetary
Science (1 unit)
Description:
Students will discuss their current or recent experiences as a student.
They will also learn how to create productive learning environments by
reviewing research on the nature of teaching and learning; setting
course goals and objectives; using interactive lectures, peer
instruction, engaging demonstrations, collaborative groups, tutorials,
and ranking tasks; and observing other instructors. Students will
conduct a collaborative research project of their choosing related to
astronomy and space science. The course will culminate with students
presenting mock lectures using these techniques. Graduate-level
requirements include an increased degree of rigor required to earn the
same grade. Since graduate students are further along their academic
path, the bar is set higher for equal achievement.
Usually offered: Fall, Spring.
ASTR 557A -- The Anthropology of Astronomy (3 units)
Temporary course: offered during Spring 2009 only.
Description:
This course is designed for students who want to add a cultural
astronomy component to their undergraduate senior thesis,
master�s
thesis research, or their dissertation. Cultural astronomy encompasses
the fields of astronomy, ethnoastronomy, and archaeoastronomy. This
semester we will explore ethnoastronomy (the astronomy beliefs and
practices of contemporary cultures); archaeoastronomy (built structures
aligned to celestial bodies); and astrology (how the positions of
celestial bodies are used to predict human events on Earth). The course
emphasizes data collection methods from cultural anthropology,
archaeology, historical/archival research, and mathematical
calculations. The case studies provide detailed information about the
relationship between individual communities and the sky, which can be
compared cross-culturally. The course is discussion based, thus you
must do the assigned readings. You are required to turn in a 15+ page
research paper and to give a 20 minute oral presentation on your
research paper. Graduate-level requirements include extra participation
in class discussion, five homework assignments, and an individual
research papers.
ASTR 558 -- Plasma Physics with Astrophysical and Solar System
Applications (3 units)
Description:
The goal of this course is to present an introduction to fundamental
plasma physics and magnetohydrodymics, beginning with kinetic theory.
The various important limits including the vlasov equation and
magnetohydrodynamics will be derived. Applications will be mostly from
astrophysics and the solar system. These will include the main
dynamical processes in the solar atmosphere, interplanetary medium,
magnetospheres, interstellar medium, blast waves, accretion disks, etc.
The emphasis throughout will be on basic physical processes and the
various approximations used in their application to concrete problems.
Usually offered: Fall.
ASTR 571 -- General Relativity and Cosmology (3 units)
Description:
General relativity with application to celestial mechanics, stellar
structure, gravitational radiation, black holes, gravitational lensing
and cosmology.
Usually offered: Fall, Spring.
ASTR 579 -- Writing for Astronomers (3 units)
Description:
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 astronomy to popular articles about astronomy. 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 astronomy.
Usually offered: Fall.
ASTR 586 -- Astronomy Education and Public Outreach (3
units)
Description:
The four overarching ideas about astronomy education and public
outreach that frame this course can be summarized as: (1) the main
conceptual ideas that students and the public need to be engaged in
regarding astronomy; (2) a working knowledge of science education
research and how people learn astronomy in different venues; (3) the
most effective strategies to partner with and disseminate materials to
K-14 formal learning entities; and (4) the nature of effective informal
free-choice learning environments (including modern museums,
planetariums, observatory visitor centers, and science centers).
Students will study and apply contemporary learning theory in a variety
of learning environments and critically evaluate existing products and
programs as preparation for planning and evaluating novel programs.
Course is characterized by discussion on assigned readings,
mini-lectures, field-trips, evaluation of existing programs, and by
creation of new programs. Graduate-level requirements include two
additional critical review projects, one of which must be suitable for
submission to Astronomy Education Review as a scholarly review.
Usually offered: Fall, Spring, Summer.
ASTR 596B -- Methods in Computational Astrophysics (3
units)
Description:
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).
Usually offered: Spring.
ASTR 596F -- College Astronomy Teaching (1 unit)
Description:
An overview of the introductory astronomy curriculum, effective
teaching approaches that focus on student learning, and appropriate
testing and grading methods for students planning on teaching at the
collegiate level. Current topics in pedagogical content knowledge are
covered in depth, with an emphasis on the undergraduate non-science
major.
Usually offered: Spring, Summer.
ASTR 597A -- Teacher Leaders in Research-Based Science Education (3
units)
Description:
This course includes a 16 week distant learning course and a two week
summer in-residence workshop at Kitt Peak National Observatory.
Participants are trained in astronomy content, pedagogy, and leadership
skills.
Usually offered: Spring.