Introduction to the astronomical universe: sky and celestial objects, planetary motion, planets and the Solar System, Sun and stars, the Milky Way and galaxies, cosmology and the universe.
Introduction to the astronomical universe: sky and celestial objects, planetary motion, planets and the Solar System, Sun and stars, the Milky Way and galaxies, cosmology and the universe.
Observations of constellations and the night sky, the sun and moon, planets, stars, and deep-sky objects; laboratory and observational experiments illustrating basic concepts in astronomy. Offered in the evening. Pre: 110 (or concurrent), or consent.
Formation of the sun and stars; origin of our solar system; formation and evolution of galaxies, including the Milky Way Galaxy; origin of chemical elements, and the beginnings of the cosmos. A-F only.
Formation of the sun and stars; origin of our solar system; formation and evolution of galaxies, including the Milky Way Galaxy; origin of chemical elements, and the beginnings of the cosmos. A-F only.
Astronomy and celestial lore in ancient cultures: Neolithic Europe, Mayan, Mesoamerican, Egyptian, Mesopotamian, American Indian, Chinese, and Polynesian. Concepts of the cosmos, calendars, eclipse predictions, motion of celestial bodies, and navigation.
Construction of simple observing tools.
Covers the major discoveries in astronomy and astrophysics from the Babylonians through the 20th century, and the evolution of modern astrophysics. A-F only. (Fall only)
An illustrated voyage through the Solar System based on recent scientific results. The class highlights the origin, evolution, and current knowledge of the eight planets, their moons, asteroids, comets, and one star, the Sun. Field trip. (Cross-listed as ERTH 105)
A rigorous overview of modern astronomy: solar system, stellar, galactic and extragalactic astronomy and cosmology. For science and engineering students. Pre: 110; PHYS 151 or PHYS 170.
Solar system astrophysics. Dynamics of planets, satellite systems, asteroids and comets;
planetary atmospheres and internal structure; thermal balance; the Sun as a star. Introduces numerical computing. A-F only. Pre: PHYS 170, MATH 242 or 252A, and PHYS 272 (or concurrent). (Fall only)
Stellar and galactic astrophysics. Stellar magnitudes, colors, distances, and spectra. Galactic structure and evolution, active nuclei, large-scale structure, Big-Bang cosmology. Stellar interiors, nuclear “burning,” main-sequence and evolved stars. Introduces computer programming. A-F only. Pre: 241, PHYS 274 (or concurrent), and MATH 243 (or concurrent) or 253A (or concurrent). (Spring only)
The Big Bang, origin of the elements, formation and evolution of galaxies and stars. Pre: 110 or 210 or 241 or 242, or consent
Are we alone in the universe? Modern astronomical, biological, and geological perspectives on this fundamental question. Searches for life on Mars, oceans on Europa, planets orbiting other stars. Space exploration and colonies, interstellar spaceflight and communication. Pre: 110 or 210, or consent. (Spring only)
Principles and techniques of optical and near-infrared astronomical observation. Astronomical coordinate systems. Telescopes, cameras, spectrographs, and detectors. Astrometry, photometry, and spectroscopy of astronomical objects. A-F only. Pre: 210 or 242; PHYS 152 or 274; MATH 216, 242, or 252A. (Fall only)
Optical and near-infrared astronomy laboratory. Error analysis, properties of light, data, and image processing. Astrometric, photometric, and spectroscopic measurement. A-F only. Pre: 300 (or concurrent); PHYS 152 or 274; PHYS 152L or 274L; MATH 216, 242, or 252A. (Fall only)
Practical astronomical observing. Students select objects to study, plan, and conduct remote observations using research-grade telescopes, reduce data, present results in written and verbal form. Introduces LaTeX, literature research, time allocation. A-F only. Pre: 300 and 300L. (Spring only)
Introduction to astronomical spectroscopy. Stellar atmospheres, line formation, elements of radiative transfer. Phases of interstellar medium. Emission line diagnostics. Doppler shift and kinematics. A-F only. Pre: 210 or 242; PHYS 152 or 274; MATH 216 or 242 or 252A. (Spring only)
History and intellectual context of astronomical discovery; the evolution of ideas of space, time, and motion from the Babylonians to relativistic cosmologies; emphasis on the interaction of astronomy with the history of ideas. Pre: 110 (or concurrent). (Spring only)
Individual reading, observation, or experimentation in astronomy and astrophysics. Repeatable four times. Pre: consent.
Advanced survey of stellar astrophysics, including application of astrometry, photometry, and spectrometry to determine fundamental stellar properties; stellar structure and evolution of single and binary stars; astrophysical distance determination methods; stellar nucleosynthesis. Pre: 242 and 300, and PHYS 480.
Survey of extragalactic astronomy and cosmology, including: galaxy morphology and kinematics; luminosity functions; dark matter; properties of galaxy groups/ clusters; gravitational lensing; redshifts; cosmological models; the Big Bang; thermal history of the Universe; structure formation. A-F only. Pre: 300 (or concurrent); PHYS 152 or PHYS 274; MATH 216 or MATH 242 or MATH 252A. (Alt. years)
Observations and physical nature of planets and moons, asteroids, comets, and other small bodies; formation of the Solar System; discovery of other planetary systems; solar activity. Pre: 300; and PHYS 152 or 274; and MATH 216, 242, or 252A. (Alt. years)
Seminar focusing on development of professional skills for astronomical research, and on scientific writing as a tool for organizing research. A final paper describing a supervised research project is required. Repeatable one time. A-F only. Pre: 301; 399 (or concurrent) or PHYS 399 (or concurrent).
Astrophysics of diffuse matter, HII regions, molecular clouds, etc. Pre: consent. (Alt. years)
Structure and evolution; energy sources, radiative processes; relations to observables. Pre: consent. (Alt. years)
Observations and stellar dynamics of elliptical and spiral galaxies including our galaxy, globular clusters, and dark matter. Galaxy formation and evolution. Pre: consent. (Alt. years: spring)
Geometry and evolution of the universe. Dark matter. Early universe. Formation of large–scale structure, galaxies, and clusters. Cosmological models. Pre: consent. (Alt. years)
Survey of observational data and physical concepts on planets and smaller bodies; formation of planetary systems; solar activity. Pre: consent. (Alt. years)
Excitation, ionization, and radiative transfer in stellar atmospheres; model atmospheres, formation of line and continuum radiation. Pre: consent. (Alt. years)
Telescopes, positional astronomy, photon detection, error analysis, photometry, spectroscopy. Pre: consent. (Fall only)
Design and operation of astronomical instrumentation. Physics of optical and infrared detectors. Wavefront sensors and adaptive optics. Radio and infrared interferometry. Optical design: methods and software. A-F only. Pre: 633 (with a minimum grade of B-). (Alt. years: spring)
Applications of fundamental physics to astrophysical situations. Elements of general relativity. Basics of hydrodynamics and shock waves. Radiative processes, high energy astrophysics. Modern dynamics. Pre: consent. (Fall only)
Introduction to gravity and general relativity. Tensor basics, classical scalar, vector and tensor field theories. Exact symmetric Einstein equation, gravito-magnetic weak field, and radiation solutions. Pre: consent. (Alt. years)
Phenomenology of active galactic nuclei, black holes, accretion flows and jets, emission mechanisms, host galaxies, and cosmic evolution. Pre: 635 or consent. (Alt. years: spring)
Formation of astrobiologically important molecules and their precursors in the interstellar medium and in our solar system: first principles and latest trends. Pre: consent. (Fall only) (Cross-listed as CHEM 657 and ERTH 657)
Repeatable unlimited times. Pre: consent
Repeatable unlimited times.
Selected advanced topics in astronomy and astrophysics. Available for 1 to 3 credit hours by arrangement. Repeatable unlimited times. Pre: consent.
Selected advanced topics in astronomy and astrophysics. Available for 1 to 3 credit hours by arrangement. Repeatable unlimited times. Pre: consent.
Selected advanced topics in astronomy and astrophysics. Available for 1 to 3 credit hours by arrangement. Repeatable unlimited times. Pre: consent.
Interdisciplinary research topics in astrobiology as they relate to the theme of water: formation in space, role in creating pre-biotic molecules, delivery to earth, and terrestrial planet habitability. Repeatable three times. Pre: graduate level sciences and ideas, or consent.
Principles of scientific grant writing are taught by working on draft proposals through a mix of lectures, discussions, and hands on activities. The final proposal will be reviewed and evaluated via a review panel. Graduate students only. A-F only. (Fall only)
Molecular clouds, collapse processes, physics of circumstellar disks and accretion, properties of young stars, outflows and jets, formation of binaries, extrasolar planets and planet formation, meteorites and the early solar system. Pre: graduate standing or consent. (Alt. years: spring)
Seminar discussions of the most recent research papers covering all areas of astronomy. Student lead discussion sessions and discuss papers of their choice during the semester. ASTR majors only. Graduate students only. CR/NC only. (Fall only)
Repeatable unlimited times