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Course Criteria
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3.00 Credits
This Foundations course provides an introduction to the breadth of Astronomy through the use of astronomical examples to reinforce physical concepts such as distance scales, magnitudes, mass, velocity, temperature, pressure and angular momentum. Topics include the celestial sphere, coordinate systems, Kepler's Laws, orbits, eclipses, tides, emission and absorption spectra, astronomical detection of light, telescopes, the Sun, properties of stars, our Galaxy, and galaxies. Prerequisites: "C-" or better in (((MATH 1220 OR MATH 1250 OR MATH 1320 OR MATH 1321 OR MATH 2210) OR AP Calculus BC score of 4+) AND ((PHYS 2210 OR PHYS 3210) OR AP Physics C Mech score of 4+)).
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3.00 Credits
This course will look at the challenges and opportunities for mitigating problems associated with light pollution and our exposure to artificial light. From better lighting design to the need for developing new environmental policies that regulate the over-use of artificial light, this course will explore ways that a new generation of practitioners in multiple fields can address the global challenge of light pollution. Students will learn about the emerging research on artificial light exposure and its impact on human health, animal health, public safety, and our loss of access to the night skies in the majority of the developed world. The course will include some field work, including learning how to use new drone technology to measure lighting impacts in communities inside and outside of Salt Lake City.
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3.00 Credits
This course focuses on how our personal relationship with the night creates emergent systems of connections throughout the globe and between species. Students will examine specific case studies of these connections in-depth and in so doing will gain interdisciplinary knowledge and skills in astronomy, biology, anthropology, engineering, and policy-making. The course will include some fieldwork, including learning how to use new drone technology to measure lighting impacts in communities inside and outside of Salt Lake City.
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3.00 Credits
This course will serve as an introduction to the tools and techniques used in optical and radio astronomy. Using the facilities at the University of Utah Observatory, we will explore the cosmos and study the Sun, planets, asteroids, stars and galaxies. Measurements of basic properties of astronomical objects will be performed. Quantitative analysis of these measurements will enable us to determine such things as the mass of Jupiter as well as the ages of stars. Recommended Prerequisites: Familiarity with computers. "C-" or better in (MATH 1210 OR MATH 1250 OR MATH 1311 OR MATH 1310 OR AP Calculus AB score of 4+ OR AP Calculus BC score of 3+) AND (PHYS 2010/2210/3210) AND (ASTR/PHYS 1060 OR PHYS 2020/2220/3220) OR instructor consent.
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3.00 Credits
This course will introduce undergraduate students to the study of galaxies, one of the most active fields of research in astrophysics. The course is intended for students following the astrophysics emphasis or getting an astronomy minor. The course will focus on understanding both the contents of galaxies and the tools we sue to understand their formation and evolution. It will cover galaxies near and far, from the Milky Way to the most distant galaxies visible to us. Topics will include galaxy structure, galaxy dynamics, stellar populations, the measurement of distances, gas and star formation in galaxies, the mass spectrum of galaxies, and evidence of dark matter. Prerequisites: 'C-' or better in (PHYS 3070 OR ASTR 3070) AND (MATH 1260 OR MATH 1321 OR MATH 2210 OR MATH 3140).
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3.00 Credits
An introductory course which explores modern cosmological concepts. Discusses formation of galaxies, and clusters of galaxies, the expansion and the age of the Universe. Topics include the existence and properties of the cosmic microwave background, the origin of the light elements, cosmological inflation, and the role of dark matter and dark energy in the formation and expansion of the Universe. The course will introduce concepts of statistical mechanics, quantum mechanics, special and general relativity as needed to explore the course topics. Prerequisites: 'C-' or better in (PHYS 3070 OR ASTR 3070) AND (PHYS 2710 OR PHYS 3740) AND MATH 2250
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3.00 Credits
This course introduces students to one of the most active areas of research in astrophysics. It is intended for students who have taken a first course in astronomy and are interested in learning more. It also satisfies requirements of the astrophysics emphasis and astronomy minor. We focus on understanding how stars function by using physical concepts and observational results. Topics include star formation; nucleosynthesis & stellar evolution (including discussion of supernovae, white dwarfs, neutron stars, and stellar black holes); radiative transfer and energy transport; stellar atmospheres and interiors. The course will introduce concepts of statistical and quantum mechanics, and aspects of relativity, as needed to help explore the course topics. Prerequisites: 'C-' or better in (PHYS 3070 OR ASTR 3070).
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3.00 Credits
This course provides an introduction to professional observational astronomy skills: instrumentation in optical astronomy, analysis of data and image processing, and observational techniques. Using real data, the student will develop the ability to plan observations and produce a final scientific result. The course will emphasize the capabilities and limitations of optical observations, and provide insight into current research. Prerequisites: 'C-' or better in (PHYS 2710 AND (PHYS 4060 OR PHYS 4070 OR PHYS 4080 OR PHYS 4090 OR ASTR 4060 OR ASTR 4070 OR ASTR 4080 OR ASTR 4090)) OR Graduate status in Physics/Astronomy
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3.00 Credits
As a core astrophysics course, it will be taken by graduate students of Physics & Astronomy. Students will survey the properties of stars and star clusters (as laboratories for understanding stellar evolution). Topics include: properties of stars, including fundamental parameters, positions, distances, magnitudes & luminosities, radii, masses; nuclesythesis (i.e. energy generation); stellar evolution; stellar atmospheres spectra & spectral line analysis; interstellar reddening; colour-magnitude diagrams; properties of globular and open clusters; simple stellar populations, isochrones, age estimates, distance determinations, luminosity functions, mass functions; chemical compositions & determinations; formation and evolution of globular and open clusters; stellar populations in the context of the Milky Way. Prerequisites: 'C-' or better in ((PHYS 4070 OR PHYS 4080 OR PHYS 4090 OR ASTR 4070 OR ASTR 4080 OR ASTR 4090) AND (PHYS 2710 OR PHYS 3740)) OR Graduate status in Physics/Astronomy.
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3.00 Credits
A core course intended for graduate students of Physics & Astronomy. This course explores the properties of present day galaxies and the evolution of galaxies over cosmic history based on recent results from multi-wavelength observations and simulations. Topics include Milky Way structure & populations; galaxy classification, morphology and dynamics; distance measurements; the interstellar medium; star formation and star formation rate indicators; chemical evolution; dynamical evidence for dark matter; dark matter halos; black holes and active galactic nuclei; galaxy interactions and mergers; the intergalactic medium; galaxy clusters and groups; and galaxy evolution from high-redshift observations and simulations. Prerequisites: 'C-' or better in ((PHYS 4070 OR PHYS 4080 OR PHYS 4090 OR ASTR 4070 OR ASTR 4080 OR ASTR 4090) AND (PHYS 2710 OR PHYS 3740)) OR Graduate status in Physics/Astronomy.
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