Astronomy Undergraduate Courses • Fall 2016
This seminar discusses the physics of Black Holes, the evidence for their existence, and some of the interesting implications that black holes pose for the universe. Using Kip Thorne's book, "Black Holes and Time Warps; Einstein's Outrageous Legacy," we will delve into the ordinary predictions about black holes, including space-time curvature, time dilation, the dangers of getting too close, the central singularities, frame dragging, as well as some of the more exotic predictions like black hole evaporation and wormholes. Although the concepts in this course are not intuitive for most students, they can be understood by …
A description of modern astronomy with emphasis on the structure and evolution of stars, galaxies, and the Universe. Additional topics optionally discussed include quasars, pulsars, black holes, and extraterrestrial communication, etc. Individual instructor's synopses available from the department.
Optical and Infrared Astronomy Laboratory - Astro 120
Instructor: Gaspard Duchene
Tu 6-12A, 541 CAMPBELL
In this course, students undertake several inquiry-based lab experiments to acquire the bases of observational optical astronomy. The experiments, which build on theoretical knowledge obtained in previous classes and include the measurement of the Earth-Sun distance and the detection of an extrasolar planet, provide the students with a first introduction to the methodology of professional research. The skills that are emphasized and developed in the course include data acquisition and processing, thorough error analysis and the underlying statistics, as well as high-quality report writing, weekly show-and-tell discussions and group work. …
Physics of planetary systems, both solar and extra-solar. Star and planet formation, radioactive dating, small-body dynamics and interaction of radiation with matter, tides, planetary interiors, atmospheres, and magnetospheres. High-quality oral presentations may be required in addition to problem sets and a final exam.
Stars are the building blocks of galaxies and play a central role in the evolution of structure in the universe, in the nucleosynthesis of most elements, in the formation of compact objects (white dwarfs, neutron stars, and black holes), and as tools for measuring cosmological distances (e.g., Cepheids and Type 1a SN). This course will cover the observations and physics of stars. Primary topics will include the structure of self-gravitating objects, energy transport in stars, nuclear fusion in stars, stellar evolution, the birth of compact objects, and stellar oscillations. The course will emphasize physical understanding and …
This is the first part of an overview of astrophysics, with an emphasis on the way in which physics is applied to astronomy. We will start with an introduction to astronomy, and learn how astronomers observe the night sky and measure the radiation, velocities, and distances of stars. We will interpret the observations of stars in terms of physical properties, and discuss how the telescopes that we use to obtain these observations work. We will also cover mechanics and celestial motions, and we will learn how to derive masses and other properties of stars and (extra-solar) planets. Next we move on to stellar atmospheres and interiors, and …
Origins: from the Big Bang to the Emergence of Humans - Astro C13
Instructor: Eliot Quataert, Charles Marshall
TuThurs 2-3:30P, 390 HEARST MINING
Many of the most important scientific breakthroughs in history have dramatically reshaped humankind’s understanding of our place in the universe. Examples include the Copernican revolution, evolution by natural selection, the Big Bang theory of the origin and evolution of the universe, and the molecular and genetic basis of evolution. In addition to their intrinsic scientific importance, these ideas also have far reaching implications for other aspects of people’s lives (e.g., philosophical, religious, and political). This course will cover the modern understanding of origins, from the Big Bang through …