An introduction to modern astronomy, with an emphasis on using astronomical observations to understand the evolution of stars, galaxies and the Universe. Students are introduced to the night sky and how to navigate around it using astronomical coordinates. The design, performance and use of visible and radio wavelength telescopes is discussed in detail, including imaging and spectroscopy. Visible and radio wavelength observations will be interpreted to determine the distances, masses, ages and evolution of stars and galaxies. Laboratory work is a key component of ASP2011, including an astronomical observing session and analysis of data from major observatories. -- Course Website
Instructor: Dr Heath Jones
Prerequisites: 6 points of physics at first-year level
