GALAXIES
Distribution of stars, gas, and dust within our Milky Way, and their motions. Nearby galaxies: our Local Group. Optical, radio, and other techniques for observing galaxies. Composition and motions of other galaxies; galaxies with active nuclei; galaxy formation.
Prerequisites & course information
Requisites: ASTRON 200 and ( PHYSICS 241 , 249 , PHYSICS/E C E 235 , or concurrent enrollment) Course Designation: Core GenEd - Natural Science & Wellness Breadth - Physical Science Level - Advanced L&S Credit - L&S Liberal Arts and Science Repeatable for Credit: No Last Taught: Spring 2026 Learning Outcomes: 1. Describe current astrophysical theories and modern observations of galaxies. Audience: Undergraduate 2. Apply physical principles and mathematical techniques to understand the natural laws governing galaxies. Audience: Undergraduate 3. Use scientific computing methods to analyze and physically interpret galaxy data. Audience: Undergraduate 4. Practice clear and concise written and oral scientific communication. Audience: Undergraduate 5. Exhibit proper professional and ethical conduct while working in group settings. Audience: Undergraduate Learning Outcomes: 1. Describe current astrophysical theories and modern observations of galaxies. Audience: Undergraduate 2. Apply physical principles and mathematical techniques to understand the natural laws governing galaxies. Audience: Undergraduate 3. Use scientific computing methods to analyze and physically interpret galaxy data. Audience: Undergraduate 4. Practice clear and concise written and oral scientific communication. Audience: Undergraduate 5. Exhibit proper professional and ethical conduct while working in group settings. Audience: Undergraduate
Sources
- Course catalogue ↗2026-2027