ASP2062 · Introduction to astrophysics

Overview

An introduction to contemporary astrophysics, with a focus on the range of physical processes which shape the universe and the objects within. You will study the generation, propagation and absorption of radiation; star and planet formation; celestial mechanics; accretion disks; interiors of stars and nucleosynthesis; post main sequence evolution; compact objects and black holes; the Milky Way; galaxies and cosmology. Laboratory work will include analytic and computer-based exercises, involving research-grade data and numerical codes.

Areas of study: Astrophysics Physics

Offerings

Assessment

The Handbook lists an examination for this unit.

Assessment details may change. Please refer to the assessment information in Moodle closer to the start of the teaching period.

Requisites

The Handbook lists no prerequisite, corequisite or prohibition for this unit.

Learning outcomes

1. Apply basic physical and mathematical principles, including dimensional analysis, to gain a quantitative and qualitative understanding of astrophysical processes.
2. Explain how observational data may be exploited to infer the physical properties of cosmic objects.
3. Solve astrophysical problems, and complete a range of problem solving tasks by drawing on physical principles.
4. Use practical skills to computationally model astrophysical systems.
5. Demonstrate a knowledge of stars, planets, and galaxies sufficient to undertake further astrophysics studies at Level 3.

Workload

The workload to achieve the learning outcomes for this unit is 144 hours spread across the semester (roughly 12 hours per week) - which requires an even mixture of attendance at scheduled activities and self-scheduled study time. Learning activities comprise a mixture of instructor directed, peer directed and self-directed learning, which includes face-to-face and online engagement.

Student experience, not official rules. Nothing here changes what the Handbook says.