- Code ASTR6007
- Unit Value 6 units
- Offered by Research School of Astronomy and Astrophysics
- ANU College ANU Joint Colleges of Science
- Course subject Astronomy and Astrophysics
- Areas of interest Astronomy and Astrophysics
This course provides an introduction to stellar structure, evolution, and atmospheres. It covers the basic physical processes that govern the behaviour of stars, including hydrostatic equilibrium, thermal balance, nuclear energy generation, and radiation transport, the application of these principles to modeling the life cycle of stars from birth to the main sequence to death, and the development of tools to deduce stars' physical properties from the light they emit.
This course is co-taught with undergraduate students but assessed separately.
Upon successful completion, students will have the knowledge and skills to:
- Explain the concepts of hydrostatic balance, equations of state for stellar matter, transfer of heat through stars, stellar nucleosynthesis, and radiation transport, and perform calculations using these concepts;
- Calculate the internal structures of stars at a variety of levels of approximation;
- Describe the life cycles of stars from birth to death, and how these cycles depend on stellar mass;
- Explain the basic theory of stellar spectra, and use this theory to interpret the observed spectra of stars;
- Work effectively as part of a group;
- Read, interpret, and critically analyse professional research literature in the areas of stars;
- Identify unsolved problems in stars, and propose research approaches that could be used to address them.
- 6 problem sets (40) [LO 1,2,3,4,5]
- Final exam (40) [LO 1,2,3,4]
- Critical reflection on research literature, delivered in written and oral form (20) [LO 6,7]
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The expected workload will consist of approximately 130 hours throughout the semester including:
- Face-to face component which may consist of 3 hours of lectures (1x2 hour lecture plus 1x1 hour lecture) and 1 x 1 hour tutorial per week
- Approximately 96 hours of self-study which will include preparation for lectures, presentations and other assessment tasks (average 5 hours per week of problem sets and 3 hours per week of work on the literature analysis).
To be determined
Requisite and Incompatibility
Prescribed TextsUnderstanding Stellar Evolution, by H. Lamers and E. Levesque
Radiative Transfer in Stellar Atmospheres, by R. Rutten
Assumed KnowledgeBachelor of Science or equivalent with a major in astronomy, physics, or mathematics with relevant experience or academic achievement. Students should have basic familiarity with computer programming.
Tuition fees are for the academic year indicated at the top of the page.
If you are a domestic graduate coursework or international student you will be required to pay tuition fees. Tuition fees are indexed annually. Further information for domestic and international students about tuition and other fees can be found at Fees.
- Student Contribution Band:
- Unit value:
- 6 units
If you are an undergraduate student and have been offered a Commonwealth supported place, your fees are set by the Australian Government for each course. At ANU 1 EFTSL is 48 units (normally 8 x 6-unit courses). You can find your student contribution amount for each course at Fees. Where there is a unit range displayed for this course, not all unit options below may be available.
Offerings, Dates and Class Summary Links
Class summaries, if available, can be accessed by clicking on the View link for the relevant class number.
|Class number||Class start date||Last day to enrol||Census date||Class end date||Mode Of Delivery||Class Summary|
|3634||24 Feb 2020||02 Mar 2020||31 Mar 2020||29 May 2020||In Person||N/A|