units
ASP2062
Faculty of Science
This unit entry is for students who completed this unit in 2012 only. For students planning to study the unit, please refer to the unit indexes in the the current edition of the Handbook. If you have any queries contact the managing faculty for your course or area of study.
Refer to the specific census and withdrawal dates for the semester(s) in which this unit is offered, or view unit timetables.
Level | Undergraduate |
Faculty | Faculty of Science |
Offered | Clayton Second semester 2012 (Day) |
Coordinator(s) | Dr Alina Donea |
Processes of star and planet formation; celestial mechanics; tides, accretion disks; solar system formation; extra-solar planets; the Sun; interiors of stars and the main sequence; post main sequence evolution; degenerate remnants; the Milky Way; the nature of galaxies; active galaxies; particles and cosmic rays.
On completion of this unit students will become familiar with the application of basic physical and mathematical principles to quantitative and qualitative understanding of the nature of the universe around us; will develop the ability to think physically about astronomical problems, and demonstrate this in a range of problem solving tasks; will develop practical skills in computationally modelling astrophysical systems and will have gained a knowledge of stars, planets, and galaxies sufficient to undertake further astrophysics studies at Level 3.
Examination (3 hours): 50%
Problem sets: 10%
Computer laboratories: 30%
Tests: 10%
A pass in the examination is required to pass the unit.
Three 1-hour lectures per week, one weekly 2-hour computer practical class, one weekly 1-hour support class
MTH1030, MTH1035 or equivalent, and 6 points of physics at level one
MTH2010 or MTH2015 recommended
ASP2022 (except with permission from the unit coordinator)