units
ASP2062
Faculty of Science
This unit entry is for students who completed this unit in 2014 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 |
Organisational Unit | School of Mathematical Sciences |
Offered | Clayton Second semester 2014 (Day) |
Coordinator(s) | Dr Duncan Galloway |
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 be able to:
Examination (3 hours): 60%
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
ASP2022 (except with permission from the unit coordinator)