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(SCI)
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Leader: Professor Paul Cally (School of Mathematical Sciences)
Offered:
Clayton Second semester 2006 (Day)
Synopsis: 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.
Objectives: 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.
Assessment: Examination (3 hours): 50% + Problem sets: 10% + Computer laboratories: 30% + Tests: 10% A pass in the examination is required to pass the unit.
Contact Hours: Three 1-hour lectures per week, one weekly 2-hour computer practical class, one weekly 1-hour support class
Prerequisites: MTH1030 or equivalent and 6 points of physics at level one
Corequisites: MTH2010 recommended
Prohibitions: ASP2022 (except with permission of unit leader)