units
ASP3231
Faculty of Science
Refer to the specific census and withdrawal dates for the semester(s) in which this unit is offered.
| Level | Undergraduate |
| Faculty | Faculty of Science |
| Offered | Clayton First semester 2012 (Day) |
| Coordinator(s) | Dr Michael Brown |
This unit gives students theoretical background and practical experience in modern observational astronomy. ASP3231 students study telescope optics, spectroscopy, CCD imaging, image processing, statistics, astronomical distances, stellar evolution, extra-solar planets, neutron stars and galaxies. An observational project, including an astronomical observing session and analysis of the observations, comprises a substantial component of ASP3231.
On completion of this unit students will be able to operate an astronomical telescope; obtain CCD images of celestial objects; process and calibrate images using the techniques of research astronomy; utilise photometry to understand the nature of celestial objects; utilise spectra to measure the distances, masses and temperatures of celestial objects; utilise statistics to constrain measurements and test hypotheses; understand the operation of CCDs; understand telescope design, including telescopes operating beyond the visible wavelength range; describe and characterise the performance of astronomical spectrographs; describe the impact of the atmosphere on astronomical observations; understand how adaptive optics improves the angular resolution of astronomical images; complete a substantial observational project and written report as a member of a team.
Examination (3 hours): 40%
Laboratory: 15%
Project: 35%
Assignments: 10%
Students must achieve a pass mark in the laboratory/project component to achieve an overall pass grade.
Two 1-hour lectures per week, 4 hours laboratory or project sessions per week on average (including night-time observing)