| Unit name | Formation and Evolution of the Terrestrial Planets |
|---|---|
| Unit code | EASCM1017 |
| Credit points | 10 |
| Level of study | M/7 |
| Teaching block(s) |
Teaching Block 1B (weeks 7 - 12) |
| Unit director | Professor. Tim Elliott |
| Open unit status | Not open |
| Pre-requisites |
None |
| Co-requisites |
None |
| School/department | School of Earth Sciences |
| Faculty | Faculty of Science |
The course will examine the processes that shape the gross composition and structure of the terrestrial planets. The course will concentrate on early planetary history from nebula accretion and initial differentiation. Information provided on planetary formation by the meteorite record will be investigated. The Earth will be used as a well-studied reference to understand both physical and chemical aspects of planetary-scale evolution but comparisons will be made to other terrestrial bodies.
On successful completion of the unit students will be able to:
Teaching will be dominantly through lectures. There will be a practical session examining extra-terrestrial materials (pending availability of externally sourced materials). Skills in using research literature will be developed through sessions in which small groups will lead discussions on current research topics.
40% open book examination in the last practical session, 60% closed book examination in the January exam period.
Both exams will be 2 hours long and will be based on questions about a specific research paper that will be given to students before the exam (5pm on the day prior to the exam).
For the open book exam students will be allowed to bring annotated versions of the paper and any supporting documents they wish (within limits of space on their desk).
No supporting material may be brought into the closed book exam.
