Units / EAE2051
EAE2051 · Introduction to the formation and evolution of planets
2026 Handbook6 credit pointsLevel 2School of Earth, Atmosphere and Environment
Last checked: 23 Aug 2026 UTCOverview
This unit is an introduction to the processes that led to formation of planets in our solar system, and controlled their evolution over the last 4.56 billion years. It starts with aspects of larger scale astronomy to generate a picture of our place in the universe and where planets form within galaxies. Next we focus in on the planets in our solar system, generating an understanding of how they formed in a way that explains their large-scale characteristics. The unit then moves through geologic time from the first few million years of the solar system’s history when planets first formed, through 4.56 billion years of planetary evolution to what we see today. This covers aspects of planetary geology, deep time climate change, and planetary surface geomorphology. In doing so, Earth is compared and contrasted with the other planets. The unit thus provides an understanding of links within the broader discipline of Earth sciences and should be of interest to anyone wanting to learn more about geology, climate science and environmental geography.
Offerings
| Campus | Teaching period | Mode |
|---|---|---|
| Clayton | First semester | Teaching activities are on-campus (ON-CAMPUS) |
Assessment
The Handbook does not list a final examination among the assessment items. That is not a guarantee there is none.
| # | Assessment | Type | Weight | Hurdle |
|---|---|---|---|---|
| 1 | Semester-long research project | Demonstration | 50% | — |
| 2 | In-class practical exercises | Demonstration | 30% | — |
| 3 | Critical evaluation of the literature essay | Written | 20% | — |
Assessment details may change. Please refer to the assessment information in Moodle closer to the start of the teaching period.
Requisites
The Handbook lists no prerequisite, corequisite or prohibition for this unit.
Learning outcomes
- Explain the current hypotheses for the large-scale formation and evolution of the Solar System, and how these may differ to planetary systems around other stars;
- Describe the characteristic building blocks of different types of planets and moons;
- Discuss how surface features on planets and moons indicate different geological, climate, and geomorphological processes;
- Combine scientific data to design and evaluate strategies to conduct research on planetary materials;
- Combine scientific data to form a hypothesis that can be used in exploration of planetary surfaces for evidence of life, or for resources;
- Communicate effectively with scientists and engineers in the space sector.
Workload
• One 3-hour workshop; • One 2-hour workshop and • Seven hours of independent study per week.
| Activity | Duration |
|---|---|
| Workshops | 60 hours |
Ask about EAE2051
Answered from the Handbook fields above — no AI, no guessing. Every answer links back to the source.
Community discussions about EAE2051
CommunityStudent experience, not official rules. Nothing here changes what the Handbook says.