Module description
Learning aims & outcomes
Students will gain a thorough grounding in the life cycle of stars.
Students should be able to:
- Describe the stages of nucleosynthesis in stars.
- Calculate the equations of hydrostatic equilibrium.
- Use the equations of energy transport to calculate basic properties of stars.
- Describe in detail the evolutionary stages different classes of stars are thought to go through.
- Describe in detail the end stages of the life cycle of a star and the different types of stellar remnants.
Syllabus
An indicative list of topics covered by this module, but which may change slightly from year to year, is given by:
Hydrostatic equilibrium and stellar evolution, the Piston Model, nucleosynthesis, ideal gas spheres, the formation of stars (free fall collapse), stellar timescales, simple energy transport equations, stellar stability, evolution of low mass / high mass stars, final states of stars.
Assessment details
Details of the module's assessment/s
Please note: - module assessment may be subject to change. If you have any questions, please contact ug-physics@kcl.ac.uk
Students studying at King's for Semester 1 only (September-December) will be set alternative assessment in lieu of in-person exams in January / May as necessary. Further information will be provided by the Department.
Teaching pattern
Two lectures per week (Approx total 4 hours per week)