Qualitatively describing the equilibrium between pressure and gravitation in stars
Using the astronomical unit (AU), light year (ly) and parsec (pc)
Describing the method to determine distance to stars through stellar parallax
Solving problems involving luminosity, apparent brightness and distance
Guidance:
For this course, objects in the universe include planets, comets, stars (single and binary), planetary systems, constellations, stellar clusters (open and globular), nebulae, galaxies, clusters of galaxies and super clusters of galaxies
Students are expected to have an awareness of the vast changes in distance scale from planetary systems through to super clusters of galaxies and the universe as a whole