Learning outcomes
After studying this course, you should be able to:
demonstrate knowledge of the electromagnetic spectrum and how it is used to infer properties of sources of radiation
demonstrate knowledge of the range of sizes, distances and motions of objects in the Universe and how they can be measured
demonstrate knowledge of the structure of, and the main processes operating in, the Sun
comprehend concepts lying well outside everyday experience, including those that involve very large and very small distances, times, temperatures and energies, and those that are non-intuitive.
OpenLearn - The Sun

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