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# Learning outcomes

After studying this course, you should be able to:

- use mathematical models to calculate properties of protoplanetary discs
- understand the core-accretion scenario for the growth of planetary cores from smaller components
- understand the disc-instability scenario for the formation of planets from a circumstellar disc
- describe how planets migrate and interact after forming
- appreciate how planet formation models can explain the observed exoplanet population.

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OpenLearn - The formation of exoplanets
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