Heat and composition transport in gas giant planets and exoplanets

The growing collection of directly-imaged young gas giant planets
together with the new results from the Juno spacecraft on Jupiter's
interior provide new ways to constrain the physics of gas giant
formation and evolution. In this talk, I will focus on two outstanding
questions: how accretion sets the luminosity of newly-formed gas giants,
and how the composition profile interacts with convection during the
planet's evolution. Resolving these open questions is crucial if we are
to connect planet formation models to Jupiter today.