Comparing Jupiter interior structure models to <i>Juno</i> gravity measurements and the role of a dilute core

Abstract

The Juno spacecraft has measured Jupiter's low‐order, even gravitational moments, J 2 – J 8 , to an unprecedented precision, providing important constraints on the density profile and core mass of the planet. Here we report on a selection of interior models based on ab initio computer simulations of hydrogen‐helium mixtures. We demonstrate that a dilute core, expanded to a significant fraction of the planet's radius, is helpful in reconciling the calculated J n with Juno 's observations. Although model predictions are strongly affected by the chosen equation of state, the prediction of an enrichment of Z in the deep, metallic envelope over that in the shallow, molecular envelope holds. We estimate Jupiter's core to contain a 7–25 Earth mass of heavy elements. We discuss the current difficulties in reconciling measured J n with the equations of state and with theory for formation and evolution of the planet.