Hydrostatic Equilibrium – Pressure balance
“Hydrostatic equilibrium” governs the structure of all gaseous bodies
(planets or stars). The inside has higher temperature and density because of the weight of the overlying material.
Temperature at center is ~20000K. Note relation between temperature and pressure – pressure needed to prevent collapse (and more upper weight requires more pressure). Note odd state of metallic hydrogen (conducting – semi-free electrons). Core is uncertain (current limit about 5 earth masses – that’s odd).