Continue reading "HYDROSTATIC EQUILIBRIUM and PLANETARY DIFFERENTIATION"
HYDROSTATIC EQUILIBRIUM and PLANETARY DIFFERENTIATION
By: Mike Luciuk, Jeremy Carlo INTRODUCTION During formation of the solar system 4.6 billion years ago, a cold molecular gas and dust cloud began to contract around its denser portions. As the cloud contracted, its rotation rate increased and it evolved to a disk‐like configuration. Over time, the proto‐Sun and proto‐ planets formed. Figure 1 …