Volcanic activity on Io — the innermost Galilean moon of Jupiter and the most volcanically active body in the Solar System — is unlikely to be sourced from a global magma ocean just below the surface, according to a new analysis of Juno and Galileo Doppler data from the Deep Space Network and astrometric observations. The internal structure of Io as revealed by the present study. Image credit: Sofia Shen / NASA / JPL / Caltech. Slightly...
