This graphic and animation show the internal structure of Jupiter’s moon Io as revealed by data from NASA’s Galileo spacecraft. The low-density crust about 30 to 50 kilometers (20 to 30 miles) thick is shown in gray in the cross-section. Image credit: NASA/JPL/University of Michigan/UCLA › Play animation
Pasadena, CA-(ENEWSPF)- New data analysis from NASA’s Galileo spacecraft reveals a subsurface ocean of molten or partially molten magma beneath the surface of Jupiter’s volcanic moon Io.
