“…The experiments (57,60,61) suggest that on the Jovian isentrope molecular hydrogen probably begins to dissociate at 400 kbar and dissociation continues smoothly to completion at -3 Mbar, with metallization occurring right in the middle of this region at -1.4 Mbar and -4000 K. It now seems likely (60) that currents near the surface of Jupiter, at radii out to 0.95R, contribute to the surface magnetic field, whereas previously it was thought that the magnetic field was formed deeper in the interior at -0.75 R,. The EOS of astrophysically relevant materials are bein, 0 measured on other lasers as well, including LULI (62), Vulcan (62,63), Helen (60,64), Astrix (65), Gekko (66), and Shenguang-I (67). This whole area of measuring high pressure EOS on intense lasers represents fertile new territory for planetary and astrophysics research.…”