Mass of the core and heavy elements in the interior of Jupiter derived with different Js. Models use Z-discontinuous scenario, P_sep = 2 Mbar and different EOS indicated in the figure. Colored areas show solutions within 2σ from the radius, J₂ and J₄ of Jupiter estimated by Campbell & Synnott (1985; black), Guillot (1999; orange), Jacobson (2003; yellow), and Jacobson (2013; red). No solution was found with MH13+SCvH and constraints by JUP230.