Top panel: Jupiter density and temperature for different equations of state: SCvH (green solid), REOS3b (blue dashed), and MH13+SCvH (red dotted line). The discontinuity is due to the separation of the outer and deeper envelope at P_sep = 1 Mbar. Bottom panel: differences in the temperature obtained with the three different equations of state. The blue line is the temperature difference between REOS3b and SCvH, the red dotted line is the difference between SCvH and MH13+SCvH, and the orange dashed line is the difference between REOS3b and MH13+SCvH.