Ganymede has strong evidence of a subsurface ocean primarily composed of MgSO 4. We conducted experimental measurements of the electrical conductivity of aqueous MgSO 4 at 200-1,200 MPa and 243-295 K in a multianvil press, simulating the high-pressure and low-temperature (HPLT) conditions of Ganymede's subsurface ocean. A numerical model is proposed with logσ = − 3.1605 +940.931/T+0.8986logc+2logΛ 0 − log(5Λ 0 +2695c 1/2), where σ is electrical conductivity in S/m, T is temperature in K, c is molar concentration in mol/L, and Λ 0 is limiting equivalent conductance in S•cm 2 •equiv −1. We used this model to generate electrical conductivity curves up to 500 km deep in Ganymede and found that the values are lower than previously predicted. Our novel experimental methods demonstrate access to the HPLT environment of liquid samples that expands our ability for experimental simulation of icy ocean worlds in the outer solar system. Plain Language Summary The idea that a liquid ocean exists within Ganymede is widely accepted through various indirect observations. One of the evidences, based on Galileo's magnetometer data, postulates that Ganymede's inductive magnetic field is most likely derived from a conductive liquid ocean. It is highly probable that the composition of this subsurface ocean is MgSO 4. Therefore, direct measurement of the electrical conductivity of the MgSO 4 solution in this environment can help to establish a more accurate internal structure model. However, this ocean is located at high-pressure and low-temperature (HPLT) conditions that are difficult to achieve with high-pressure devices, so there is a lack of experimental data. In this study, we achieved a HPLT environment with a modified multianvil press and performed electrical conductivity measurements on 10 wt% MgSO 4 solution. A comparative analysis of our data and previous theoretical values shows our measurements are somewhat lower and may provide experimental reference for analysis of future data obtained by the JUICE mission at Ganymede.