Fig. 1.
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Schematic view of Jupiter’s dilute core model used in this study and the computational process: given a combination of the seven marked interior parameters (left), the CMS method (right) converges to solve the gravity moments and mass, which is then compared to the Juno measurements to determine the feasibility. The image in Jupiter’s schematic (left) is available at https://www.planetary.org/space-images/merged-cassini-and-juno.
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