Equation 10 · How We Know What Is Inside a Planet
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Symbol J_2
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For the giant planets, only low-degree harmonics are available, and the interpretation problem sharpens. Juno measured Jupiter’s even zonal harmonics through to high precision, and Wahl and colleagues found that models fit those moments best when the heavy-element core is not compact but dilute, expanded over a significant fraction of the planet’s radius, with total heavy-element content in the core region of roughly 7 to 25 Earth masses [ 17 ] . That range is wide for a reason the authors state plainly: the inferred structure is strongly affected by the chosen hydrogen-helium equation of state [ 17 ] . The gravity data are excellent; the translation into structure is only as…
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For the giant planets, only low-degree harmonics are available, and the interpretation problem sharpens. Juno measured Jupiter’s even zonal harmonics through to high precision, and Wahl and colleagues found that models fit those moments best when the heavy-element core is not compact but dilute, expanded over a significant fraction of the planet’s radius, with total heavy-element content in the core region of roughly 7 to 25 Earth masses [ 17 ] . That range is wide for a reason the authors state plainly: the inferred structure is strongly affected by the chosen hydrogen-helium equation of state [ 17 ] . The gravity data are excellent; the translation into structure is only as good as the laboratory and computational physics behind it.
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