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At the mid-mission perijove 17, Juno registered a Love number $k_2=0.565\\pm0.006$ that is $-4\\pm1\\%$ ($1\\sigma$) from the theoretical hydrostatic $k_2^{(hs)}=0.590$. Here we assess whether the aforementioned departure of tides from hydrostatic equilibrium represents the neglected gravitational contribution of dynamical tides. 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