Relativistic contributions to the rotation of Mars

Open Access

Fig. 2

Difference between the [ϕ]_GR(t) obtained by numerically integrating Eq. (17), using the DE440 planetary ephemerides and using Eq. (25) and the fitted series from Eq. (37). This curve provides an estimate of the accuracy of the fitted analytical model provided by the coefficients from Table 2.

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