Extended Data Table 2 Best solution of the main Mars rotation parameter estimates corresponding to an average of the GINS and MONTE sets of full arc solutions reported in Supplementary Table S1

From: Spin state and deep interior structure of Mars from InSight radio tracking

  1. Uncertainties are \(\sigma =\sqrt{(({\sigma }_{M}^{2}+{\sigma }_{G}^{2}+({p}_{M}-{p}_{G}{)}^{2})/2)}\), where \({{p}_{M}\pm \sigma }_{M}\) and \({p}_{G}\,\pm \,{\sigma }_{G}\) are MONTE and GINS solutions (central value plus or minus formal errors), respectively.
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