Extended Data Table 1 Gravity spherical harmonic coefficients of Ceres7

From: A partially differentiated interior for (1) Ceres deduced from its gravity field and shape

  1. The observed un-normalized coefficients Cnm and Snm up to degree and order 8 (named CERES08A) are computed from Dawn’s tracking data. The parameters σ C n m and σ S n m represent the uncertainties of Cnm and Snm, which are computed by multiplying the formal standard deviations by a factor of six to account for potential systematic errors. The last two columns show the un-normalized spherical harmonic coefficients derived from topography assuming a homogeneous Ceres with mean density, denoted with an asterisk.
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