Fig. 6


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Comparison of the specific angular momentum and the normalized angular velocity of our targets with the expected values for Maclaurin and Jacobi ellipsoids as well as dumb-bell shapes. Our targets are successively grouped as a function of their oblateness (upper panel), volatile content (middle panel), and size (lower panel). Both the mean distance (md) and chi-square of each group with respect to the Maclaurin sequence are indicated in each panel. We note that (216) Kleopatra isnot included in these calculations. Large volatile-rich spherical bodies that fall very close to the Maclaurin sequence are highlighted in the bottom panel.

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