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Triaxial Shapes and Densities of G!kún∣∣’hòmdímà, Haumea, and Varda from Stellar Occultations

  • Authors: Benjamin Proudfoot, Will Grundy, Flavia Luane Rommel, Estela Fernández-Valenzuela, Darin Ragozzine

Benjamin Proudfoot et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 2.

Our best-fit triaxial shape model for G!kún∣∣’hòmdímà. Colored lines show the various occultation chords detected during the 2014 stellar occultation (G. Benedetti-Rossi et al. 2016; K. Schindler et al. 2017), while the red line tips show the uncertainty in the start and end of the occultation chords. This best-fit model corresponds to a shape of a = 339 km, b = 326 km, and c = 298 km.

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