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. 2017 Oct 11;550(7675):219-223.
doi: 10.1038/nature24051.

The size, shape, density and ring of the dwarf planet Haumea from a stellar occultation

J L Ortiz  1 P Santos-Sanz  1 B Sicardy  2 G Benedetti-Rossi  3 D Bérard  2 N Morales  1 R Duffard  1 F Braga-Ribas  3   4 U Hopp  5   6 C Ries  5 V Nascimbeni  7   8 F Marzari  9 V Granata  7   8 A Pál  10 C Kiss  10 T Pribulla  11 R Komžík  11 K Hornoch  12 P Pravec  12 P Bacci  13 M Maestripieri  13 L Nerli  13 L Mazzei  13 M Bachini  14   15 F Martinelli  15 G Succi  14   15 F Ciabattari  16 H Mikuz  17 A Carbognani  18 B Gaehrken  19 S Mottola  20 S Hellmich  20 F L Rommel  4 E Fernández-Valenzuela  1 A Campo Bagatin  21   22 S Cikota  23   24 A Cikota  25 J Lecacheux  2 R Vieira-Martins  3   26   27   28 J I B Camargo  3   27 M Assafin  28 F Colas  26 R Behrend  29 J Desmars  2 E Meza  2 A Alvarez-Candal  3 W Beisker  30 A R Gomes-Junior  28 B E Morgado  3 F Roques  2 F Vachier  26 J Berthier  26 T G Mueller  6 J M Madiedo  31 O Unsalan  32 E Sonbas  33 N Karaman  33 O Erece  34 D T Koseoglu  34 T Ozisik  34 S Kalkan  35 Y Guney  36 M S Niaei  37 O Satir  37 C Yesilyaprak  37   38 C Puskullu  39 A Kabas  39 O Demircan  39 J Alikakos  40 V Charmandaris  40   41 G Leto  42 J Ohlert  43   44 J M Christille  18 R Szakáts  10 A Takácsné Farkas  10 E Varga-Verebélyi  10 G Marton  10 A Marciniak  45 P Bartczak  45 T Santana-Ros  45 M Butkiewicz-Bąk  45 G Dudziński  45 V Alí-Lagoa  6 K Gazeas  46 L Tzouganatos  46 N Paschalis  47 V Tsamis  48 A Sánchez-Lavega  49 S Pérez-Hoyos  49 R Hueso  49 J C Guirado  50   51 V Peris  50 R Iglesias-Marzoa  52   53
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The size, shape, density and ring of the dwarf planet Haumea from a stellar occultation

J L Ortiz et al. Nature. .

Abstract

Haumea-one of the four known trans-Neptunian dwarf planets-is a very elongated and rapidly rotating body. In contrast to other dwarf planets, its size, shape, albedo and density are not well constrained. The Centaur Chariklo was the first body other than a giant planet known to have a ring system, and the Centaur Chiron was later found to possess something similar to Chariklo's rings. Here we report observations from multiple Earth-based observatories of Haumea passing in front of a distant star (a multi-chord stellar occultation). Secondary events observed around the main body of Haumea are consistent with the presence of a ring with an opacity of 0.5, width of 70 kilometres and radius of about 2,287 kilometres. The ring is coplanar with both Haumea's equator and the orbit of its satellite Hi'iaka. The radius of the ring places it close to the 3:1 mean-motion resonance with Haumea's spin period-that is, Haumea rotates three times on its axis in the time that a ring particle completes one revolution. The occultation by the main body provides an instantaneous elliptical projected shape with axes of about 1,704 kilometres and 1,138 kilometres. Combined with rotational light curves, the occultation constrains the three-dimensional orientation of Haumea and its triaxial shape, which is inconsistent with a homogeneous body in hydrostatic equilibrium. Haumea's largest axis is at least 2,322 kilometres, larger than previously thought, implying an upper limit for its density of 1,885 kilograms per cubic metre and a geometric albedo of 0.51, both smaller than previous estimates. In addition, this estimate of the density of Haumea is closer to that of Pluto than are previous estimates, in line with expectations. No global nitrogen- or methane-dominated atmosphere was detected.

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