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Table 6

Diameters and albedos of confirmed Haumea family members.

Name Δvmin H2 O Thermal Diameter Geometric Size/albedo
(m s−1) reference data (km) albedo reference
136108 Haumea (2003 EL61) 323.5 Brown et al. (2007) (S+H) 2322 × 1704 0.51 ± 0.02 O17
× 1026
Hi’iaka Barkume et al. (2006) 383a default TW
Namaka Fraser & Brown (2009) 193a default TW
19308 (1996 TO66) 24.2 Brown et al. (1999) (S+H) 210a default TW
24835 (1995 SM55) 149.7 Brown et al. (2007) (S+H) 243a default TW
55636 (2002 TX300) 107.5 Licandro et al. (2006) S+H TW, E10b
86047 (1999 OY3) 292.8 Ragozzine & Brown (2007) 91a default TW
120178 (2003 OP32) 123.3 Brown et al. (2007) S+H 274 0.54 TW
145453 (2005 RR43) 111.2 Brown et al. (2007) H 300 0.44 TW
308193 (2005 CB79) 96.7 Schaller & Brown (2008) 224a default TW
386723 (2009 YE7) 85c Trujillo et al. (2011) 226a default TW
2003 SQ317 148.0 Snodgrass et al. (2010) 98a default TW
2003 UZ117 66.8 Schaller & Brown (2008) H 222 0.29 TW

Notes. (a) Inferred using geometric albedo of pV = 0.48. Δvmin (from Ragozzine & Brown 2007 unless otherwise indicated) is the minimum of four possible solutions of velocity relative to the collision location’s orbit in a calculation where the information about the original orbital angles Ω, ω, and M has been lost. References to first detection of water ice confirming family membership, sources of thermal data: S for Spitzer Space Telescope and H for Herschel Space Observatory (the parentheses indicate that thermal data were not used in the size/albedo solution shown in this table). O17 = Ortiz et al. (2017), TW = This work, E10 = (Elliot et al. 2010). (b) The result of 2002 TX300 is from an occultation event re-analysed in this work (see Sect. 3.3). (c) This work.

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