Table 8
Diameters and geometric albedos of probable dynamical interlopers of the Haumea family.
| Name | Diameter | Geometric | Ref. | Cause of |
|---|---|---|---|---|
| (km) | albedo | exclusion | ||
| 1996 TR66 | … | … | NIR colours | |
| 1999 KR16 | 232 |
0.105 |
(1) | Very red |
| 2002 AW197 |  |
 |
(3) | NIR spectra |
| 1999 RY215 |  |
 |
(3) | (J-HS) colour |
| Salacia | 901 ± 45 | 0.044 ± 0.004 | (4) | NIR spectra |
| Makemake | 1430 ± 9 | 0.77 ± 0.03 | (2) | Methane ice |
| 1998 WT31 | … | … | Red slope | |
| 2005 UQ513 |  |
 |
(3) | Red slope |
| 1996 RQ20 | … | … | Very red | |
| 1999 CD158 | <310 | >0.13 | (1) | Very red |
| 1999 OH4 | … | … | NIR colours | |
| 2000 CG105 | … | … | NIR colours | |
| 2001 FU172 | … | … | Red slope | |
| 2001 QC298 |  |
 |
(3) | (J-HS) colour |
| 2002 GH32 | <230 | >0.13 | (3) | Very red |
| 2003 TH58 | … | … | (J-HS) colour | |
| 2004 PT107 |  |
 |
(3) | (J-HS) colour |
| 2005 GE187 | … | … | (J-HS) colour | |
| 2010 KZ39 | … | … | NIR colours |
Notes. Diameter is given only if measured by thermal radiometric techniques or by occultations. The upper/lower limits of size/albedo are based on 2σ flux density limits of the most constraining wavelength band. The reason used in the literature (e.g. Snodgrass et al. 2010) to reject a target as a family member is given in the last column. References. (1) This work, (2) Ortiz et al. 2012a, (3) Vilenius et al. 2014, (4) Fornasier et al. 2013.
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