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Table 7:

Comparison of orbital and physical properties of some intermediate-large size water-bearing objects of interest.

Parameter
Orcus Charon (208996) 2003 AZ84 Quaoar Haumea
Dynamical Classa 3:2 3:2 3:2 Classical Classical
Orbit inclination ($^{\circ}$)b 20.6 17.1 13.6 8.0 28.2
Semi-major axis (AU)c 39.2 39.6 39.4 43.5 43.0
q (AU)d 30.2 29.7 32.3 41.7 34.5
Q (AU)e 48.1 49.6 46.5 45.2 51.5
r (AU)f 47 31 45 43 51
Diameter (km) $946\pm70^{(1)}$ $1207\pm3^{(2)}$ $686\pm95^{(1)}$ $850\pm200^{(1)}$ $1150\pm200^{(1)}$
  $940\pm70^{(3)}$     $910\pm100^{(6)}$ $\sim $ $2000\times1500\times1000^{(5)}$
        $1260\pm190^{(4)}$  
pV (%)g $19.7\pm3^{(1)}$ $\sim $40(7) $12.3\pm4^{(1)}$ $19.9\pm10^{(1)}$ $80\pm15^{(1)}$
  $28\pm4^{(3)}$     $17.2\pm5^{(6)}$ 60-80(8)
        $9.2\pm4^{(4)}$  
Vis. slope (%/100 nm)h $\sim $2 - $\sim $3 $\sim $28 $\sim $0
Dominant ice at surface H2O (cryst) H2O (cryst) H2O (cryst) H2O (cryst) H2O (cryst)
Volatiles and other NH4++C2H6 NH4++CH4+NH3:H2O(9) CH3OH ?(10) CH4+C2H6(11) -
  NH3:H2O+CH4 NH3:H2O, NH3(13)   CH4+C2H6+N2(12)  
  NH3+CH4 NH4OH(13)      

Notes.  (a) Using classification by Gladman et al. (2008). (b) With respect to ecliptic plane, from the Minor Planet Center. (c) From the Minor Planet Center. (d) Perihelion from the Minor Planet Center. (e) Aphelion from the Minor Planet Center. (f) Approximate current heliocentric distance. (g) Visible geometric albedo. (h) Slope of the visible spectrum from Fornasier et al. (2009) and references therein, except for Orcus: this paper.

References. (1) Stansberry et al. (2008), (2) Sicardy et al. (2006) and references therein, (3) Brown et al. (2010), (4) Brown & Trujillo (2004), (5) Brown (2008), (6) Brucker et al. (2009), (7) computed from Buie et al. (2010), (8) Rabinowitz et al. (2006), (9) Cook et al. (2009), (10) Guilbert et al. (2009), (11) Schaller & Brown (2007a), (12) Dalle Ore et al. (2009), (13) Merlin et al. (2010a) and references therein.


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