Table 1
Trans-Neptunian objects studied in this paper.
Name | kp:k | LY07 | GL08 | GL12 | SH16 | BA16 | a 0 | η 0 | −2πJ | ω |
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2001 KG76 | 4:9 | ⋆ | × | 51.718 | 0.939 | 0.02 | 2.668 | 34.017 | ||||
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(42301) | 2001 UR163 | 4:9 | ⋆ | × | 51.719 | 0.958 | 0.04 | 6.148 | 36.974 | |||
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(95625) | 2002 GX32 | 3:7 | ⋆ | × | 52.987 | 0.901 | 0.07 | 3.359 | 33.146 | |||
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2002 CZ248 | 3:7 | ⋆ | 52.987 | 0.919 | 0.026 | 5.252 | 32.413 | |||||
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(131696) | 2001 XT254 | 3:7 | ⋆ | × | ⋆ | 52.988 | 0.946 | 0.04 | 3.294 | 35.910 | ||
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(181867) | 1999 CV118 | 3:7 | × | 52.988 | 0.949 | 0.04 | 2.650 | 37.493 | ||||
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(79978) | 1999 CC158 | 5:12 | × | 53.991 | 0.904 | 0.017 | 1.841 | 39.096 | ||||
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(119878) | 2002 CY224 | 5:12 | ⋆ | × | 53.991 | 0.896 | 0.011 | 2.689 | 35.275 | |||
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(84522) | 2002 TC302 | 2:5 | × | 55.474 | 0.784 | 0.13 | 1.585 | 39.002 | ||||
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(26375) | 1999 DE9 | 2:5 | ⋆ | × | 55.478 | 0.897 | 0.18 | 2.884 | 32.283 | |||
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(60621) | 2000 FE8 | 2:5 | ⋆ | × | ⋆ | 55.479 | 0.909 | 0.05 | 2.739 | 33.109 | ||
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(38084) | 1999 HB12 | 2:5 | ⋆ | × | 55.480 | 0.890 | 0.105 | 1.052 | 32.615 | |||
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2004 KZ18 | 2:5 | ⋆ | 55.480 | 0.847 | 0.0015 | 0.136 | 34.310 | |||||
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2004 EG96 | 2:5 | ⋆ | ⋆ | 55.481 | 0.871 | 0.045 | 0.185 | 32.110 | ||||
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2002 GP32 | 2:5 | ⋆ | × | ⋆ | 55.481 | 0.907 | 0.0013 | 0.463 | 32.081 | |||
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2000 SR331 | 2:5 | ⋆ | × | 55.481 | 0.896 | 0.023 | 3.812 | 31.157 | ||||
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(143707) | 2003 UY117 | 2:5 | ⋆ | × | 55.481 | 0.899 | 0.064 | 1.895 | 32.510 | |||
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(135571) | 2002 GG32 | 2:5 | ⋆ | × | 55.481 | 0.907 | 0.03 | 4.140 | 35.905 | |||
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(69988) | 1998 WA31 | 2:5 | ⋆ | × | 55.481 | 0.890 | 0.12 | 5.571 | 31.581 | |||
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(119068) | 2001 KC77 | 2:5 | ⋆ | × | 55.482 | 0.913 | 0.24 | 3.239 | 35.455 | |||
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2004 HO79 | 2:5 | ⋆ | 55.482 | 0.907 | 0.08 | 2.359 | 32.507 | |||||
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2001 XQ254 | 2:5 | ⋆ | × | 55.484 | 0.894 | 0.19 | 0.189 | 31.089 | ||||
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2015 GP50 | 2:5 | × | ||||||||||
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2012 FH84 | 2:5 | × | ||||||||||
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(82075) | 2000 YW134 | 3:8 | ⋆ | × | 57.920 | 0.909 | 0.00035 | 5.489 | 41.146 | |||
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2004 XR190 | 3:8 | × | ||||||||||
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2015 FJ345 | 1:3 | × | 62.649 | 0.809 | 0.065 | 1.391 | 50.905 | |||||
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(136120) | 2003 LG7 | 1:3 | ⋆ | × | 62.660 | 0.817 | 0.5 | 5.913 | 32.483 | |||
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2015 KH162 | 1:3 | × | ||||||||||
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2013 FQ28 | 1:3 | × | ||||||||||
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(160148) | 2001 KV76 | 2:7 | × | 69.430 | 0.835 | 0.076 | 4.098 | 34.421 | ||||
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(126619) | 2002 CX154 | 3:11 | × | |||||||||
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2014 FC69 | 3:11 | × | ||||||||||
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2014 FZ71 | 1:4 | × | 75.900 | 0.860 | 0.035 | 4.277 | 56.117 | |||||
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2015 RR245 | 2:9 | ⋆ | 82.100 | 0.802 | 0.075 | 4.360 | 33.942 | |||||
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(26181) | 1996 GQ21 | 2:11 | × | |||||||||
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2008 ST291 | 1:6 | × | 99.453 | 0.761 | 0.003 | 5.721 | 42.566 | |||||
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(184212) | 2004 PB112 | 5:27 | × | 107.575 | 0.713 | 0.0055 | 0.158 | 35.392 |
Notes. The resonance ratios kp:k are all with Neptune. The references used are abbreviated in LY07 (Lykawka & Mukai 2007), GL08 (Gladman et al. 2008), GL12 (Gladman et al. 2012), SH16 (Sheppard et al. 2016) and BA16 (Bannister et al. 2016). A cross indicates that the object is classified as “resonant”; a star indicates that the article provides also the oscillation amplitude of the resonant angle with its uncertainty. In LY07 and GL12, the star is omitted if the classification is said “insecure”. The right part of the table gives the characteristics of the resonant secular models obtained in this paper: a0 is the reference semi-major axis chosen (au) whereas η0 (no unit) and −2πJ (au2 rad2 yr-1) are the fixed parameters. Finally, ω (rad) and (au) are the current secular argument of perihelion and reference perihelion distance of the object (see Sect. 2.1). Blank fields mean that the object was found non-resonant in the numerical integration starting from the nominal orbit given by AstDyS database. In the particular case of 2014 FZ71, a secular model was developed although the nominal orbital solution was not resonant (see Sect. 3.3). In theory, the 1-sigma error bars would allow it also for 2015 GP50, 2012 FH84 and 2013 FQ28.
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