Table A.1
Asteroids in RMMRs with planets.
| Designation | a (au) | e | i | U | RMMR | n (f) | S | Resonant angle | k | Configurations |
|---|---|---|---|---|---|---|---|---|---|---|
| 2015 BZ509 | 5.137 | 0.391 | 163.0 | 2 | 1/−1J | 10 (100%) | 10.00 | Lib.at 180 | 1 | Currently in RMMR |
| 2000 DG8 | 10.76 | 0.794 | 129.3 | 4 | 1/−3J* | 10 (100%) | 10.00 | Lib.at 0 | 0 | Currently in RMMR |
| 2011 KT19 | 35.58 | 0.331 | 110.1 | 2 | 7/−9N | 10 (100%) | 10.00 | Lib.at 180 | 6 | Currently in polar RMMR |
| 2006 RJ2 | 9.675 | 0.762 | 164.6 | 7 | 2/−5J | 7 (38.9%) | 2.723 | Lib.at 180 | 2 | Capture in RMMR |
| 1/−1S | 10 (90.9%) | 9.090 | Lib.at 0 | 0 | Currently in RMMR | |||||
| 2018 DO4 | 25.75 | 0.907 | 160.5 | 4 | 1/−11J* | 10 (90.9%) | 9.090 | Lib.at 0 | 0 | Capture in RMMR |
| 2012 YO6 | 6.317 | 0.478 | 106.9 | 4 | 3/−4J* | 10 (88.2%) | 8.820 | Lib.at 180 | 3 | Capture in polar RMMR |
| 2005 NP82 | 5.870 | 0.478 | 130.5 | 1 | 5/−6J* | 10 (87.3%) | 8.730 | Lib.at 180 | 4 | Currently in RMMR |
| 2011 MM4 | 21.13 | 0.473 | 100.5 | 4 | 3/−10S | 10 (83.6%) | 8.360 | Lib.at 180 | 3 | Currently in polar RMMR |
| 5/−3N | 3 (36.3%) | 1.089 | Lib.at 180 | 4 | Capture in polar RMMR | |||||
| 2008 KV42 | 41.50 | 0.491 | 103.4 | 3 | 8/−13N | 10 (83.6%) | 8.360 | Lib.at 180 | 6 | Capture in polar RMMR |
| 2013 NS11 | 12.65 | 0.787 | 130.3 | 2 | 2/−3S* | 10 (78.2%) | 7.820 | Lib.at 180 | 0 | Capture in RMMR |
| 2009 QY6 | 12.47 | 0.835 | 137.6 | 4 | 2/−3S | 10 (77.3%) | 7.730 | Lib.at 180 | 0 | Currently in RMMR |
| 2016 LS | 13.34 | 0.608 | 114.3 | 4 | 1/−4J* | 9 (81.8%) | 7.362 | Lib.at 180 | 1 | Currently in RMMR |
| 3/−5S* | 5 (13.6%) | 0.680 | Lib.at 180 | 2 | Capture in RMMR | |||||
| 2016 JK24 | 13.05 | 0.660 | 152.3 | 3 | 1/−4J* | 8 (81.8%) | 6.544 | Lib.at 180 | 2 | Capture in RMMR |
| 2016 PN66 | 31.46 | 0.908 | 105.1 | 3 | 1/−15J* | 8 (81.8%) | 6.544 | Lib.at 0 | 0 | Capture in polar RMMR |
| 2017 SV13 | 9.682 | 0.793 | 113.2 | 6 | 2/−5J | 4 (19.1%) | 0.764 | Lib.at 180 | 3 | Capture in RMMR |
| 1/−1S | 9 (68.2%) | 6.138 | Lib.at 0 | 0 | Currently in RMMR | |||||
| 2009 HC82 | 2.527 | 0.807 | 154.4 | 0 | 3/−1J* | 7 (83.3%) | 5.831 | Lib.at 180 | 1 | Capture in RMMR |
| 1999 LE31 | 8.135 | 0.466 | 151.8 | 3 | 1/−2J* | 8 (68.2%) | 5.456 | Lib.at 0 | 0 | Capture in RMMR |
| 7/−1N* | 8 (68.2%) | 5.456 | Lib.at 0 | 0 | Capture in RMMR | |||||
| 2008 YB3 | 11.63 | 0.440 | 105.1 | 1 | 3/−10J | 10 (54.5%) | 5.450 | Lib.at 180 | 3 | Currently in polar RMMR |
| 2016 NM56 | 73.50 | 0.794 | 161.7 | 2 | 3/−11N* | 10 (45.5%) | 4.550 | Lib.at 180 | 4 | Capture in RMMR |
| 2012 YE8 | 9.380 | 0.592 | 136.1 | 7 | 2/−5J | 6 (23.9%) | 1.434 | Lib.at 180 | 0 | Capture in RMMR |
| 3/−7J* | 4 (22.3%) | 0.892 | Lib.at 180 | 2 | Capture in RMMR | |||||
| 1/−1S | 6 (68.2%) | 4.092 | Lib.at 0 | 0 | Capture in RMMR | |||||
| 2015 AO44 | 22.15 | 0.836 | 140.0 | 2 | 5/−6U* | 4 (83.6%) | 3.344 | Lib.at 180 | 5 | Capture in RMMR |
| 2008 SO218 | 8.112 | 0.565 | 170.3 | 2 | 1/−2J | 6 (47.3%) | 2.838 | Lib.at 180 | 1 | Currently in RMMR |
| 7/−1N* | 8 (36.4%) | 2.912 | Lib.at 180 | 4 | Capture in RMMR | |||||
| 2006 BZ8 | 9.606 | 0.803 | 165.3 | 2 | 2/−5J | 8 (33.7%) | 2.696 | Lib.at 180 | 0 | Currently in RMMR |
| 1/−1S | 3 (11.4%) | 0.342 | Lib.at 0 | 0 | Capture in RMMR | |||||
| 2014 AT28 | 10.93 | 0.404 | 165.6 | 3 | 1/−3J* | 4 (54.5%) | 2.180 | Lib.at 180 | 0 | Capture in RMMR |
| 2016 FH13 | 24.55 | 0.615 | 93.5 | 3 | 9/−13U* | 4 (54.5%) | 2.180 | Lib.at 180 | 5 | Capture in polar RMMR |
| 2015 XX351 | 14.61 | 0.854 | 159.1 | 3 | 3/−14J* | 3 (62.6%) | 1.878 | Lib.at 180 | 3 | Capture in RMMR |
| 2012 TL139 | 30.14 | 0.883 | 160.0 | 7 | 1/−14J* | 8 (21.4%) | 1.712 | Lib.at 0 | 0 | Currently in RMMR |
| 2009 YS6 | 20.18 | 0.921 | 147.8 | 2 | 1/−3S* | 3 (54.5%) | 1.635 | Lib.at 180 | 2 | Capture in RMMR |
| 2016 VY17 | 11.20 | 0.851 | 148.4 | 2 | 4/−13J* | 9 (17.7%) | 1.593 | Lib.at 0 | 0 | Capture in RMMR |
| 2014 SQ339 | 28.66 | 0.903 | 128.5 | 7 | 1/−13J* | 8 (18.3%) | 1.464 | Lib.at 180 | 2 | Capture in RMMR |
| 6/−11U* | 5 (13.9%) | 0.695 | Lib.at 180 | 1 | Capture in RMMR | |||||
| 2016 TK2 | 9.180 | 0.552 | 92.3 | 4 | 3/−7J* | 6 (21.4%) | 1.284 | Lib.at 180 | 2 | Capture in polar RMMR |
| 2011 SP25 | 19.58 | 0.884 | 109.0 | 6 | 1/−3S* | 4 (32.1%) | 1.284 | Lib.at 0 | 0 | Capture in polar RMMR |
| 2005 TJ50 | 9.240 | 0.589 | 110.2 | 7 | 3/−7J* | 7 (18.2%) | 1.274 | Lib.at 180 | 3 | Capture in polar RMMR |
| 1/−1S* | 1 (16.9%) | 0.169 | Lib.at 0 | 0 | Currently in polar RMMR | |||||
| 2017 NM2 | 14.67 | 0.625 | 101.3 | 4 | 3/−14J* | 3 (36.4%) | 1.092 | Lib.at 180 | 3 | Capture in polar RMMR |
| 2017 QO33 | 34.55 | 0.857 | 148.8 | 4 | 1/−7S* | 3 (27.3%) | 0.819 | Lib.at 180 | 2 | Capture in RMMR |
| 4/−5N* | 2 (31.8%) | 0.636 | Lib.at 180 | 4 | Capture in RMMR | |||||
| 2017 UX51 | 30.26 | 0.749 | 90.5 | 5 | 1/−14J* | 3 (13.6%) | 0.408 | Lib.at 180 | 2 | Currently in polar RMMR |
| 2016 YB13 | 5.460 | 0.408 | 139.7 | 2 | 13/−5S* | 2 (19.1%) | 0.382 | Lib.at 0 | 0 | Capture in RMMR |
| 2016 TP93 | 7.479 | 0.560 | 138.3 | 7 | 4/−1U* | 1 (13.6%) | 0.136 | Lib.at 0 | 1 | Capture in RMMR |
Notes. The orbital elements and condition codes U are taken from the website of the JPL Small-Body Database Search Engine, retrieved on 10 April 2019. In the sixth column J, S, U, and N are acronyms of Jupiter, Saturn, Uranus, and Neptune, respectively. The asterisk indicates the original results. The value of the seventh column n presents the number of clones (including the nominal one) that are trapped in this RMMR. The data given in the parentheses f are longest times that the resonant clones remain trapped in corresponding RMMR relative to the whole integration time-span (−10 000 to 100 000 yr). Resonant status S and resonant angle ϕ are defined as in Eqs. (3) and (2), respectively. The parameter k of the resonant angle is also indicated. The last column shows whether an asteroid is currently in RMMR or will be captured in RMMR in our numerical calculation. Objects are ordered by their resonant status from high to low S. If an asteroid evolves in several RMMRs, we sort it according to the best resonant status.
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