The following information shows the result of the orbit fit based on Gary Bernstein's method. Most of the information should be self-explanatory. Take special note that while the original Bernstein software works with barycentric coordinates, we convert these results into a heliocentric coordinate system.
# Object: 10JJ124 # Created Sat Apr 20 01:13:21 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 21 observations of 21 # Arc: 8.09y # First observation: 2010/05/11 # Last observation: 2018/06/14 # Chi-squared of fit: 26.97 DOF: 36 RMS: 0.20 # Min/Max residuals: -0.48 0.35 # Exact a, adot, b, bdot, g, gdot: 2.175954E-05 6.131334E-02 1.528870E-05 4.091340E-02 4.377024E-02 -5.542064E-03 # Covariance matrix: 1.2881E-13 -4.7450E-14 1.2513E-14 -2.1096E-14 1.6281E-14 -5.9559E-14 -4.7450E-14 1.3256E-13 -4.6242E-14 7.0293E-14 2.1007E-13 2.0221E-13 1.2513E-14 -4.6242E-14 1.2385E-13 -4.6760E-14 -7.1224E-14 -7.7905E-14 -2.1096E-14 7.0293E-14 -4.6760E-14 5.1748E-14 1.0015E-13 1.2017E-13 1.6281E-14 2.1007E-13 -7.1224E-14 1.0015E-13 6.0976E-13 2.9250E-13 -5.9559E-14 2.0221E-13 -7.7905E-14 1.2017E-13 2.9250E-13 3.4473E-13 # lat0 lon0 xBary yBary zBary JD0 -19.134911 -115.932757 0.247488 -0.321295 -0.925979 2455327.587566 # Heliocentric elements and errors Epoch: 2455328.5000 = 2010/05/12 Mean Anomaly: 358.78842 +/- 0.001 Argument of Peri: 339.63189 +/- 0.001 Long of Asc Node: 268.83448 +/- 0.000 Inclination: 37.74569 +/- 0.000 Eccentricity: 0.71855094 +/- 0.0001 Semi-Major Axis: 83.87520114 +/- 0.0249 Time of Perihelion: 2456272.7768 +/- 124.4 Perihelion: 23.60659664 +/- 0.0096 Aphelion: 144.14380565 +/- 0.0433 Period (y) 768.1722 +/- 0.34 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X -10.08589976 +/- 0.0002 Ecliptic Y -20.18662613 +/- 0.0003 Ecliptic Z -7.48862960 +/- 0.0001 Ecliptic XDOT 0.00322711 +/- 0.0000 Ecliptic YDOT -0.00213109 +/- 0.0000 Ecliptic ZDOT 0.00253135 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 23.77618658 +/- 0.0003 Geocenter to KBO 22.84664892 +/- 0.0004 # Hcoef: 6.64
The following table shows the complete astrometric record for 10JJ124. The first three columns show the date of observation. The next six columns are RA and DEC. The next column (when provided) is the observed magnitude and filter. The next column is the object name (10JJ124) followed by the observatory code and reference code for the source of the astrometry.
2010 05 11.08680 15 50 05.770 -39 41 43.00 20.2R 10JJ124 304 C~0HbC 2010 05 11.15146 15 50 05.165 -39 41 40.61 10JJ124 304 C~0HbC 2010 05 11.20653 15 50 04.625 -39 41 38.71 10JJ124 304 C~0HbC 2010 05 18.09365 15 48 58.975 -39 37 07.14 20.3R 10JJ124 304 C~0HbC 2010 05 18.20425 15 48 57.899 -39 37 02.20 10JJ124 304 C~0HbC 2010 05 18.29604 15 48 56.977 -39 36 58.27 10JJ124 304 C~0HbC 2010 05 25.13159 15 47 51.468 -39 31 43.06 19.7R 10JJ124 304 C~0I3j 2010 05 25.18979 15 47 50.881 -39 31 40.21 20.2R 10JJ124 304 C~0I3j 2010 05 25.24807 15 47 50.323 -39 31 37.32 10JJ124 304 C~0I3j 2011 05 03.16251 16 11 29.180 -38 09 10.86 19.6R 10JJ124 304 C~0Wc5 2011 05 03.24978 16 11 28.410 -38 09 08.79 10JJ124 304 C~0Wc5 2011 05 03.34601 16 11 27.550 -38 09 06.55 10JJ124 304 C~0Wc5 2011 05 12.10182 16 10 09.484 -38 05 02.39 10JJ124 304 C~0Wc5 2011 05 12.16775 16 10 08.868 -38 05 00.32 10JJ124 304 C~0Wc5 2013 08 01.04676 16 37 31.72 -33 13 08.4 19.7R 10JJ124 304 C~1oYc 2013 08 01.15525 16 37 31.32 -33 13 02.1 10JJ124 304 C~1oYc 2013 08 01.99417 16 37 28.59 -33 12 15.9 10JJ124 304 C~1oYc 2013 08 02.03814 16 37 28.43 -33 12 13.7 10JJ124 304 C~1oYc 2013 08 02.13134 16 37 28.12 -33 12 08.2 10JJ124 304 C~1oYc 2018 06 14.35756 18 02 25.213 -22 16 49.39 20.8R 10JJ124 G37 C~2kMZ 2018 06 14.42875 18 02 24.566 -22 16 47.48 10JJ124 G37 C~2kMZ
The following table shows the residuals to the orbit fit. The first coumn is the point number. The second column is the time, in years, measured from the first observation. The third and fifth columns are the regularized positions used in the orbit fit. The fourth and sixth columns are the residuals, in arc seconds, for RA and Dec respectively.
1 0.0000 0.00 0.07 0.00 -0.12
2 0.0002 0.00 0.29 0.00 0.00
3 0.0003 0.00 0.13 0.00 -0.06
4 0.0192 0.00 0.28 0.00 0.05
5 0.0195 0.00 0.35 0.00 0.29
6 0.0197 0.00 -0.03 0.00 0.25
7 0.0385 0.00 0.08 0.00 -0.06
8 0.0386 0.00 -0.23 0.00 -0.07
9 0.0388 0.00 -0.10 0.00 -0.07
10 0.9776 0.00 -0.12 0.00 -0.25
11 0.9779 0.00 -0.22 0.00 -0.20
12 0.9781 0.00 -0.48 0.00 -0.27
13 1.0021 0.00 -0.05 0.00 -0.09
14 1.0023 0.00 -0.04 0.00 -0.08
15 3.2251 0.00 0.28 0.00 0.05
16 3.2254 0.00 0.00 0.00 0.30
17 3.2277 0.00 0.03 0.00 0.24
18 3.2278 0.00 -0.14 0.00 0.02
19 3.2280 0.00 -0.11 0.00 0.34
20 8.0938 0.00 0.35 0.00 -0.21
21 8.0940 0.00 -0.23 0.00 -0.05
The following table comes from a 10My integration of the orbit of the object. Three columns are shown. The first column is the result of integrating the nominal orbit. The other two columns are based on clones of the nominal orbit that are +/- 3 sigma from the nominal orbit. If all three types agree then the classificiation is deemed secure. The basis for these calculations is described in more detail in AJ, 129, 1117 (2005). Any use made of these calculations should refer to and credit this publication and the Deep Ecliptic Survey Team.
10JJ124 quality flag:2 Type: CENTAURR CENTAURS CENTAURS axisobj 82.352 82.351 82.354 ecceobj 0.714 0.714 0.714 incobj 37.779 37.779 37.779 qmin 22.560 22.422 22.583 qmax 152.513 157.781 156.695 amean 83.675 86.847 85.971 amin 75.951 82.351 81.887 amax 87.798 90.930 91.021 emean 0.706 0.721 0.717 emin 0.624 0.685 0.675 emax 0.737 0.744 0.740 imean 40.164 39.793 39.968 imin 37.981 37.925 38.113 imax 44.729 43.052 43.636 excite_mean 0.957 0.964 0.963 fracstop 0.943 1.000 1.000 cjmean 2.159 2.152 2.153 libcent 0 -180.0 -180.0 -180.0 libamp 0 -180.0 -180.0 -180.0 libcent 1 -180.0 -180.0 -180.0 libamp 1 -180.0 -180.0 -180.0 libcent 2 -180.0 -180.0 -180.0 libamp 2 -180.0 -180.0 -180.0 libcent 3 -180.0 -180.0 -180.0 libamp 3 -180.0 -180.0 -180.0 libcent 4 -180.0 -180.0 -180.0 libamp 4 -180.0 -180.0 -180.0 kozaimean 92.1 102.5 92.6 kozaiamp 180.0 180.0 180.0