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: 592245 # Created Tue Apr 1 01:07:35 2025 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 76 observations of 76 # Arc: 5.21y # First observation: 2013/09/13 # Last observation: 2018/11/30 # Chi-squared of fit: 81.47 DOF: 146 RMS: 0.18 # Min/Max residuals: -0.55 0.55 # Exact a, adot, b, bdot, g, gdot: 1.715128E-05 2.635893E-02 -1.649838E-07 -1.310612E-03 2.363219E-02 -1.998573E-03 # Covariance matrix: 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 # lat0 lon0 xBary yBary zBary JD0 -43.069546 -16.199746 -0.115448 -0.682961 -0.730760 2456548.841188 # Heliocentric elements and errors Epoch: 2456548.5000 = 2013/09/13 Mean Anomaly: 353.19518 +/- 0.000 Argument of Peri: 282.93526 +/- 0.000 Long of Asc Node: 78.03958 +/- 0.000 Inclination: 42.23166 +/- 0.000 Eccentricity: 0.37236493 +/- 0.0000 Semi-Major Axis: 67.87824438 +/- 0.0000 Time of Perihelion: 2460409.5779 +/- 0.0 Perihelion: 42.60276654 +/- 0.0000 Aphelion: 93.15372222 +/- 0.0000 Period (y) 559.2476 +/- 0.00 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 30.67753046 +/- 0.0000 Ecliptic Y -8.78914612 +/- 0.0000 Ecliptic Z -28.89645088 +/- 0.0000 Ecliptic XDOT 0.00058378 +/- 0.0000 Ecliptic YDOT 0.00300743 +/- 0.0000 Ecliptic ZDOT 0.00004733 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 43.05077999 +/- 0.0000 Geocenter to KBO 42.31526261 +/- 0.0000 # Hcoef: 6.76
The following table shows the complete astrometric record for 592245. 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 (592245) followed by the observatory code and reference code for the source of the astrometry.
2013 09 13.34041 00 27 31.244 -45 02 25.39 23.9g 592245 W84 C~4yTx 2013 10 03.03936 00 25 34.132 -45 09 21.55 24.3g 592245 W84 C~4yTx 2013 10 11.29010 00 24 44.829 -45 10 11.60 23.7g 592245 W84 C~4yTx 2013 11 21.18145 00 21 30.407 -44 55 26.57 22.6z 592245 W84 C~4yTx 2013 12 29.07716 00 20 56.125 -44 19 02.55 22.9r 592245 W84 C~4yTx 2013 12 30.09129 00 20 57.588 -44 17 53.31 23.4r 592245 W84 C~4yTx 2013 12 30.09268 00 20 57.594 -44 17 53.28 22.9i 592245 W84 C~4yTx 2014 01 13.05008 00 21 30.612 -44 01 35.66 22.5z 592245 W84 C~4yTx 2014 08 18.211973 00 36 58.95 -43 57 41.2 23.9g 592245 W84 C~1VcI 2014 08 18.214178 00 36 58.93 -43 57 41.1 23.1r 592245 W84 C~1VcI 2014 08 18.216528 00 36 58.92 -43 57 41.3 22.9i 592245 W84 C~1VcI 2014 08 18.220336 00 36 58.91 -43 57 41.5 22.8z 592245 W84 C~1VcI 2014 08 22.378200 00 36 42.08 -44 01 08.6 23.8g 592245 W84 C~1VcI 2014 08 22.380417 00 36 42.08 -44 01 08.8 22.9r 592245 W84 C~1VcI 2014 08 22.382778 00 36 42.07 -44 01 08.9 23.3i 592245 W84 C~1VcI 2014 08 22.386597 00 36 42.04 -44 01 09.2 23.0z 592245 W84 C~1VcI 2014 09 12.099317 00 34 59.66 -44 15 35.0 23.6r 592245 W84 C~1VcI 2014 09 12.105475 00 34 59.62 -44 15 35.1 23.4z 592245 W84 C~1VcI 2014 10 30.18358 00 30 22.825 -44 22 40.21 23.0z 592245 W84 C~4yTx 2014 11 15.20435 00 29 10.382 -44 15 26.85 23.1r 592245 W84 C~4yTx 2014 11 17.21304 00 29 02.780 -44 14 13.12 22.6r 592245 W84 C~4yTx 2014 11 21.06344 00 28 49.332 -44 11 40.92 22.5r 592245 W84 C~4yTx 2014 11 21.06488 00 28 49.323 -44 11 40.93 22.8i 592245 W84 C~4yTx 2015 01 08.047025 00 28 21.66 -43 24 20.1 23.0r 592245 W84 C~1VcI 2015 01 08.049375 00 28 21.66 -43 24 19.8 23.1i 592245 W84 C~1VcI 2015 01 08.053171 00 28 21.68 -43 24 19.5 22.8z 592245 W84 C~1VcI 2015 01 15.061291 00 28 40.70 -43 16 01.7 24.2g 592245 W84 C~1VcI 2015 01 15.063507 00 28 40.71 -43 16 01.5 23.4r 592245 W84 C~1VcI 2015 01 15.065868 00 28 40.71 -43 16 01.4 23.0i 592245 W84 C~1VcI 2015 01 15.069664 00 28 40.72 -43 16 01.2 23.5z 592245 W84 C~1VcI 2015 01 22.047500 00 29 05.21 -43 07 42.8 23.0r 592245 W84 C~1VcI 2015 01 22.049838 00 29 05.19 -43 07 42.5 23.1i 592245 W84 C~1VcI 2015 01 22.053634 00 29 05.23 -43 07 42.2 22.8z 592245 W84 C~1VcI 2015 01 29.039282 00 29 34.99 -42 59 27.1 23.3r 592245 W84 C~1VcI 2015 01 29.045428 00 29 35.03 -42 59 26.5 22.0z 592245 W84 C~1VcI 2015 09 13.188623 00 42 04.65 -43 28 08.1 22.7r 592245 W84 C~1ae1 2015 09 13.190984 00 42 04.64 -43 28 08.3 22.7i 592245 W84 C~1ae1 2015 09 13.194780 00 42 04.61 -43 28 08.3 22.7z 592245 W84 C~1ae1 2015 09 18.132292 00 41 37.13 -43 30 47.6 23.0r 592245 W84 C~1ae1 2015 09 18.134641 00 41 37.13 -43 30 47.6 23.3i 592245 W84 C~1ae1 2015 09 18.138438 00 41 37.10 -43 30 47.5 23.3z 592245 W84 C~1ae1 2015 09 26.084375 00 40 51.25 -43 34 15.0 23.4i 592245 W84 C~1ae1 2015 09 26.088194 00 40 51.21 -43 34 15.0 22.8z 592245 W84 C~1ae1 2015 10 16.021244 00 38 53.42 -43 38 03.1 24.1g 592245 W84 C~1ae1 2015 10 16.023449 00 38 53.41 -43 38 03.2 23.2r 592245 W84 C~1ae1 2015 10 16.025799 00 38 53.41 -43 38 03.3 23.3i 592245 W84 C~1ae1 2015 10 16.029595 00 38 53.37 -43 38 03.2 23.0z 592245 W84 C~1ae1 2015 10 30.010527 00 37 35.99 -43 36 13.6 23.9g 592245 W84 C~1cIX 2015 10 30.012743 00 37 35.96 -43 36 13.7 22.9r 592245 W84 C~1cIX 2015 10 30.015093 00 37 35.96 -43 36 13.6 22.9i 592245 W84 C~1cIX 2015 10 30.018900 00 37 35.95 -43 36 13.7 22.4z 592245 W84 C~1cIX 2015 11 03.029473 00 37 15.52 -43 35 01.1 23.7g 592245 W84 C~1cIX 2015 11 03.031678 00 37 15.52 -43 35 01.0 23.2r 592245 W84 C~1cIX 2015 11 03.034051 00 37 15.51 -43 35 00.9 22.9i 592245 W84 C~1cIX 2015 11 03.037847 00 37 15.50 -43 35 00.8 22.0z 592245 W84 C~1cIX 2015 11 08.227037 00 36 50.64 -43 32 59.7 23.2r 592245 W84 C~1cIX 2015 11 08.229398 00 36 50.62 -43 32 59.7 22.6i 592245 W84 C~1cIX 2015 11 08.233206 00 36 50.59 -43 32 59.5 22.7z 592245 W84 C~1cIX 2015 12 16.036736 00 35 03.92 -43 04 44.5 23.0i 592245 W84 C~1h5p 2015 12 16.040729 00 35 03.92 -43 04 44.4 22.7z 592245 W84 C~1h5p 2016 08 16.26533 00 51 04.496 -42 17 56.76 23.0z 592245 W84 C~4yTx 2016 09 01.34402 00 49 59.644 -42 30 59.79 23.2r 592245 W84 C~4yTx 2016 09 01.34539 00 49 59.635 -42 30 59.92 22.6i 592245 W84 C~4yTx 2016 09 01.34676 00 49 59.621 -42 30 59.91 23.7g 592245 W84 C~4yTx 2016 10 07.03786 00 46 43.290 -42 48 16.53 23.0i 592245 W84 C~4yTx 2016 10 07.03924 00 46 43.321 -42 48 16.46 23.4r 592245 W84 C~4yTx 2016 10 29.10066 00 44 37.977 -42 47 51.21 23.1r 592245 W84 C~4yTx 2016 11 19.06840 00 43 01.761 -42 38 53.60 23.4g 592245 W84 C~4yTx 2016 12 31.08393 00 41 57.125 -42 00 35.35 22.7i 592245 W84 C~4yTx 2017 01 06.08305 00 42 04.68 -41 53 41.1 22.8i 592245 W84 C~3cnK 2017 10 15.28835 00 52 48.137 -41 58 33.56 23.4g 592245 W84 C~4yTx 2017 10 19.21940 00 52 25.538 -41 58 41.04 22.8i 592245 W84 C~4yTx 2017 11 24.05856 00 49 33.770 -41 46 17.55 23.2r 592245 W84 C~4yTx 2017 11 26.16006 00 49 26.666 -41 44 50.96 22.9z 592245 W84 C~4yTx 2018 11 15.17163 00 56 50.072 -41 00 15.61 22.9i 592245 W84 C~4yTx 2018 11 30.13101 00 55 54.086 -40 51 04.68 23.1r 592245 W84 C~4yTx
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 0.23 0.00 -0.07
2 0.0539 0.00 0.27 0.00 -0.33
3 0.0765 0.00 0.30 0.00 -0.34
4 0.1885 0.00 -0.05 0.00 -0.26
5 0.2922 0.00 0.40 0.00 -0.15
6 0.2950 0.00 0.17 0.00 -0.19
7 0.2950 0.00 0.23 0.00 -0.26
8 0.3332 0.00 0.17 0.00 -0.18
9 0.9278 0.00 0.02 0.00 -0.03
10 0.9278 0.00 -0.15 0.00 0.18
11 0.9278 0.00 -0.16 0.00 0.10
12 0.9278 0.00 -0.09 0.00 0.10
13 0.9392 0.00 -0.14 0.00 0.20
14 0.9392 0.00 -0.00 0.00 0.11
15 0.9392 0.00 0.00 0.00 0.12
16 0.9392 0.00 -0.20 0.00 0.01
17 0.9959 0.00 -0.01 0.00 -0.03
18 0.9959 0.00 -0.09 0.00 0.08
19 1.1276 0.00 -0.02 0.00 -0.10
20 1.1714 0.00 0.36 0.00 -0.00
21 1.1769 0.00 0.12 0.00 0.10
22 1.1875 0.00 0.24 0.00 -0.12
23 1.1875 0.00 0.18 0.00 -0.19
24 1.3188 0.00 -0.22 0.00 -0.03
25 1.3188 0.00 -0.30 0.00 0.10
26 1.3189 0.00 -0.13 0.00 0.14
27 1.3380 0.00 0.13 0.00 0.10
28 1.3381 0.00 0.18 0.00 0.14
29 1.3381 0.00 0.07 0.00 0.07
30 1.3381 0.00 0.05 0.00 -0.01
31 1.3572 0.00 0.05 0.00 -0.07
32 1.3572 0.00 -0.39 0.00 0.06
33 1.3572 0.00 -0.01 0.00 0.09
34 1.3763 0.00 -0.25 0.00 0.02
35 1.3763 0.00 -0.07 0.00 0.19
36 1.9982 0.00 0.09 0.00 0.21
37 1.9982 0.00 0.13 0.00 0.09
38 1.9982 0.00 0.00 0.00 0.22
39 2.0118 0.00 -0.40 0.00 -0.08
40 2.0118 0.00 -0.20 0.00 -0.01
41 2.0118 0.00 -0.32 0.00 0.21
42 2.0335 0.00 0.25 0.00 0.03
43 2.0335 0.00 -0.01 0.00 0.12
44 2.0881 0.00 -0.10 0.00 0.07
45 2.0881 0.00 -0.06 0.00 -0.02
46 2.0881 0.00 0.15 0.00 -0.12
47 2.0881 0.00 -0.11 0.00 -0.02
48 2.1264 0.00 -0.02 0.00 0.34
49 2.1264 0.00 -0.30 0.00 0.21
50 2.1264 0.00 -0.11 0.00 0.27
51 2.1264 0.00 0.04 0.00 0.11
52 2.1374 0.00 -0.33 0.00 -0.03
53 2.1374 0.00 -0.16 0.00 0.02
54 2.1374 0.00 -0.13 0.00 0.07
55 2.1374 0.00 0.01 0.00 0.10
56 2.1516 0.00 0.03 0.00 0.00
57 2.1516 0.00 -0.11 0.00 -0.06
58 2.1517 0.00 -0.29 0.00 0.04
59 2.2552 0.00 -0.55 0.00 0.12
60 2.2552 0.00 -0.50 0.00 -0.02
61 2.9238 0.00 -0.01 0.00 -0.12
62 2.9678 0.00 0.22 0.00 -0.01
63 2.9678 0.00 0.18 0.00 -0.08
64 2.9678 0.00 0.07 0.00 -0.01
65 3.0656 0.00 -0.03 0.00 -0.01
66 3.0656 0.00 0.55 0.00 0.08
67 3.1260 0.00 0.20 0.00 -0.10
68 3.1834 0.00 0.21 0.00 -0.14
69 3.2984 0.00 0.39 0.00 -0.08
70 3.3148 0.00 0.44 0.00 0.06
71 4.0875 0.00 0.08 0.00 -0.19
72 4.0982 0.00 0.30 0.00 -0.12
73 4.1964 0.00 0.22 0.00 -0.03
74 4.2021 0.00 0.08 0.00 -0.12
75 5.1713 0.00 -0.24 0.00 -0.10
76 5.2123 0.00 -0.03 0.00 -0.17
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.
592245 quality flag:3 Type: SCATNEAR SCATNEAR SCATNEAR axisobj 68.561 68.561 68.562 ecceobj 0.379 0.379 0.379 incobj 42.256 42.256 42.256 qmin 41.943 41.943 41.943 qmax 95.170 95.173 95.149 amean 68.006 68.006 68.008 amin 67.253 67.254 67.238 amax 68.967 68.964 68.988 emean 0.363 0.363 0.363 emin 0.349 0.350 0.349 emax 0.381 0.381 0.380 imean 41.122 41.122 41.122 imin 40.687 40.688 40.687 imax 41.541 41.540 41.539 excite_mean 0.751 0.751 0.751 fracstop 1.000 1.000 1.000 cjmean 2.553 2.553 2.553 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 195.4 195.2 195.0 kozaiamp 180.0 180.0 180.0