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: 541132 # Created Fri Apr 19 01:08:49 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 34 observations of 34 # Arc: 3.02y # First observation: 2015/10/13 # Last observation: 2018/10/20 # Chi-squared of fit: 39.02 DOF: 62 RMS: 0.19 # Min/Max residuals: -0.38 0.56 # Exact a, adot, b, bdot, g, gdot: 1.419094E-05 1.113703E-02 5.274389E-07 9.603096E-04 1.266846E-02 -5.308848E-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 10.769503 6.243987 -0.227154 0.182435 -0.958321 2457308.756450 # Heliocentric elements and errors Epoch: 2457308.5000 = 2015/10/13 Mean Anomaly: 359.33664 +/- 0.000 Argument of Peri: 118.25124 +/- 0.000 Long of Asc Node: 301.10850 +/- 0.000 Inclination: 11.68238 +/- 0.000 Eccentricity: 0.93863363 +/- 0.0000 Semi-Major Axis: 1055.28888080 +/- 0.0000 Time of Perihelion: 2480381.4686 +/- 0.0 Perihelion: 64.75924628 +/- 0.0000 Aphelion: 2045.81851531 +/- 0.0000 Period (y) 34281.9286 +/- 0.00 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 78.02711806 +/- 0.0000 Ecliptic Y 8.76624223 +/- 0.0000 Ecliptic Z 14.74993955 +/- 0.0000 Ecliptic XDOT -0.00142238 +/- 0.0000 Ecliptic YDOT 0.00225924 +/- 0.0000 Ecliptic ZDOT -0.00001046 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 79.89193956 +/- 0.0000 Geocenter to KBO 78.93673921 +/- 0.0000 # Hcoef: 5.51
The following table shows the complete astrometric record for 541132. 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 (541132) followed by the observatory code and reference code for the source of the astrometry.
2015 10 13.255661 00 05 33.685 +12 21 12.16 24.0G 541132 T09 C~2lVV 2015 10 13.341162 00 05 33.486 +12 21 10.71 24.0G 541132 T09 C~2lVV 2015 10 13.487574 00 05 33.145 +12 21 08.31 24.0G 541132 T09 C~2lVV 2015 12 07.03832 00 04 10.961 +12 07 26.32 24.3r 541132 304 C~2lVV 2015 12 09.07673 00 04 10.197 +12 07 04.63 24.2r 541132 304 C~2lVV 2016 09 25.16349 00 08 33.733 +12 44 17.33 24.0r 541132 304 C~2lVV 2016 09 25.24466 00 08 33.531 +12 44 16.25 24.1r 541132 304 C~2lVV 2016 09 26.11520 00 08 31.404 +12 44 03.50 24.0r 541132 304 C~2lVV 2016 09 28.23197 00 08 26.240 +12 43 31.76 24.1r 541132 304 C~2lVV 2016 10 01.23767 00 08 18.913 +12 42 46.07 24.0r 541132 304 C~2lVV 2016 11 02.12125 00 07 08.649 +12 33 58.44 541132 304 C~2lVV 2016 11 03.05868 00 07 06.943 +12 33 42.54 24.2r 541132 304 C~2lVV 2016 12 30.06127 00 06 30.754 +12 22 47.03 24.3r 541132 304 C~2lVV 2017 09 21.18143 00 11 04.641 +13 03 56.62 24.2R 541132 G37 C~2lVV 2017 09 21.18871 00 11 04.623 +13 03 56.15 24.1R 541132 G37 C~2lVV 2017 09 21.23762 00 11 04.505 +13 03 55.69 24.2R 541132 G37 C~2lVV 2017 09 21.25991 00 11 04.451 +13 03 55.12 24.1R 541132 G37 C~2lVV 2017 09 22.14910 00 11 02.269 +13 03 42.62 24.0R 541132 G37 C~2lVV 2017 12 13.05631 00 08 44.228 +12 43 11.02 541132 304 C~2lVV 2017 12 14.05111 00 08 44.094 +12 43 01.20 541132 304 C~2lVV 2018 05 16.41893 00 14 31.482 +13 13 23.50 24.3r 541132 304 C~2lVV 2018 05 19.42075 00 14 37.764 +13 14 25.34 24.2r 541132 304 C~2lVV 2018 10 15.991030 00 12 27.49 +13 16 19.2 24.4r 541132 950 C~2nvw 2018 10 16.937686 00 12 25.30 +13 16 03.4 24.7r 541132 950 C~2nvw 2018 10 16.946484 00 12 25.26 +13 16 03.3 24.6r 541132 950 C~2nvw 2018 10 16.955674 00 12 25.24 +13 16 03.2 24.5r 541132 950 C~2nvw 2018 10 17.917361 00 12 23.03 +13 15 46.9 24.8r 541132 950 C~2nvw 2018 10 17.922245 00 12 23.02 +13 15 46.8 24.6r 541132 950 C~2nvw 2018 10 17.926727 00 12 23.02 +13 15 46.7 24.7r 541132 950 C~2nvw 2018 10 17.933141 00 12 23.01 +13 15 46.6 24.9r 541132 950 C~2nvw 2018 10 17.937832 00 12 23.00 +13 15 46.4 25.0r 541132 950 C~2nvw 2018 10 17.952652 00 12 22.95 +13 15 46.1 24.8r 541132 950 C~2nvw 2018 10 17.957695 00 12 22.95 +13 15 46.0 25.1r 541132 950 C~2nvw 2018 10 20.215602 00 12 17.892 +13 15 07.50 541132 275 S~7mm3
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 -0.11 0.00 0.10
2 0.0002 0.00 -0.11 0.00 0.06
3 0.0006 0.00 -0.09 0.00 0.09
4 0.1500 0.00 -0.06 0.00 0.25
5 0.1556 0.00 0.04 0.00 -0.05
6 0.9525 0.00 -0.05 0.00 -0.15
7 0.9527 0.00 -0.05 0.00 -0.04
8 0.9551 0.00 -0.12 0.00 0.01
9 0.9609 0.00 0.07 0.00 -0.12
10 0.9691 0.00 0.01 0.00 0.18
11 1.0564 0.00 0.14 0.00 0.19
12 1.0590 0.00 0.21 0.00 -0.21
13 1.2151 0.00 0.00 0.00 0.13
14 1.9409 0.00 -0.01 0.00 0.14
15 1.9410 0.00 -0.01 0.00 -0.23
16 1.9411 0.00 0.04 0.00 -0.02
17 1.9411 0.00 0.06 0.00 -0.28
18 1.9436 0.00 -0.04 0.00 -0.38
19 2.1678 0.00 0.24 0.00 0.14
20 2.1706 0.00 0.40 0.00 -0.32
21 2.5905 0.00 0.35 0.00 -0.19
22 2.5987 0.00 0.39 0.00 -0.18
23 3.0082 0.00 0.17 0.00 -0.08
24 3.0108 0.00 0.06 0.00 0.11
25 3.0108 0.00 -0.23 0.00 0.16
26 3.0108 0.00 -0.21 0.00 0.21
27 3.0134 0.00 -0.34 0.00 0.20
28 3.0135 0.00 -0.32 0.00 0.18
29 3.0135 0.00 -0.16 0.00 0.15
30 3.0135 0.00 -0.09 0.00 0.16
31 3.0135 0.00 -0.07 0.00 0.04
32 3.0135 0.00 -0.31 0.00 -0.01
33 3.0136 0.00 -0.13 0.00 -0.02
34 3.0197 0.00 0.56 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.
541132 quality flag:3 Type: SCATNEAR SCATNEAR SCATNEAR axisobj 1416.815 1416.593 1417.037 ecceobj 0.954 0.954 0.954 incobj 11.674 11.674 11.674 qmin 51.988 51.990 51.986 qmax 2768.606 2831.624 2769.053 amean 1120.675 1121.504 1121.998 amin 981.550 977.801 968.068 amax 1416.812 1448.275 1417.034 emean 0.942 0.942 0.942 emin 0.929 0.929 0.930 emax 0.954 0.955 0.954 imean 13.234 13.234 13.233 imin 12.561 12.548 12.544 imax 14.042 14.030 14.057 excite_mean 0.969 0.969 0.969 fracstop 1.000 1.000 1.000 cjmean 4.012 4.012 4.012 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 118.7 118.7 118.7 kozaiamp 6.4 6.5 6.5