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: 15KG175
# Created Wed Apr 24 01:17:17 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 39 observations of 39
# Arc: 6.95y
# First observation: 2014/05/30
# Last observation: 2021/05/12
# Chi-squared of fit: 5.60 DOF: 72 RMS: 0.07
# Min/Max residuals: -0.13 0.20
# Exact a, adot, b, bdot, g, gdot:
1.394492E-05 2.124027E-02 4.595121E-07 1.038462E-03 2.293166E-02 1.411845E-03
# Covariance matrix:
1.5780E-13 -1.2535E-13 3.7136E-15 -4.6615E-15 -2.3441E-14 -6.8297E-13
-1.2535E-13 1.4703E-13 -5.6927E-15 6.0176E-15 -1.6450E-16 8.7824E-13
3.7136E-15 -5.6927E-15 7.6013E-14 -2.5877E-14 2.9662E-15 -3.7744E-14
-4.6615E-15 6.0176E-15 -2.5877E-14 1.7773E-14 1.1762E-16 4.0835E-14
-2.3441E-14 -1.6450E-16 2.9662E-15 1.1762E-16 1.0417E-13 2.8883E-14
-6.8297E-13 8.7824E-13 -3.7744E-14 4.0835E-14 2.8883E-14 5.9630E-12
# lat0 lon0 xBary yBary zBary JD0
6.940797 -125.183443 -0.246198 0.119019 -0.977251 2456807.910378
# Heliocentric elements and errors
Epoch: 2456808.5000 = 2014/05/31
Mean Anomaly: 105.03225 +/- 0.069
Argument of Peri: 314.50525 +/- 0.061
Long of Asc Node: 167.33698 +/- 0.003
Inclination: 7.32599 +/- 0.000
Eccentricity: 0.07833366 +/- 0.0001
Semi-Major Axis: 43.46209507 +/- 0.0031
Time of Perihelion: 2426274.4394 +/- 20.2
Perihelion: 40.05755001 +/- 0.0049
Aphelion: 46.86664012 +/- 0.0052
Period (y) 286.5327 +/- 0.03
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -25.30988942 +/- 0.0003
Ecliptic Y -36.32499280 +/- 0.0005
Ecliptic Z 5.26981263 +/- 0.0001
Ecliptic XDOT 0.00197960 +/- 0.0000
Ecliptic YDOT -0.00158934 +/- 0.0000
Ecliptic ZDOT 0.00014357 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 44.58544962 +/- 0.0005
Geocenter to KBO 43.60782898 +/- 0.0006
# Hcoef: 7.36
The following table shows the complete astrometric record for 15KG175. 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 (15KG175) followed by the observatory code and reference code for the source of the astrometry.
2014 05 30.40960 15 36 42.907 -12 13 51.55 23.5r 15KG175 568 C~2nvg 2014 06 01.33608 15 36 34.442 -12 13 25.20 23.9r 15KG175 568 C~2nvg 2014 06 01.37892 15 36 34.251 -12 13 24.69 23.3r 15KG175 568 C~2nvg 2014 06 01.42181 15 36 34.065 -12 13 24.09 23.9r 15KG175 568 C~2nvg 2014 06 22.33318 15 35 10.088 -12 09 42.26 23.8r 15KG175 568 C~2nvg 2014 06 22.37610 15 35 09.916 -12 09 42.03 23.6r 15KG175 568 C~2nvg 2014 07 19.34974 15 33 56.524 -12 08 21.10 23.8r 15KG175 568 C~2nvg 2015 02 25.63010 15 46 24.559 -12 52 17.08 24.0r 15KG175 568 C~2nvg 2015 03 19.62451 15 46 05.934 -12 47 39.36 23.6r 15KG175 568 C~2nvg 2015 03 22.54324 15 46 00.341 -12 46 54.43 23.9r 15KG175 568 C~2nvg 2015 04 13.55598 15 44 58.040 -12 40 38.27 23.9r 15KG175 568 C~2nvg 2015 04 13.59705 15 44 57.891 -12 40 37.60 23.9r 15KG175 568 C~2nvg 2015 04 18.56046 15 44 39.694 -12 39 07.42 24.0r 15KG175 568 C~2nvg 2015 05 21.32647 15 42 18.605 -12 29 36.98 23.7r 15KG175 568 C~2nvg 2015 05 21.36772 15 42 18.417 -12 29 36.33 23.6r 15KG175 568 C~2nvg 2015 05 21.40894 15 42 18.226 -12 29 35.76 23.6r 15KG175 568 C~2nvg 2015 05 22.48541 15 42 13.335 -12 29 19.18 24.0r 15KG175 568 C~2nvg 2015 05 25.47599 15 41 59.806 -12 28 34.24 23.8r 15KG175 568 C~2nvg 2015 06 20.36530 15 40 10.869 -12 23 32.24 23.7r 15KG175 568 C~2nvg 2015 06 20.40617 15 40 10.710 -12 23 31.92 23.7r 15KG175 568 C~2nvg 2015 07 11.29956 15 39 04.945 -12 21 51.80 24.1r 15KG175 568 C~2nvg 2015 07 11.30916 15 39 04.921 -12 21 51.68 23.9r 15KG175 568 C~2nvg 2015 07 18.36957 15 38 49.228 -12 21 50.93 23.8r 15KG175 568 C~2nvg 2016 02 06.64936 15 50 51.052 -13 06 56.03 24.4w 15KG175 568 C~2nvg 2016 02 12.63490 15 51 01.547 -13 06 28.63 24.3w 15KG175 568 C~2nvg 2016 03 17.61801 15 50 58.733 -13 00 36.89 24.2w 15KG175 568 C~2nvg 2016 03 17.63019 15 50 58.706 -13 00 36.53 24.2w 15KG175 568 C~2nvg 2016 03 17.64294 15 50 58.703 -13 00 36.63 24.4w 15KG175 568 C~2nvg 2016 04 03.57496 15 50 20.251 -12 56 08.50 24.0w 15KG175 568 C~2nvg 2016 04 08.62452 15 50 04.777 -12 54 41.67 24.1w 15KG175 568 C~2nvg 2016 04 09.56848 15 50 01.716 -12 54 25.24 24.1w 15KG175 568 C~2nvg 2016 04 29.50952 15 48 46.023 -12 48 32.04 24.0w 15KG175 568 C~2nvg 2016 05 04.48214 15 48 24.687 -12 47 05.30 24.1w 15KG175 568 C~2nvg 2016 05 30.45796 15 46 27.900 -12 40 21.46 23.9w 15KG175 568 C~2nvg 2016 07 04.31842 15 44 13.510 -12 35 19.00 24.0w 15KG175 568 C~2nvg 2016 07 05.39078 15 44 10.340 -12 35 15.51 24.1w 15KG175 568 C~2nvg 2017 07 28.31662 15 48 12.358 -12 48 19.68 15KG175 568 C~2nvg 2021 05 12.394040 16 12 16.245 -13 44 21.50 23.5G 15KG175 G37 C~4pVs 2021 05 12.425650 16 12 16.107 -13 44 21.29 15KG175 G37 C~4pVs
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 0.16 0.00 0.02
2 0.0053 0.00 -0.00 0.00 0.04
3 0.0054 0.00 -0.01 0.00 -0.03
4 0.0055 0.00 0.06 0.00 -0.00
5 0.0628 0.00 0.11 0.00 0.00
6 0.0629 0.00 -0.12 0.00 -0.09
7 0.1367 0.00 -0.10 0.00 0.05
8 0.7426 0.00 0.02 0.00 -0.05
9 0.8028 0.00 -0.13 0.00 -0.04
10 0.8108 0.00 -0.08 0.00 0.03
11 0.8710 0.00 -0.06 0.00 0.03
12 0.8711 0.00 -0.07 0.00 -0.04
13 0.8847 0.00 0.02 0.00 -0.07
14 0.9744 0.00 0.02 0.00 0.08
15 0.9746 0.00 0.06 0.00 0.09
16 0.9747 0.00 0.05 0.00 0.03
17 0.9776 0.00 0.04 0.00 0.02
18 0.9858 0.00 0.01 0.00 0.03
19 1.0567 0.00 0.00 0.00 0.02
20 1.0568 0.00 -0.04 0.00 0.01
21 1.1140 0.00 0.03 0.00 -0.05
22 1.1140 0.00 0.04 0.00 0.06
23 1.1334 0.00 -0.12 0.00 0.01
24 1.6899 0.00 -0.00 0.00 -0.07
25 1.7063 0.00 0.04 0.00 -0.02
26 1.7993 0.00 0.02 0.00 -0.02
27 1.7994 0.00 -0.08 0.00 0.17
28 1.7994 0.00 0.20 0.00 -0.12
29 1.8458 0.00 -0.07 0.00 -0.03
30 1.8596 0.00 -0.10 0.00 0.01
31 1.8622 0.00 0.00 0.00 -0.00
32 1.9168 0.00 0.03 0.00 -0.01
33 1.9304 0.00 0.05 0.00 0.07
34 2.0015 0.00 -0.06 0.00 -0.04
35 2.0969 0.00 0.04 0.00 -0.02
36 2.0999 0.00 0.05 0.00 -0.05
37 3.1620 0.00 -0.04 0.00 0.06
38 6.9514 0.00 -0.03 0.00 0.12
39 6.9514 0.00 0.02 0.00 -0.13
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.
15KG175 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 43.209 43.210 43.209 ecceobj 0.077 0.077 0.077 incobj 7.342 7.342 7.342 qmin 39.233 39.225 39.211 qmax 48.039 48.033 48.060 amean 43.522 43.521 43.522 amin 43.171 43.177 43.173 amax 43.893 43.894 43.883 emean 0.080 0.080 0.080 emin 0.065 0.064 0.065 emax 0.096 0.096 0.096 imean 7.275 7.275 7.275 imin 6.519 6.519 6.521 imax 8.070 8.068 8.073 excite_mean 0.150 0.150 0.150 fracstop 1.000 1.000 1.000 cjmean 3.069 3.069 3.069 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 178.5 178.7 178.7 kozaiamp 179.9 179.9 180.0