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: 14XX47 # Created Thu Apr 18 01:16:56 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 37 observations of 37 # Arc: 5.93y # First observation: 2014/12/12 # Last observation: 2020/11/14 # Chi-squared of fit: 25.84 DOF: 68 RMS: 0.15 # Min/Max residuals: -0.52 0.62 # Exact a, adot, b, bdot, g, gdot: 1.534432E-05 2.242847E-02 -1.056584E-08 -1.570619E-03 2.299239E-02 -6.818538E-03 # Covariance matrix: 1.3370E-13 -9.3128E-14 -4.4780E-15 4.9613E-15 -3.1710E-14 -5.4223E-13 -9.3128E-14 1.4082E-13 4.4326E-15 -1.2312E-14 -1.1221E-14 1.0315E-12 -4.4780E-15 4.4326E-15 9.1121E-14 -3.3619E-14 5.9897E-15 4.2600E-14 4.9613E-15 -1.2312E-14 -3.3619E-14 2.3173E-14 4.6283E-15 -1.0441E-13 -3.1710E-14 -1.1221E-14 5.9897E-15 4.6283E-15 1.0727E-13 -2.7759E-14 -5.4223E-13 1.0315E-12 4.2600E-14 -1.0441E-13 -2.7759E-14 8.9831E-12 # lat0 lon0 xBary yBary zBary JD0 -26.559216 3.267907 -0.956399 -0.103649 -0.207791 2457003.629298 # Heliocentric elements and errors Epoch: 2457004.5000 = 2014/12/13 Mean Anomaly: 315.12993 +/- 0.008 Argument of Peri: 340.44635 +/- 0.014 Long of Asc Node: 102.19286 +/- 0.001 Inclination: 26.61574 +/- 0.000 Eccentricity: 0.30871067 +/- 0.0001 Semi-Major Axis: 51.62250486 +/- 0.0051 Time of Perihelion: 2473889.8984 +/- 17.7 Perihelion: 35.68608699 +/- 0.0076 Aphelion: 67.55892273 +/- 0.0095 Period (y) 370.9085 +/- 0.05 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 39.01423608 +/- 0.0006 Ecliptic Y 3.18736242 +/- 0.0000 Ecliptic Z -19.44660205 +/- 0.0003 Ecliptic XDOT -0.00096490 +/- 0.0000 Ecliptic YDOT 0.00261508 +/- 0.0000 Ecliptic ZDOT 0.00019584 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 43.70877274 +/- 0.0005 Geocenter to KBO 43.49289364 +/- 0.0006 # Hcoef: 6.99
The following table shows the complete astrometric record for 14XX47. 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 (14XX47) followed by the observatory code and reference code for the source of the astrometry.
2014 12 12.12852 00 56 28.724 -22 57 03.77 24.7g 14XX47 W84 C~4yVR 2014 12 12.13280 00 56 28.711 -22 57 03.60 23.4r 14XX47 W84 C~4yVR 2014 12 12.13280 00 56 28.71 -22 57 03.6 23.5r 14XX47 W84 C~3cpY 2014 12 16.07850 00 56 23.482 -22 55 03.21 23.8g 14XX47 W84 C~4yVR 2014 12 16.07850 00 56 23.48 -22 55 03.2 23.9g 14XX47 W84 C~3cpY 2014 12 16.07986 00 56 23.49 -22 55 03.1 23.2r 14XX47 W84 C~3cpY 2014 12 20.11189 00 56 19.602 -22 52 49.04 23.4i 14XX47 W84 C~4yVR 2014 12 20.11189 00 56 19.59 -22 52 48.8 23.4i 14XX47 W84 C~3cpY 2014 12 24.09869 00 56 17.251 -22 50 25.98 23.5g 14XX47 W84 C~4yVR 2014 12 24.09869 00 56 17.25 -22 50 26.0 23.7g 14XX47 W84 C~3cpY 2015 10 08.21414 01 05 41.09 -22 30 11.2 23.2r 14XX47 W84 C~3cpY 2015 10 08.21551 01 05 41.106 -22 30 11.43 23.2g 14XX47 W84 C~4yVR 2015 11 16.06728 01 02 51.865 -22 36 12.13 23.7r 14XX47 W84 C~4yVR 2015 11 16.06728 01 02 51.86 -22 36 12.1 23.6r 14XX47 W84 C~3cpY 2015 12 01.05023 01 02 05.291 -22 32 50.98 23.6g 14XX47 W84 C~4yVR 2016 08 16.35659 01 14 16.396 -21 26 59.76 22.6z 14XX47 W84 C~4yVR 2016 08 16.35797 01 14 16.389 -21 26 59.90 22.8i 14XX47 W84 C~4yVR 2016 08 16.35797 01 14 16.39 -21 26 59.9 23.2i 14XX47 W84 C~3cpY 2016 08 30.32419 01 13 38.418 -21 37 00.52 23.7r 14XX47 W84 C~4yVR 2016 08 30.32419 01 13 38.42 -21 37 00.5 23.8r 14XX47 W84 C~3cpY 2016 08 30.32556 01 13 38.406 -21 37 00.69 24.0g 14XX47 W84 C~4yVR 2016 08 30.32556 01 13 38.41 -21 37 00.7 24.2g 14XX47 W84 C~3cpY 2016 10 28.14359 01 09 24.542 -22 05 33.26 23.0i 14XX47 W84 C~4yVR 2016 10 28.14359 01 09 24.54 -22 05 33.2 23.1i 14XX47 W84 C~3cpY 2016 12 02.05774 01 07 16.519 -22 02 20.07 23.2i 14XX47 W84 C~4yVR 2016 12 02.06189 01 07 16.505 -22 02 19.86 23.3r 14XX47 W84 C~4yVR 2016 12 02.06189 01 07 16.51 -22 02 19.8 23.1r 14XX47 W84 C~3cpY 2016 12 02.06326 01 07 16.495 -22 02 19.87 23.9g 14XX47 W84 C~4yVR 2016 12 02.06326 01 07 16.49 -22 02 19.8 24.2g 14XX47 W84 C~3cpY 2016 12 21.04594 01 06 43.248 -21 53 33.27 23.4r 14XX47 W84 C~4yVR 2016 12 21.04594 01 06 43.25 -21 53 33.3 23.6r 14XX47 W84 C~3cpY 2016 12 21.04731 01 06 43.248 -21 53 33.24 23.1i 14XX47 W84 C~4yVR 2018 10 01.32900 01 22 16.214 -20 51 36.54 22.8i 14XX47 W84 C~4yVR 2018 11 30.17657 01 18 00.475 -20 59 58.02 23.0r 14XX47 W84 C~4yVR 2018 11 30.17794 01 18 00.474 -20 59 58.09 24.0g 14XX47 W84 C~4yVR 2020 11 14.207700 01 29 44.027 -19 54 35.07 23.0G 14XX47 G37 C~4Nuh 2020 11 14.288670 01 29 43.611 -19 54 35.58 14XX47 G37 C~4Nuh
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 0.12 0.00 -0.19
2 0.0000 0.00 0.02 0.00 -0.15
3 0.0000 0.00 0.01 0.00 -0.15
4 0.0108 0.00 -0.03 0.00 -0.05
5 0.0108 0.00 -0.06 0.00 -0.04
6 0.0108 0.00 0.12 0.00 0.02
7 0.0219 0.00 0.07 0.00 -0.02
8 0.0219 0.00 -0.11 0.00 0.22
9 0.0328 0.00 0.06 0.00 -0.03
10 0.0328 0.00 0.07 0.00 -0.01
11 0.8216 0.00 0.00 0.00 0.21
12 0.8216 0.00 0.34 0.00 0.01
13 0.9280 0.00 -0.24 0.00 0.06
14 0.9280 0.00 -0.17 0.00 0.03
15 0.9690 0.00 -0.10 0.00 -0.09
16 1.6789 0.00 0.11 0.00 0.07
17 1.6789 0.00 0.07 0.00 -0.01
18 1.6789 0.00 0.06 0.00 -0.01
19 1.7172 0.00 -0.02 0.00 0.06
20 1.7172 0.00 -0.05 0.00 0.04
21 1.7172 0.00 -0.10 0.00 -0.09
22 1.7172 0.00 -0.16 0.00 -0.08
23 1.8782 0.00 0.00 0.00 0.00
24 1.8782 0.00 0.03 0.00 -0.06
25 1.9738 0.00 0.11 0.00 -0.02
26 1.9738 0.00 0.14 0.00 0.17
27 1.9738 0.00 0.07 0.00 0.11
28 1.9738 0.00 -0.10 0.00 0.14
29 1.9738 0.00 -0.03 0.00 0.07
30 2.0258 0.00 -0.02 0.00 -0.04
31 2.0258 0.00 -0.05 0.00 -0.01
32 2.0258 0.00 -0.03 0.00 -0.03
33 3.8034 0.00 -0.05 0.00 0.05
34 3.9673 0.00 -0.03 0.00 0.13
35 3.9673 0.00 0.02 0.00 0.03
36 5.9249 0.00 0.62 0.00 0.19
37 5.9251 0.00 -0.52 0.00 -0.46
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.
14XX47 quality flag:3 Type: SCATNEAR SCATNEAR SCATNEAR axisobj 52.174 52.174 52.174 ecceobj 0.311 0.311 0.311 incobj 26.620 26.620 26.620 qmin 33.609 33.802 33.633 qmax 70.803 70.633 70.771 amean 51.754 51.639 51.711 amin 51.076 51.032 51.016 amax 52.504 52.504 52.494 emean 0.323 0.318 0.321 emin 0.297 0.293 0.294 emax 0.350 0.347 0.350 imean 24.399 24.560 24.483 imin 23.431 23.518 23.519 imax 25.290 25.403 25.391 excite_mean 0.525 0.524 0.524 fracstop 1.000 1.000 1.000 cjmean 2.841 2.841 2.841 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 168.2 164.8 167.0 kozaiamp 180.0 180.0 180.0