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: 14VB41 # Created Wed Dec 25 02:10:06 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 35 observations of 35 # Arc: 7.09y # First observation: 2013/10/11 # Last observation: 2020/11/14 # Chi-squared of fit: 6.35 DOF: 64 RMS: 0.08 # Min/Max residuals: -0.19 0.30 # Exact a, adot, b, bdot, g, gdot: 1.770287E-05 2.866419E-02 4.411514E-06 7.440610E-03 2.640842E-02 -5.168576E-03 # Covariance matrix: 4.3250E-13 -2.4127E-13 7.1910E-14 -5.3270E-14 -2.1075E-14 -9.6868E-13 -2.4127E-13 1.6614E-13 -5.5378E-14 4.1123E-14 1.0147E-14 7.4790E-13 7.1910E-14 -5.5378E-14 1.9819E-13 -6.0189E-14 -6.2791E-15 -2.7348E-13 -5.3270E-14 4.1123E-14 -6.0189E-14 2.6031E-14 1.9427E-15 2.0337E-13 -2.1075E-14 1.0147E-14 -6.2791E-15 1.9427E-15 1.6760E-13 3.2433E-14 -9.6868E-13 7.4790E-13 -2.7348E-13 2.0337E-13 3.2433E-14 3.6990E-12 # lat0 lon0 xBary yBary zBary JD0 -10.358911 6.547428 -0.193768 -0.175928 -0.963119 2456576.734588 # Heliocentric elements and errors Epoch: 2456576.5000 = 2013/10/11 Mean Anomaly: 338.80343 +/- 0.007 Argument of Peri: 6.26811 +/- 0.015 Long of Asc Node: 40.75108 +/- 0.000 Inclination: 17.70636 +/- 0.000 Eccentricity: 0.31867541 +/- 0.0001 Semi-Major Axis: 53.53894807 +/- 0.0051 Time of Perihelion: 2465001.4286 +/- 19.6 Perihelion: 36.47740211 +/- 0.0047 Aphelion: 70.60049403 +/- 0.0074 Period (y) 391.7536 +/- 0.06 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 37.95660958 +/- 0.0006 Ecliptic Y 4.55464040 +/- 0.0001 Ecliptic Z -6.80883223 +/- 0.0001 Ecliptic XDOT -0.00073089 +/- 0.0000 Ecliptic YDOT 0.00290662 +/- 0.0000 Ecliptic ZDOT 0.00085531 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 38.83063245 +/- 0.0006 Geocenter to KBO 37.86687317 +/- 0.0006 # Hcoef: 7.28
The following table shows the complete astrometric record for 14VB41. 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 (14VB41) followed by the observatory code and reference code for the source of the astrometry.
2013 10 11.23381 00 40 28.857 -06 54 46.03 24.7g 14VB41 W84 C~4yV3 2014 09 21.19136 00 47 31.73 -05 42 45.3 14VB41 W84 C~3coV 2014 09 21.27145 00 47 31.34 -05 42 47.5 23.6V 14VB41 W84 C~3coV 2014 09 21.31846 00 47 31.12 -05 42 48.9 14VB41 W84 C~3coV 2014 11 14.12837 00 43 25.10 -06 00 24.6 23.4i 14VB41 W84 C~3coV 2014 11 14.12975 00 43 25.091 -06 00 24.53 22.9i 14VB41 W84 C~4yV3 2014 11 16.16255 00 43 17.983 -06 00 35.30 23.4r 14VB41 W84 C~4yV3 2014 11 16.16392 00 43 17.981 -06 00 35.28 23.4r 14VB41 W84 C~4yV3 2015 09 04.29212 00 54 12.47 -04 30 35.6 22.6z 14VB41 W84 C~3coV 2015 09 04.29349 00 54 12.47 -04 30 35.7 22.9i 14VB41 W84 C~3coV 2015 11 02.11053 00 49 37.705 -04 54 50.97 22.5r 14VB41 W84 C~4yV3 2015 11 16.05865 00 48 42.117 -04 57 16.83 23.1r 14VB41 W84 C~4yV3 2016 08 26.36563 01 00 09.055 -03 22 21.80 22.8i 14VB41 W84 C~4yV3 2016 08 26.36701 01 00 09.043 -03 22 21.68 23.4r 14VB41 W84 C~4yV3 2016 08 26.36839 01 00 09.048 -03 22 21.73 22.1z 14VB41 W84 C~4yV3 2016 09 01.38668 00 59 47.532 -03 25 03.69 24.3g 14VB41 W84 C~4yV3 2016 11 05.20636 00 54 47.225 -03 51 25.56 22.8i 14VB41 W84 C~4yV3 2016 11 05.20773 00 54 47.218 -03 51 25.59 23.3r 14VB41 W84 C~4yV3 2016 11 05.20910 00 54 47.211 -03 51 25.64 24.0g 14VB41 W84 C~4yV3 2016 11 06.12076 00 54 43.356 -03 51 37.61 22.3z 14VB41 W84 C~4yV3 2016 11 06.20939 00 54 42.981 -03 51 38.86 22.4i 14VB41 W84 C~4yV3 2016 11 06.21077 00 54 42.976 -03 51 38.78 23.1r 14VB41 W84 C~4yV3 2016 11 07.20345 00 54 38.815 -03 51 51.31 23.6g 14VB41 W84 C~4yV3 2016 11 08.15923 00 54 34.871 -03 52 02.81 22.5z 14VB41 W84 C~4yV3 2017 08 28.36267 01 05 31.356 -02 18 01.14 23.2r 14VB41 W84 C~4yV3 2017 08 28.36404 01 05 31.351 -02 18 01.13 22.9i 14VB41 W84 C~4yV3 2017 08 28.36542 01 05 31.356 -02 18 01.00 23.7g 14VB41 W84 C~4yV3 2017 09 14.31264 01 04 24.767 -02 25 41.36 22.5z 14VB41 W84 C~4yV4 2017 09 24.25052 01 03 39.180 -02 30 20.53 23.5g 14VB41 W84 C~4yV4 2018 10 10.27473 01 07 53.946 -01 31 20.23 22.6i 14VB41 W84 C~4yV4 2018 10 10.27611 01 07 53.941 -01 31 20.32 22.5r 14VB41 W84 C~4yV4 2018 10 10.27748 01 07 53.937 -01 31 20.35 23.5g 14VB41 W84 C~4yV4 2018 10 19.15341 01 07 09.545 -01 34 55.49 22.5z 14VB41 W84 C~4yV4 2020 11 14.106150 01 16 17.363 +00 30 40.22 22.8G 14VB41 G37 C~4Nte 2020 11 14.163520 01 16 17.133 +00 30 39.14 14VB41 G37 C~4Nte
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 -0.04
2 0.9444 0.00 0.04 0.00 -0.05
3 0.9447 0.00 -0.03 0.00 0.04
4 0.9448 0.00 0.06 0.00 -0.01
5 1.0921 0.00 -0.01 0.00 0.02
6 1.0921 0.00 -0.07 0.00 0.10
7 1.0977 0.00 -0.06 0.00 0.14
8 1.0977 0.00 -0.02 0.00 0.17
9 1.8975 0.00 0.02 0.00 0.02
10 1.8975 0.00 0.10 0.00 -0.04
11 2.0585 0.00 -0.05 0.00 -0.03
12 2.0967 0.00 0.03 0.00 -0.02
13 2.8751 0.00 0.02 0.00 -0.09
14 2.8751 0.00 -0.09 0.00 0.06
15 2.8751 0.00 0.06 0.00 0.05
16 2.8916 0.00 0.07 0.00 -0.05
17 3.0691 0.00 0.04 0.00 0.01
18 3.0691 0.00 0.03 0.00 -0.00
19 3.0691 0.00 0.01 0.00 -0.03
20 3.0716 0.00 0.03 0.00 0.01
21 3.0718 0.00 0.10 0.00 -0.09
22 3.0718 0.00 0.12 0.00 0.00
23 3.0745 0.00 -0.02 0.00 -0.03
24 3.0771 0.00 -0.02 0.00 -0.02
25 3.8799 0.00 -0.08 0.00 -0.06
26 3.8799 0.00 -0.09 0.00 -0.01
27 3.8799 0.00 0.06 0.00 0.15
28 3.9263 0.00 0.00 0.00 -0.09
29 3.9535 0.00 0.00 0.00 -0.03
30 4.9967 0.00 0.03 0.00 -0.02
31 4.9967 0.00 0.06 0.00 -0.07
32 4.9967 0.00 0.10 0.00 -0.07
33 5.0210 0.00 0.02 0.00 -0.08
34 7.0934 0.00 -0.19 0.00 0.30
35 7.0936 0.00 0.02 0.00 -0.04
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.
14VB41 quality flag:3 Type: SCATNEAR SCATNEAR SCATNEAR axisobj 53.936 53.936 53.936 ecceobj 0.322 0.322 0.322 incobj 17.686 17.686 17.686 qmin 35.210 35.246 35.234 qmax 72.508 72.461 72.471 amean 53.445 53.429 53.443 amin 52.851 52.861 52.869 amax 54.145 54.159 54.146 emean 0.323 0.322 0.323 emin 0.305 0.307 0.306 emax 0.340 0.338 0.339 imean 16.565 16.573 16.563 imin 15.890 15.890 15.883 imax 17.269 17.262 17.264 excite_mean 0.431 0.430 0.431 fracstop 1.000 1.000 1.000 cjmean 2.981 2.981 2.981 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 173.6 170.7 173.9 kozaiamp 179.9 180.0 180.0