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: 14VM43 # Created Tue Apr 1 01:10:13 2025 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 17 observations of 17 # Arc: 5.12y # First observation: 2013/10/13 # Last observation: 2018/11/27 # Chi-squared of fit: 10.27 DOF: 28 RMS: 0.14 # Min/Max residuals: -0.36 0.30 # Exact a, adot, b, bdot, g, gdot: 1.606017E-05 2.338355E-02 -3.856649E-06 -6.391770E-03 2.301118E-02 -1.264409E-02 # Covariance matrix: 5.8528E-13 -3.7283E-13 -6.9561E-14 7.9404E-14 -1.1054E-14 -2.2075E-12 -3.7283E-13 3.9217E-13 9.1053E-14 -1.0376E-13 -3.3677E-14 2.8945E-12 -6.9561E-14 9.1053E-14 3.9268E-13 -1.2211E-13 -1.3790E-14 7.3357E-13 7.9404E-14 -1.0376E-13 -1.2211E-13 6.1630E-14 1.3953E-14 -8.3515E-13 -1.1054E-14 -3.3677E-14 -1.3790E-14 1.3953E-14 4.8513E-13 -4.8820E-13 -2.2075E-12 2.8945E-12 7.3357E-13 -8.3515E-13 -4.8820E-13 2.3342E-11 # lat0 lon0 xBary yBary zBary JD0 -7.393355 2.034603 -0.301982 -0.122206 -0.942708 2456578.671578 # Heliocentric elements and errors Epoch: 2456578.5000 = 2013/10/13 Mean Anomaly: 349.08661 +/- 0.009 Argument of Peri: 274.47007 +/- 0.014 Long of Asc Node: 157.44470 +/- 0.001 Inclination: 16.72897 +/- 0.000 Eccentricity: 0.69646973 +/- 0.0002 Semi-Major Axis: 108.21557353 +/- 0.0607 Time of Perihelion: 2469043.4443 +/- 335.7 Perihelion: 32.84670233 +/- 0.0287 Aphelion: 183.58444473 +/- 0.1053 Period (y) 1125.7523 +/- 0.95 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 44.00739994 +/- 0.0013 Ecliptic Y 1.86869927 +/- 0.0001 Ecliptic Z -5.59229287 +/- 0.0002 Ecliptic XDOT -0.00169368 +/- 0.0000 Ecliptic YDOT 0.00272251 +/- 0.0000 Ecliptic ZDOT -0.00056044 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 44.40101587 +/- 0.0013 Geocenter to KBO 43.45755505 +/- 0.0013 # Hcoef: 7.09
The following table shows the complete astrometric record for 14VM43. 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 (14VM43) followed by the observatory code and reference code for the source of the astrometry.
2013 10 13.17080 00 19 15.680 -05 58 22.27 23.1i 14VM43 W84 C~52UT 2013 10 13.17363 00 19 15.671 -05 58 22.22 22.6z 14VM43 W84 C~52UT 2014 11 13.11961 00 23 04.638 -05 56 24.65 23.9r 14VM43 W84 C~52UT 2014 11 15.12231 00 22 59.319 -05 56 48.50 21.9i 14VM43 W84 C~52UT 2016 09 07.36013 00 38 52.799 -05 01 41.08 23.8r 14VM43 W84 C~52UT 2016 09 08.35816 00 38 49.055 -05 02 14.17 24.2g 14VM43 W84 C~52UT 2016 09 08.35952 00 38 49.078 -05 02 13.73 22.3i 14VM43 W84 C~52UT 2016 09 30.19372 00 37 20.486 -05 14 01.58 22.9i 14VM43 W84 C~52UT 2016 09 30.19509 00 37 20.492 -05 14 01.74 23.6r 14VM43 W84 C~52UT 2016 09 30.19645 00 37 20.468 -05 14 01.80 23.7g 14VM43 W84 C~52UT 2016 11 06.19531 00 34 54.042 -05 29 26.14 23.5i 14VM43 W84 C~52UT 2016 11 06.19669 00 34 54.047 -05 29 26.01 24.0g 14VM43 W84 C~52UT 2017 09 26.30306 00 43 39.422 -04 57 56.30 23.7i 14VM43 W84 C~52UT 2018 10 18.26309 00 48 16.514 -04 54 23.05 23.1z 14VM43 W84 C~52UT 2018 11 15.05695 00 46 32.102 -05 03 55.33 23.5i 14VM43 W84 C~52UT 2018 11 26.09090 00 46 02.067 -05 05 44.97 23.3r 14VM43 W84 C~52UT 2018 11 27.09163 00 45 59.765 -05 05 51.21 24.0g 14VM43 W84 C~52UT
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 0.05 0.00 -0.10
2 0.0000 0.00 0.08 0.00 0.02
3 1.0840 0.00 0.14 0.00 0.11
4 1.0895 0.00 -0.36 0.00 0.07
5 2.9026 0.00 0.07 0.00 -0.07
6 2.9054 0.00 -0.12 0.00 -0.31
7 2.9054 0.00 0.30 0.00 0.17
8 2.9652 0.00 0.00 0.00 0.09
9 2.9652 0.00 0.18 0.00 -0.03
10 2.9652 0.00 -0.09 0.00 -0.05
11 3.0665 0.00 -0.10 0.00 -0.04
12 3.0665 0.00 0.04 0.00 0.11
13 3.9538 0.00 -0.16 0.00 0.07
14 5.0133 0.00 -0.22 0.00 0.01
15 5.0894 0.00 0.12 0.00 0.01
16 5.1196 0.00 0.11 0.00 -0.01
17 5.1223 0.00 0.07 0.00 -0.00
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.
14VM43 quality flag:3 Type: SCATNEAR SCATNEAR SCATNEAR axisobj 109.692 109.690 109.695 ecceobj 0.699 0.699 0.699 incobj 16.678 16.678 16.678 qmin 31.871 31.997 32.006 qmax 191.241 204.427 190.747 amean 104.254 112.367 106.174 amin 97.128 105.342 102.467 amax 112.603 119.343 112.284 emean 0.679 0.698 0.683 emin 0.649 0.684 0.664 emax 0.704 0.713 0.705 imean 16.976 17.938 17.413 imin 15.287 15.664 15.658 imax 18.798 19.117 19.604 excite_mean 0.739 0.763 0.746 fracstop 1.000 1.000 1.000 cjmean 2.901 2.899 2.899 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 172.7 132.7 161.6 kozaiamp 180.0 180.0 180.0