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: 14TY114 # Created Fri Nov 22 02:10:04 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 13 observations of 13 # Arc: 5.08y # First observation: 2013/09/10 # Last observation: 2018/10/10 # Chi-squared of fit: 6.38 DOF: 20 RMS: 0.12 # Min/Max residuals: -0.26 0.18 # Exact a, adot, b, bdot, g, gdot: 1.456540E-05 2.043092E-02 4.048055E-06 5.258104E-03 2.275103E-02 7.791416E-06 # Covariance matrix: 8.4201E-13 -4.5544E-13 6.9357E-14 -8.5105E-14 8.5524E-14 -3.2222E-12 -4.5544E-13 6.7073E-13 -1.5718E-13 1.7642E-13 5.1255E-13 6.5790E-12 6.9357E-14 -1.5718E-13 4.8051E-13 -1.8077E-13 -1.4977E-13 -1.6931E-12 -8.5105E-14 1.7642E-13 -1.8077E-13 1.0688E-13 1.5725E-13 1.8941E-12 8.5524E-14 5.1255E-13 -1.4977E-13 1.5725E-13 9.5467E-13 5.7914E-12 -3.2222E-12 6.5790E-12 -1.6931E-12 1.8941E-12 5.7914E-12 7.0592E-11 # lat0 lon0 xBary yBary zBary JD0 -9.577934 11.058932 0.403661 -0.153547 -0.910554 2456545.819698 # Heliocentric elements and errors Epoch: 2456546.5000 = 2013/09/11 Mean Anomaly: 203.90641 +/- 0.838 Argument of Peri: 123.49565 +/- 0.835 Long of Asc Node: 43.08388 +/- 0.001 Inclination: 17.07263 +/- 0.001 Eccentricity: 0.02491903 +/- 0.0002 Semi-Major Axis: 43.86322425 +/- 0.0057 Time of Perihelion: 2502554.3367 +/- 247.1 Perihelion: 42.77019529 +/- 0.0092 Aphelion: 44.95625320 +/- 0.0094 Period (y) 290.5086 +/- 0.06 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 43.51980874 +/- 0.0018 Ecliptic Y 8.09773865 +/- 0.0004 Ecliptic Z -7.31331686 +/- 0.0003 Ecliptic XDOT -0.00037356 +/- 0.0000 Ecliptic YDOT 0.00243221 +/- 0.0000 Ecliptic ZDOT 0.00062392 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 44.86682847 +/- 0.0018 Geocenter to KBO 43.95407826 +/- 0.0019 # Hcoef: 7.32
The following table shows the complete astrometric record for 14TY114. 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 (14TY114) followed by the observatory code and reference code for the source of the astrometry.
2013 09 10.31892 00 55 39.063 -04 26 25.33 24.3g 14TY114 W84 C~52UG 2014 10 02.30648 00 58 00.683 -03 51 38.33 23.6r 14TY114 W84 C~52UG 2014 11 15.02123 00 55 03.271 -04 04 37.87 23.2i 14TY114 W84 C~52UG 2014 11 15.09217 00 55 03.038 -04 04 38.58 24.3r 14TY114 W84 C~52UG 2014 11 17.16405 00 54 56.297 -04 04 54.77 24.2r 14TY114 W84 C~52UG 2015 09 04.28801 01 03 42.864 -02 55 20.59 23.6i 14TY114 W84 C~52UG 2015 12 05.05359 00 57 57.837 -03 21 57.61 23.7r 14TY114 W84 C~52UG 2016 10 23.16797 01 04 08.639 -02 31 06.41 24.5r 14TY114 W84 C~52UG 2016 11 05.21322 01 03 15.531 -02 34 48.08 24.3r 14TY114 W84 C~52UG 2016 11 06.12744 01 03 12.030 -02 35 00.76 22.2z 14TY114 W84 C~52UG 2017 08 28.29502 01 11 41.229 -01 24 25.81 24.1r 14TY114 W84 C~52UG 2017 09 14.31127 01 10 43.557 -01 31 18.99 23.2z 14TY114 W84 C~52UG 2018 10 10.27884 01 12 46.385 -00 57 33.56 23.6i 14TY114 W84 C~52UG
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 -0.04 0.00 -0.10
2 1.0595 0.00 -0.04 0.00 -0.05
3 1.1792 0.00 -0.06 0.00 0.18
4 1.1794 0.00 0.04 0.00 0.06
5 1.1851 0.00 0.12 0.00 0.15
6 1.9821 0.00 0.10 0.00 -0.06
7 2.2334 0.00 -0.11 0.00 -0.19
8 3.1180 0.00 -0.26 0.00 -0.17
9 3.1537 0.00 0.15 0.00 -0.09
10 3.1562 0.00 0.18 0.00 0.12
11 3.9643 0.00 -0.05 0.00 0.12
12 4.0109 0.00 0.08 0.00 0.16
13 5.0813 0.00 -0.03 0.00 -0.09
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.
14TY114 quality flag:3 Type: SCATEXTD SCATEXTD SCATEXTD axisobj 44.098 44.098 44.098 ecceobj 0.019 0.019 0.019 incobj 17.050 17.050 17.050 qmin 42.058 42.058 42.059 qmax 45.860 45.860 45.859 amean 43.872 43.872 43.872 amin 43.536 43.537 43.536 amax 44.215 44.215 44.215 emean 0.026 0.026 0.026 emin 0.016 0.016 0.016 emax 0.037 0.037 0.037 imean 16.143 16.143 16.143 imin 15.783 15.783 15.783 imax 16.529 16.529 16.529 excite_mean 0.279 0.279 0.279 fracstop 1.000 1.000 1.000 cjmean 3.005 3.005 3.005 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 180.6 180.6 180.6 kozaiamp 180.0 180.0 180.0