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: 14TP115 # Created Sun Nov 24 02:10:01 2024 # Orbit generated from Bernstein formalism # Fitting 9 observations of 9 # Arc: 4.10y # First observation: 2014/10/01 # Last observation: 2018/11/07 Preliminary a, adot, b, bdot, g, gdot: 0.000156 0.029729 -0.000027 0.001594 0.026622 0.000000 # Chi-squared of fit: 4.04 DOF: 12 RMS: 0.12 # Min/Max residuals: -0.29 0.24 # Exact a, adot, b, bdot, g, gdot: 1.822763E-05 2.934922E-02 1.115548E-06 1.574919E-03 2.601296E-02 -3.681039E-03 # Covariance matrix: 9.0013E-13 1.1430E-13 -2.8409E-14 1.6060E-14 1.0009E-12 2.5849E-12 1.1430E-13 9.3279E-13 -4.3654E-14 5.5311E-14 1.1111E-12 8.2629E-12 -2.8409E-14 -4.3654E-14 4.0865E-13 -1.3201E-13 -8.2147E-14 -4.2700E-13 1.6060E-14 5.5311E-14 -1.3201E-13 7.1839E-14 7.1869E-14 5.2896E-13 1.0009E-12 1.1111E-12 -8.2147E-14 7.1869E-14 2.5399E-12 1.1036E-11 2.5849E-12 8.2629E-12 -4.2700E-13 5.2896E-13 1.1036E-11 7.9134E-11 # lat0 lon0 xBary yBary zBary JD0 -11.477530 20.914145 0.228069 -0.194288 -0.957728 2456931.831808 # Heliocentric elements and errors Epoch: 2456930.5000 = 2014/09/30 Mean Anomaly: 343.92140 +/- 0.026 Argument of Peri: 316.92614 +/- 0.054 Long of Asc Node: 95.34107 +/- 0.002 Inclination: 11.59222 +/- 0.000 Eccentricity: 0.31839366 +/- 0.0003 Semi-Major Axis: 55.68466448 +/- 0.0232 Time of Perihelion: 2463709.2200 +/- 10.3 Perihelion: 37.95502038 +/- 0.0241 Aphelion: 73.41430858 +/- 0.0356 Period (y) 415.5388 +/- 0.26 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 36.18313902 +/- 0.0022 Ecliptic Y 13.58607345 +/- 0.0008 Ecliptic Z -7.64940319 +/- 0.0005 Ecliptic XDOT -0.00143113 +/- 0.0000 Ecliptic YDOT 0.00275708 +/- 0.0000 Ecliptic ZDOT 0.00023965 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 39.39942018 +/- 0.0020 Geocenter to KBO 38.44237752 +/- 0.0024 # Hcoef: 8.13
The following table shows the complete astrometric record for 14TP115. 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 (14TP115) followed by the observatory code and reference code for the source of the astrometry.
2014 10 01.33103 01 34 26.140 -02 29 16.65 23.7r 14TP115 W84 C~55SO 2014 11 16.06575 01 30 57.276 -02 46 44.16 24.0r 14TP115 W84 C~55SO 2014 11 17.16106 01 30 52.878 -02 46 57.21 23.9r 14TP115 W84 C~55SO 2015 11 07.12743 01 37 42.878 -02 01 56.08 23.9r 14TP115 W84 C~55SO 2016 11 25.08231 01 42 33.466 -01 23 13.59 24.0r 14TP115 W84 C~55SO 2016 11 25.08369 01 42 33.490 -01 23 13.27 24.2i 14TP115 W84 C~55SO 2017 11 18.18692 01 49 11.834 -00 38 49.80 24.7g 14TP115 W84 C~55SO 2018 09 09.26961 02 00 32.823 +00 34 11.91 24.0r 14TP115 W84 C~55SO 2018 11 07.22249 01 56 15.489 +00 07 47.72 23.9r 14TP115 W84 C~55SO
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 -0.08 0.00 -0.03
2 0.1252 -3295.08 0.11 190.50 -0.06
3 0.1282 -3361.12 -0.02 202.85 0.07
4 1.1001 3347.82 -0.02 425.24 -0.09
5 2.1513 8260.57 -0.29 956.77 0.04
6 2.1513 8261.03 0.24 956.93 0.18
7 3.1317 14818.74 0.12 1198.89 -0.08
8 3.9396 26042.74 0.06 1450.68 -0.02
9 4.1010 21814.05 -0.12 1421.97 -0.01
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.
14TP115 quality flag:2 Type: SCATNEAR SCATNEAR 5:2EEE axisobj 56.351 56.411 56.290 ecceobj 0.325 0.326 0.324 incobj 11.597 11.597 11.596 qmin 36.397 36.927 37.300 qmax 76.140 75.552 75.195 amean 55.577 55.786 55.463 amin 54.556 55.104 54.619 amax 56.543 56.581 56.518 emean 0.326 0.321 0.313 emin 0.306 0.307 0.297 emax 0.347 0.337 0.330 imean 10.028 10.039 10.071 imin 9.254 9.362 9.693 imax 10.874 10.563 10.568 excite_mean 0.369 0.366 0.359 fracstop 1.000 1.000 1.000 cjmean 3.072 3.078 3.081 libcent 0 -180.0 -180.0 181.0 libamp 0 -180.0 -180.0 169.3 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 183.5 173.1 182.1 kozaiamp 180.0 180.0 180.0