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: 14TV115 # Created Sun Dec 22 02:10:05 2024 # Orbit generated from Bernstein formalism # Fitting 17 observations of 17 # Arc: 4.16y # First observation: 2014/10/03 # Last observation: 2018/11/30 Preliminary a, adot, b, bdot, g, gdot: 0.000289 0.028477 -0.000050 -0.007764 0.027795 0.000000 # Chi-squared of fit: 7.36 DOF: 28 RMS: 0.12 # Min/Max residuals: -0.29 0.22 # Exact a, adot, b, bdot, g, gdot: 1.686615E-05 2.864548E-02 -4.408249E-06 -7.804714E-03 2.760787E-02 4.497196E-04 # Covariance matrix: 4.4173E-13 -2.7673E-13 -3.9738E-14 6.6010E-14 2.0826E-13 -2.4753E-12 -2.7673E-13 5.1804E-13 6.3545E-14 -1.4847E-13 1.0000E-13 5.3038E-12 -3.9738E-14 6.3545E-14 2.7980E-13 -1.0980E-13 -2.3412E-14 7.6585E-13 6.6010E-14 -1.4847E-13 -1.0980E-13 9.0349E-14 -1.3012E-14 -1.6867E-12 2.0826E-13 1.0000E-13 -2.3412E-14 -1.3012E-14 6.4637E-13 1.6899E-13 -2.4753E-12 5.3038E-12 7.6585E-13 -1.6867E-12 1.6899E-13 6.0702E-11 # lat0 lon0 xBary yBary zBary JD0 -17.280696 20.123118 0.181976 -0.292810 -0.941781 2456933.759468 # Heliocentric elements and errors Epoch: 2456930.5000 = 2014/09/30 Mean Anomaly: 3.86205 +/- 0.153 Argument of Peri: 224.13195 +/- 0.184 Long of Asc Node: 153.35599 +/- 0.001 Inclination: 22.64394 +/- 0.000 Eccentricity: 0.08747873 +/- 0.0001 Semi-Major Axis: 40.71502768 +/- 0.0057 Time of Perihelion: 2455912.5039 +/- 40.3 Perihelion: 37.15332888 +/- 0.0070 Aphelion: 44.27672647 +/- 0.0078 Period (y) 259.8007 +/- 0.05 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 33.46116819 +/- 0.0009 Ecliptic Y 12.06940446 +/- 0.0003 Ecliptic Z -10.75991873 +/- 0.0003 Ecliptic XDOT -0.00115781 +/- 0.0000 Ecliptic YDOT 0.00259824 +/- 0.0000 Ecliptic ZDOT -0.00075219 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 37.16310202 +/- 0.0009 Geocenter to KBO 36.22155254 +/- 0.0011 # Hcoef: 7.52
The following table shows the complete astrometric record for 14TV115. 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 (14TV115) followed by the observatory code and reference code for the source of the astrometry.
2014 10 03.25869 01 40 18.680 -08 09 21.35 22.7i 14TV115 W84 C~55SO 2014 10 03.26006 01 40 18.689 -08 09 21.41 22.7z 14TV115 W84 C~55SO 2014 12 13.14801 01 35 11.485 -08 30 38.16 23.6g 14TV115 W84 C~55SO 2014 12 24.12101 01 34 50.972 -08 28 20.23 23.5r 14TV115 W84 C~55SO 2015 10 17.18378 01 46 00.049 -08 05 14.26 23.0i 14TV115 W84 C~55SO 2015 10 18.23630 01 45 54.704 -08 05 48.98 23.6g 14TV115 W84 C~55SO 2015 11 07.16992 01 44 14.983 -08 14 45.82 23.4z 14TV115 W84 C~55SO 2016 10 03.25557 01 53 52.565 -07 44 28.64 23.0g 14TV115 W84 C~55SO 2016 10 22.28291 01 52 18.379 -07 55 37.82 23.4i 14TV115 W84 C~55SO 2017 10 30.14413 01 58 26.673 -07 46 09.95 23.4i 14TV115 W84 C~55SO 2017 10 30.14550 01 58 26.662 -07 46 10.26 22.9z 14TV115 W84 C~55SO 2017 11 16.12483 01 57 03.580 -07 51 58.75 23.1r 14TV115 W84 C~55SO 2017 11 27.19433 01 56 15.484 -07 53 50.65 23.0i 14TV115 W84 C~55SO 2017 12 22.11777 01 54 58.176 -07 52 03.67 23.1r 14TV115 W84 C~55SO 2017 12 22.11915 01 54 58.180 -07 52 03.47 23.5g 14TV115 W84 C~55SO 2018 11 30.11232 02 02 48.862 -07 40 48.35 23.2r 14TV115 W84 C~55SO 2018 11 30.11375 02 02 48.859 -07 40 48.47 24.1g 14TV115 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 -0.09 0.00 -0.01
2 0.0000 0.10 0.12 -0.11 -0.11
3 0.1941 -4705.71 -0.11 530.36 0.16
4 0.2241 -4936.44 0.05 772.22 0.01
5 1.0374 4785.73 0.21 -1692.58 -0.13
6 1.0403 4699.06 -0.03 -1694.47 0.05
7 1.0949 3124.87 -0.00 -1628.19 0.14
8 2.0014 11760.90 -0.29 -3231.97 -0.17
9 2.0535 10207.03 0.03 -3311.06 0.02
10 3.0743 15497.94 0.12 -4905.41 0.05
11 3.0743 15497.67 -0.04 -4905.63 -0.18
12 3.1208 14217.29 0.08 -4747.47 0.22
13 3.1511 13511.46 0.11 -4573.45 0.02
14 3.2193 12488.45 -0.17 -4029.48 -0.15
15 3.2193 12488.58 -0.00 -4029.32 -0.02
16 4.1584 19242.89 0.01 -6133.05 0.11
17 4.1584 19242.81 0.01 -6133.15 -0.02
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.
14TV115 quality flag:3 Type: SCATEXTD SCATEXTD SCATEXTD axisobj 41.048 41.066 41.029 ecceobj 0.095 0.095 0.095 incobj 22.583 22.584 22.583 qmin 36.365 36.364 36.380 qmax 45.452 45.462 45.429 amean 40.787 40.804 40.768 amin 40.458 40.490 40.448 amax 41.125 41.152 41.123 emean 0.091 0.091 0.090 emin 0.077 0.078 0.075 emax 0.106 0.105 0.106 imean 21.754 21.754 21.760 imin 21.230 21.228 21.228 imax 22.390 22.369 22.408 excite_mean 0.382 0.382 0.381 fracstop 1.000 1.000 1.000 cjmean 2.892 2.892 2.892 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 180.1 180.6 179.5 kozaiamp 180.0 180.0 180.0