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: 14TL95 # Created Sun Dec 22 02:10:05 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 32 observations of 32 # Arc: 10.27y # First observation: 2014/08/18 # Last observation: 2024/11/24 # Chi-squared of fit: 7.22 DOF: 58 RMS: 0.08 # Min/Max residuals: -0.22 0.25 # Exact a, adot, b, bdot, g, gdot: 1.815699E-05 3.221773E-02 6.423889E-07 1.613386E-03 2.830990E-02 -1.210000E-03 # Covariance matrix: 2.3409E-13 -6.9016E-14 7.7941E-15 -2.7659E-15 1.1087E-13 -1.9630E-13 -6.9016E-14 5.5949E-14 -2.7681E-15 2.4755E-15 -3.5356E-15 1.6899E-13 7.7941E-15 -2.7681E-15 7.4706E-14 -1.4454E-14 5.2959E-15 -9.9101E-15 -2.7659E-15 2.4755E-15 -1.4454E-14 7.0229E-15 -1.8410E-16 8.5289E-15 1.1087E-13 -3.5356E-15 5.2959E-15 -1.8410E-16 1.1602E-13 -2.0664E-14 -1.9630E-13 1.6899E-13 -9.9101E-15 8.5289E-15 -2.0664E-14 5.8283E-13 # lat0 lon0 xBary yBary zBary JD0 -10.412849 26.749777 0.892855 -0.087110 -0.474745 2456887.862138 # Heliocentric elements and errors Epoch: 2456888.5000 = 2014/08/19 Mean Anomaly: 344.11961 +/- 0.007 Argument of Peri: 307.56796 +/- 0.011 Long of Asc Node: 101.00997 +/- 0.001 Inclination: 10.59110 +/- 0.000 Eccentricity: 0.18913008 +/- 0.0000 Semi-Major Axis: 43.57690464 +/- 0.0029 Time of Perihelion: 2461523.4151 +/- 10.3 Perihelion: 35.33520130 +/- 0.0029 Aphelion: 51.81860798 +/- 0.0039 Period (y) 287.6688 +/- 0.03 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 31.85393460 +/- 0.0004 Ecliptic Y 15.05904174 +/- 0.0002 Ecliptic Z -6.38431466 +/- 0.0001 Ecliptic XDOT -0.00148488 +/- 0.0000 Ecliptic YDOT 0.00273894 +/- 0.0000 Ecliptic ZDOT 0.00017473 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 35.80796386 +/- 0.0003 Geocenter to KBO 35.32338616 +/- 0.0004 # Hcoef: 7.70
The following table shows the complete astrometric record for 14TL95. 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 (14TL95) followed by the observatory code and reference code for the source of the astrometry.
2014 08 18.36136 01 54 14.300 +00 35 17.03 24.5i 14TL95 W84 C~4yUi 2014 10 01.33657 01 51 46.721 +00 13 05.93 23.0r 14TL95 W84 C~4yUi 2014 10 01.33794 01 51 46.706 +00 13 05.78 22.9i 14TL95 W84 C~4yUi 2014 10 02.28380 01 51 42.166 +00 12 35.14 22.6i 14TL95 W84 C~4yUj 2014 10 03.279699 01 51 37.33 +00 12 02.8 23.2r 14TL95 W84 C~352R 2014 10 03.28022 01 51 37.328 +00 12 02.79 23.1r 14TL95 W84 C~4yUj 2014 10 03.32907 01 51 37.093 +00 12 01.35 23.0r 14TL95 W84 C~4yUj 2014 10 23.27656 01 49 54.755 +00 01 55.04 23.4r 14TL95 W84 C~4yUj 2014 10 23.27793 01 49 54.738 +00 01 55.14 23.1i 14TL95 W84 C~4yUj 2014 12 12.055451 01 46 14.16 -00 10 34.5 23.5r 14TL95 W84 C~352R 2014 12 12.05597 01 46 14.161 -00 10 34.54 23.7r 14TL95 W84 C~4yUj 2015 01 15.045718 01 45 34.36 -00 03 33.6 22.3z 14TL95 W84 C~352R 2015 01 15.04625 01 45 34.370 -00 03 33.64 22.7z 14TL95 W84 C~4yUj 2015 09 04.32065 02 00 25.108 +01 12 25.09 22.5z 14TL95 W84 C~4yUj 2015 12 29.13369 01 52 23.410 +00 35 31.66 23.4i 14TL95 W84 C~4yUj 2015 12 29.13643 01 52 23.413 +00 35 31.60 23.0z 14TL95 W84 C~4yUj 2016 08 26.34885 02 07 35.037 +02 00 55.43 23.7r 14TL95 W84 C~4yUj 2016 09 10.29943 02 06 54.906 +01 53 59.01 24.6g 14TL95 W84 C~4yUj 2016 11 18.11643 02 01 24.704 +01 22 20.28 23.0r 14TL95 W84 C~4yUj 2016 11 18.11780 02 01 24.705 +01 22 20.16 22.8i 14TL95 W84 C~4yUj 2016 11 28.10726 02 00 39.698 +01 20 06.61 23.3r 14TL95 W84 C~4yUj 2016 11 28.108113 02 00 39.68 +01 20 06.6 23.0i 14TL95 W84 C~352R 2016 11 28.10864 02 00 39.690 +01 20 06.32 22.9i 14TL95 W84 C~4yUj 2016 11 30.14518 02 00 31.250 +01 19 46.67 22.9z 14TL95 W84 C~4yUj 2017 08 27.408981 02 14 23.77 +02 45 16.0 22.9i 14TL95 W84 C~352R 2017 08 27.40951 02 14 23.767 +02 45 15.97 23.0i 14TL95 W84 C~4yUj 2017 09 18.334687 02 13 20.06 +02 35 03.9 23.4r 14TL95 W84 C~352R 2017 09 18.33522 02 13 20.062 +02 35 03.87 23.2r 14TL95 W84 C~4yUj 2017 11 01.16510 02 09 46.833 +02 13 32.76 22.0z 14TL95 W84 C~4yUj 2018 09 09.28945 02 20 45.852 +03 24 30.25 22.9z 14TL95 W84 C~4yUj 2024 11 24.243450 02 57 01.128 +07 20 23.73 23.1G 14TL95 G37 C~8SSe 2024 11 24.299750 02 57 00.824 +07 20 22.94 14TL95 G37 C~8SSe
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 0.04
2 0.1204 0.00 0.05 0.00 0.12
3 0.1204 0.00 -0.07 0.00 0.01
4 0.1230 0.00 0.01 0.00 0.02
5 0.1257 0.00 -0.10 0.00 -0.15
6 0.1257 0.00 -0.09 0.00 -0.14
7 0.1259 0.00 0.02 0.00 -0.00
8 0.1805 0.00 0.11 0.00 -0.13
9 0.1805 0.00 -0.03 0.00 0.01
10 0.3168 0.00 0.03 0.00 0.06
11 0.3168 0.00 0.06 0.00 0.02
12 0.4098 0.00 -0.00 0.00 0.01
13 0.4098 0.00 0.14 0.00 -0.05
14 1.0457 0.00 0.07 0.00 0.05
15 1.3628 0.00 -0.03 0.00 0.15
16 1.3628 0.00 0.07 0.00 0.06
17 2.0232 0.00 -0.06 0.00 -0.18
18 2.0642 0.00 0.25 0.00 0.05
19 2.2526 0.00 -0.11 0.00 0.12
20 2.2526 0.00 0.00 0.00 0.03
21 2.2799 0.00 -0.00 0.00 0.11
22 2.2799 0.00 -0.22 0.00 0.11
23 2.2799 0.00 -0.03 0.00 -0.17
24 2.2855 0.00 -0.01 0.00 -0.06
25 3.0255 0.00 0.04 0.00 0.06
26 3.0255 0.00 0.01 0.00 0.04
27 3.0855 0.00 -0.05 0.00 -0.01
28 3.0855 0.00 0.02 0.00 -0.02
29 3.2055 0.00 0.08 0.00 -0.02
30 4.0600 0.00 0.06 0.00 -0.01
31 10.2694 0.00 0.00 0.00 -0.08
32 10.2695 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.
14TL95 quality flag:3 Type: 7:4EEE 7:4EEE 7:4EEE axisobj 43.967 43.967 43.967 ecceobj 0.195 0.195 0.195 incobj 10.595 10.595 10.595 qmin 34.474 34.425 34.321 qmax 53.606 53.767 53.706 amean 43.727 43.727 43.726 amin 43.259 43.249 43.250 amax 44.266 44.282 44.279 emean 0.192 0.191 0.191 emin 0.167 0.167 0.165 emax 0.212 0.214 0.215 imean 8.599 8.714 8.629 imin 7.385 7.434 7.357 imax 10.012 9.983 10.063 excite_mean 0.244 0.244 0.243 fracstop 1.000 1.000 1.000 cjmean 3.027 3.027 3.027 libcent 0 181.1 179.9 180.8 libamp 0 120.0 123.2 118.8 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 184.8 178.9 184.7 kozaiamp 180.0 180.0 180.0