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: 14SB349 # Created Fri Nov 22 02:10:00 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 35 observations of 35 # Arc: 9.29y # First observation: 2014/09/24 # Last observation: 2024/01/09 # Chi-squared of fit: 30.03 DOF: 64 RMS: 0.16 # Min/Max residuals: -0.47 0.39 # Exact a, adot, b, bdot, g, gdot: 1.980511E-05 5.448055E-02 1.367098E-06 1.970249E-03 4.224217E-02 -8.110466E-03 # Covariance matrix: 1.9543E-13 -1.3937E-13 6.7751E-15 -6.2391E-15 -2.2200E-14 -2.2191E-13 -1.3937E-13 1.8847E-13 -8.0505E-15 6.3644E-15 1.3619E-13 2.8782E-13 6.7751E-15 -8.0505E-15 6.7947E-14 -1.2747E-14 -3.8310E-15 -1.3327E-14 -6.2391E-15 6.3644E-15 -1.2747E-14 5.7996E-15 1.4241E-15 1.1029E-14 -2.2200E-14 1.3619E-13 -3.8310E-15 1.4241E-15 2.3275E-13 1.7389E-13 -2.2191E-13 2.8782E-13 -1.3327E-14 1.1029E-14 1.7389E-13 4.6513E-13 # lat0 lon0 xBary yBary zBary JD0 -15.958077 35.266550 0.567942 -0.228032 -0.798015 2456924.791368 # Heliocentric elements and errors Epoch: 2456924.5000 = 2014/09/24 Mean Anomaly: 297.76377 +/- 0.006 Argument of Peri: 358.55861 +/- 0.008 Long of Asc Node: 117.27261 +/- 0.000 Inclination: 15.51895 +/- 0.000 Eccentricity: 0.17984213 +/- 0.0000 Semi-Major Axis: 25.91486019 +/- 0.0011 Time of Perihelion: 2465254.8359 +/- 2.6 Perihelion: 21.25427647 +/- 0.0010 Aphelion: 30.57544391 +/- 0.0013 Period (y) 131.9263 +/- 0.01 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 19.58645260 +/- 0.0002 Ecliptic Y 13.15884192 +/- 0.0002 Ecliptic Z -6.50851825 +/- 0.0001 Ecliptic XDOT -0.00242741 +/- 0.0000 Ecliptic YDOT 0.00260690 +/- 0.0000 Ecliptic ZDOT 0.00026741 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 24.47752294 +/- 0.0002 Geocenter to KBO 23.67313101 +/- 0.0003 # Hcoef: 9.41
The following table shows the complete astrometric record for 14SB349. 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 (14SB349) followed by the observatory code and reference code for the source of the astrometry.
2014 09 24.290590 02 32 58.19 -01 48 03.7 14SB349 W84 C~1bR3 2014 09 24.291991 02 32 58.18 -01 48 03.9 14SB349 W84 C~1bR3 2014 10 01.374641 02 32 16.87 -01 54 01.9 14SB349 W84 C~1bR3 2014 10 23.308565 02 29 43.85 -02 11 01.2 14SB349 W84 C~1bR3 2014 10 29.294468 02 28 58.20 -02 14 57.6 14SB349 W84 C~1bR3 2015 08 31.295440 02 46 11.70 -00 20 56.6 23.1z 14SB349 W84 C~1bR3 2015 09 19.327002 02 45 09.18 -00 35 56.9 24.3r 14SB349 W84 C~1bR3 2015 09 19.329363 02 45 09.18 -00 35 57.2 23.1i 14SB349 W84 C~1bR3 2015 09 26.227500 02 44 34.75 -00 41 39.1 23.8i 14SB349 W84 C~1bR3 2015 09 26.231285 02 44 34.75 -00 41 39.6 22.7z 14SB349 W84 C~1bR3 2015 10 09.208461 02 43 16.09 -00 52 13.7 22.9r 14SB349 W84 C~1bR3 2015 10 09.210810 02 43 16.09 -00 52 13.8 22.9i 14SB349 W84 C~1bR3 2015 10 16.294670 02 42 26.93 -00 57 42.8 23.8g 14SB349 W84 C~1bR3 2015 10 16.296875 02 42 26.93 -00 57 42.9 22.7r 14SB349 W84 C~1bR3 2015 10 16.299225 02 42 26.91 -00 57 43.0 23.0i 14SB349 W84 C~1bR3 2015 10 16.303032 02 42 26.89 -00 57 43.2 22.9z 14SB349 W84 C~1bR3 2015 10 20.211296 02 41 58.39 -01 00 36.0 22.8i 14SB349 W84 C~1bR3 2015 10 20.215104 02 41 58.37 -01 00 36.2 23.6z 14SB349 W84 C~1bR3 2016 01 15.23241 02 33 38.31 -01 08 50.5 24.0z 14SB349 T09 C~8Afo 2016 01 15.25231 02 33 38.27 -01 08 49.8 23.5z 14SB349 T09 C~8Afo 2016 01 15.29336 02 33 38.24 -01 08 48.3 24.3z 14SB349 T09 C~8Afo 2016 10 20.272743 02 53 54.17 +00 08 11.4 23.0i 14SB349 W84 C~2Azv 2016 10 20.279363 02 53 54.17 +00 08 11.4 22.7z 14SB349 W84 C~2Azv 2016 10 27.115301 02 53 02.55 +00 03 31.5 23.0r 14SB349 W84 C~2Azv 2016 11 10.109769 02 51 12.58 -00 04 30.4 22.8i 14SB349 W84 C~2Azv 2016 11 10.116400 02 51 12.55 -00 04 30.5 22.6z 14SB349 W84 C~2Azv 2016 12 17.173704 02 46 53.32 -00 11 52.0 22.8i 14SB349 W84 C~2Azv 2016 12 17.180336 02 46 53.31 -00 11 51.9 22.5z 14SB349 W84 C~2Azv 2016 12 24.046597 02 46 19.09 -00 10 37.9 22.8r 14SB349 W84 C~2Azv 2017 01 03.081250 02 45 40.52 -00 07 20.4 23.2r 14SB349 W84 C~2Azv 2017 01 03.083611 02 45 40.50 -00 07 20.1 22.9i 14SB349 W84 C~2Azv 2017 01 03.087593 02 45 40.48 -00 07 20.1 22.6z 14SB349 W84 C~2Azv 2024 01 09.150700 04 14 42.405 +08 16 30.34 23.0G 14SB349 G37 C~7gqt 2024 01 09.264930 04 14 41.727 +08 16 32.21 14SB349 G37 C~7gqt 2024 01 09.379110 04 14 41.060 +08 16 33.77 14SB349 G37 C~7gqt
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 0.16 0.00 -0.08
2 0.0000 0.00 0.12 0.00 -0.21
3 0.0194 0.00 0.39 0.00 -0.04
4 0.0794 0.00 -0.14 0.00 0.22
5 0.0958 0.00 -0.05 0.00 -0.29
6 0.9336 0.00 -0.10 0.00 0.14
7 0.9857 0.00 -0.26 0.00 0.14
8 0.9857 0.00 -0.09 0.00 -0.04
9 1.0046 0.00 -0.19 0.00 0.03
10 1.0046 0.00 0.13 0.00 -0.28
11 1.0402 0.00 -0.06 0.00 0.04
12 1.0402 0.00 0.18 0.00 0.05
13 1.0596 0.00 -0.19 0.00 0.03
14 1.0596 0.00 0.05 0.00 0.03
15 1.0596 0.00 0.01 0.00 0.04
16 1.0596 0.00 0.12 0.00 0.01
17 1.0703 0.00 -0.06 0.00 -0.00
18 1.0703 0.00 0.07 0.00 -0.04
19 1.3085 0.00 0.16 0.00 -0.14
20 1.3086 0.00 -0.15 0.00 -0.20
21 1.3087 0.00 0.01 0.00 -0.28
22 2.0725 0.00 -0.47 0.00 -0.16
23 2.0725 0.00 0.27 0.00 0.12
24 2.0912 0.00 0.20 0.00 -0.00
25 2.1296 0.00 -0.08 0.00 0.02
26 2.1296 0.00 0.27 0.00 0.12
27 2.2310 0.00 -0.16 0.00 0.13
28 2.2310 0.00 0.24 0.00 0.19
29 2.2498 0.00 0.01 0.00 0.24
30 2.2773 0.00 0.06 0.00 0.05
31 2.2773 0.00 -0.12 0.00 0.29
32 2.2773 0.00 -0.23 0.00 0.19
33 9.2919 0.00 0.00 0.00 -0.02
34 9.2922 0.00 -0.01 0.00 0.03
35 9.2925 0.00 0.04 0.00 -0.21
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.
14SB349 quality flag:3 Type: CENTAURR CENTAURR CENTAURR axisobj 26.041 26.040 26.041 ecceobj 0.177 0.177 0.177 incobj 15.521 15.521 15.521 qmin 21.322 18.116 21.322 qmax 30.741 30.987 30.742 amean 25.960 24.024 25.961 amin 25.664 22.961 25.664 amax 26.327 26.324 26.333 emean 0.167 0.205 0.167 emin 0.153 0.153 0.152 emax 0.177 0.250 0.177 imean 13.949 12.748 13.949 imin 13.839 11.510 13.835 imax 13.995 14.032 13.995 excite_mean 0.293 0.302 0.293 fracstop 0.002 0.028 0.002 cjmean 2.938 2.958 2.938 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 21.2 157.7 21.3 kozaiamp 178.2 178.2 178.2