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: 14RJ70 # Created Tue May 7 01:15:30 2024 # Orbit generated from Bernstein formalism # Fitting 36 observations of 36 # Arc: 4.16y # First observation: 2014/09/12 # Last observation: 2018/11/08 Preliminary a, adot, b, bdot, g, gdot: 0.000127 0.029503 -0.000049 0.000444 0.026997 0.000000 # Chi-squared of fit: 19.60 DOF: 66 RMS: 0.13 # Min/Max residuals: -0.38 0.38 # Exact a, adot, b, bdot, g, gdot: 1.742192E-05 2.972166E-02 5.379117E-07 4.666841E-04 2.674625E-02 -7.288611E-04 # Covariance matrix: 1.2506E-13 -6.3204E-14 -2.4274E-14 -1.1491E-14 2.6642E-13 -4.7575E-13 -6.3204E-14 2.2697E-13 -1.2617E-14 1.4144E-14 8.5745E-14 2.2325E-12 -2.4274E-14 -1.2617E-14 1.0411E-13 -2.4267E-14 -2.1130E-13 -5.0688E-14 -1.1491E-14 1.4144E-14 -2.4267E-14 2.4634E-14 -6.6339E-14 1.8375E-13 2.6642E-13 8.5745E-14 -2.1130E-13 -6.6339E-14 2.2309E-12 1.1718E-14 -4.7575E-13 2.2325E-12 -5.0688E-14 1.8375E-13 1.1718E-14 2.4616E-11 # lat0 lon0 xBary yBary zBary JD0 -26.923765 -57.071070 -0.726417 -0.317065 -0.624611 2456912.561418 # Heliocentric elements and errors Epoch: 2456910.5000 = 2014/09/10 Mean Anomaly: 358.75330 +/- 0.042 Argument of Peri: 274.78714 +/- 0.062 Long of Asc Node: 30.85475 +/- 0.001 Inclination: 26.47996 +/- 0.000 Eccentricity: 0.18531615 +/- 0.0002 Semi-Major Axis: 46.66346914 +/- 0.0137 Time of Perihelion: 2457313.7036 +/- 13.5 Perihelion: 38.01597461 +/- 0.0144 Aphelion: 55.31096368 +/- 0.0186 Period (y) 318.7673 +/- 0.14 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 19.11001607 +/- 0.0010 Ecliptic Y -28.17164008 +/- 0.0016 Ecliptic Z -16.92963101 +/- 0.0009 Ecliptic XDOT 0.00252451 +/- 0.0000 Ecliptic YDOT 0.00168705 +/- 0.0000 Ecliptic ZDOT 0.00007649 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 38.01902715 +/- 0.0013 Geocenter to KBO 37.38841689 +/- 0.0021 # Hcoef: 7.04
The following table shows the complete astrometric record for 14RJ70. 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 (14RJ70) followed by the observatory code and reference code for the source of the astrometry.
2014 09 12.06064 20 54 57.305 -45 29 22.80 22.5i 14RJ70 W84 C~4yUF 2014 09 12.06064 20 54 57.31 -45 29 22.8 22.4i 14RJ70 W84 C~3cnV 2014 09 12.06203 20 54 57.284 -45 29 22.89 24.2g 14RJ70 W84 C~4yUF 2014 09 12.06203 20 54 57.28 -45 29 22.9 24.3g 14RJ70 W84 C~3cnV 2014 09 12.06341 20 54 57.281 -45 29 22.68 23.0r 14RJ70 W84 C~4yUF 2014 09 12.06341 20 54 57.28 -45 29 22.7 23.0r 14RJ70 W84 C~3cnV 2014 09 24.04327 20 54 01.951 -45 25 20.63 23.6g 14RJ70 W84 C~4yUF 2014 09 24.04327 20 54 01.95 -45 25 20.7 23.7g 14RJ70 W84 C~3cnV 2014 09 26.005984 20 53 54.41 -45 24 29.7 22.6i 14RJ70 W84 C~352Q 2014 09 27.042049 20 53 50.59 -45 24 01.7 23.0r 14RJ70 W84 C~352Q 2014 09 27.04258 20 53 50.594 -45 24 01.97 23.4r 14RJ70 W84 C~4yUF 2014 10 13.03244 20 53 09.296 -45 15 13.74 23.0r 14RJ70 W84 C~4yUF 2014 10 13.03244 20 53 09.30 -45 15 13.7 23.0r 14RJ70 W84 C~3cnV 2014 10 22.03422 20 53 01.373 -45 09 05.22 21.6z 14RJ70 W84 C~4yUF 2014 10 22.03422 20 53 01.39 -45 09 05.2 22.4z 14RJ70 W84 C~3cnV 2014 10 23.047546 20 53 01.25 -45 08 20.8 22.1z 14RJ70 W84 C~352Q 2014 10 23.04807 20 53 01.248 -45 08 20.83 22.1z 14RJ70 W84 C~4yUF 2016 09 23.01421 21 12 00.554 -44 14 51.55 22.7r 14RJ70 W84 C~4yUF 2016 09 23.01421 21 12 00.55 -44 14 51.5 22.8r 14RJ70 W84 C~3cnV 2016 09 23.01557 21 12 00.538 -44 14 51.43 23.6g 14RJ70 W84 C~4yUF 2016 09 23.01557 21 12 00.54 -44 14 51.4 23.7g 14RJ70 W84 C~3cnV 2016 10 02.05056 21 11 25.001 -44 11 10.80 22.7r 14RJ70 W84 C~4yUF 2016 10 02.05056 21 11 25.00 -44 11 10.8 22.9r 14RJ70 W84 C~3cnV 2016 10 02.05193 21 11 24.993 -44 11 10.80 22.6i 14RJ70 W84 C~4yUF 2016 10 02.05193 21 11 24.99 -44 11 10.8 22.7i 14RJ70 W84 C~3cnV 2016 10 02.05332 21 11 24.993 -44 11 10.78 23.5g 14RJ70 W84 C~4yUF 2016 10 02.05332 21 11 24.99 -44 11 10.8 23.7g 14RJ70 W84 C~3cnV 2017 09 08.10623 21 22 02.969 -43 38 36.54 22.2z 14RJ70 W84 C~4yUF 2017 09 28.04775 21 20 22.120 -43 33 54.84 22.7z 14RJ70 W84 C~4yUF 2017 10 10.09138 21 19 40.983 -43 28 22.75 23.8g 14RJ70 W84 C~4yUF 2017 10 13.063565 21 19 33.57 -43 26 44.1 22.4i 14RJ70 W84 C~352Q 2017 10 13.064942 21 19 33.55 -43 26 43.8 22.9g 14RJ70 W84 C~352Q 2017 10 13.06547 21 19 33.584 -43 26 43.83 22.6g 14RJ70 W84 C~4yUF 2017 10 22.01417 21 19 18.060 -43 21 08.67 22.8z 14RJ70 W84 C~4yUF 2018 10 28.12336 21 27 37.278 -42 36 14.01 22.5i 14RJ70 W84 C~4yUF 2018 11 08.11080 21 27 38.639 -42 27 50.70 24.3g 14RJ70 W84 C~4yUF
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 0.03 0.00 -0.05
2 0.0000 0.05 0.08 -0.02 -0.07
3 0.0000 -0.28 -0.18 -0.01 -0.11
4 0.0000 -0.24 -0.14 -0.02 -0.12
5 0.0000 -0.20 -0.04 0.19 0.05
6 0.0000 -0.22 -0.05 0.18 0.03
7 0.0328 -479.92 0.05 409.32 -0.01
8 0.0328 -479.95 0.01 409.26 -0.08
9 0.0382 -539.97 0.22 482.08 0.20
10 0.0410 -569.73 0.11 521.02 0.31
11 0.0410 -569.77 0.09 520.75 0.02
12 0.0848 -823.97 -0.03 1156.46 -0.03
13 0.0848 -824.02 -0.08 1156.43 -0.05
14 0.1094 -792.01 -0.08 1532.99 -0.09
15 0.1094 -792.19 -0.26 1533.02 -0.06
16 0.1122 -779.98 0.19 1575.75 -0.04
17 0.1122 -780.01 0.16 1575.73 -0.08
18 2.0314 11757.20 -0.01 588.42 0.01
19 2.0314 11757.23 0.02 588.35 -0.05
20 2.0314 11757.14 -0.02 588.55 0.09
21 2.0314 11757.11 -0.05 588.53 0.07
22 2.0561 11478.18 -0.06 931.56 0.08
23 2.0561 11478.19 -0.05 931.55 0.07
24 2.0561 11478.08 -0.12 931.59 0.06
25 2.0561 11478.11 -0.09 931.58 0.05
26 2.0561 11478.08 -0.09 931.59 0.01
27 2.0561 11478.11 -0.05 931.60 0.01
28 2.9899 18642.85 0.38 184.93 -0.04
29 3.0445 17732.55 0.06 868.08 -0.04
30 3.0774 17443.10 -0.19 1347.11 0.27
31 3.0856 17405.60 0.09 1469.43 -0.19
32 3.0856 17405.51 0.01 1469.79 0.12
33 3.0856 17405.85 0.35 1469.62 -0.07
34 3.1101 17376.09 -0.02 1845.23 -0.17
35 4.1261 23532.22 0.14 2195.95 0.02
36 4.1562 23751.05 -0.38 2654.15 -0.12
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.
14RJ70 quality flag:3 Type: SCATEXTD SCATEXTD SCATEXTD axisobj 46.806 46.847 46.765 ecceobj 0.189 0.189 0.188 incobj 26.505 26.506 26.505 qmin 37.531 37.498 37.523 qmax 56.731 56.886 56.705 amean 46.922 46.963 46.881 amin 46.528 46.550 46.487 amax 47.381 47.441 47.352 emean 0.182 0.182 0.181 emin 0.167 0.167 0.167 emax 0.197 0.199 0.198 imean 26.161 26.163 26.159 imin 25.782 25.772 25.778 imax 26.529 26.530 26.532 excite_mean 0.477 0.477 0.477 fracstop 1.000 1.000 1.000 cjmean 2.846 2.846 2.846 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 184.9 184.9 184.9 kozaiamp 180.0 180.0 180.0