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: 14RX86 # Created Thu Apr 25 01:16:08 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 20 observations of 20 # Arc: 8.15y # First observation: 2014/09/04 # Last observation: 2022/10/29 # Chi-squared of fit: 21.06 DOF: 34 RMS: 0.18 # Min/Max residuals: -0.44 0.55 # Exact a, adot, b, bdot, g, gdot: 1.687127E-05 2.924407E-02 -4.326607E-06 -6.878387E-03 2.705649E-02 1.002634E-04 # Covariance matrix: 4.3458E-13 -1.0047E-13 -1.6480E-15 1.9907E-14 2.2679E-13 -2.9697E-13 -1.0047E-13 1.0055E-13 2.9010E-14 -2.3633E-14 4.8013E-14 3.9724E-13 -1.6480E-15 2.9010E-14 1.8003E-13 -4.3993E-14 4.0072E-14 1.3330E-13 1.9907E-14 -2.3633E-14 -4.3993E-14 2.0683E-14 -1.0330E-14 -1.0873E-13 2.2679E-13 4.8013E-14 4.0072E-14 -1.0330E-14 3.4220E-13 2.1889E-13 -2.9697E-13 3.9724E-13 1.3330E-13 -1.0873E-13 2.1889E-13 1.8274E-12 # lat0 lon0 xBary yBary zBary JD0 -23.357766 33.842734 0.800439 -0.244833 -0.567295 2456904.850808 # Heliocentric elements and errors Epoch: 2456904.5000 = 2014/09/04 Mean Anomaly: 354.37765 +/- 0.012 Argument of Peri: 248.72330 +/- 0.018 Long of Asc Node: 154.70571 +/- 0.000 Inclination: 26.61275 +/- 0.000 Eccentricity: 0.17312370 +/- 0.0001 Semi-Major Axis: 45.32730002 +/- 0.0049 Time of Perihelion: 2458645.3179 +/- 18.3 Perihelion: 37.48007017 +/- 0.0052 Aphelion: 53.17452986 +/- 0.0067 Period (y) 305.1743 +/- 0.05 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 29.13808995 +/- 0.0006 Ecliptic Y 18.57775415 +/- 0.0004 Ecliptic Z -14.65363568 +/- 0.0003 Ecliptic XDOT -0.00187428 +/- 0.0000 Ecliptic YDOT 0.00230491 +/- 0.0000 Ecliptic ZDOT -0.00064289 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 37.53520058 +/- 0.0005 Geocenter to KBO 36.95974409 +/- 0.0008 # Hcoef: 7.63
The following table shows the complete astrometric record for 14RX86. 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 (14RX86) followed by the observatory code and reference code for the source of the astrometry.
2014 09 04.35003 02 37 41.020 -09 13 44.65 23.3r 14RX86 W84 C~52Tx 2014 09 25.28565 02 36 41.076 -09 29 41.03 22.5i 14RX86 W84 C~52Tx 2014 10 28.27574 02 34 11.108 -09 50 40.81 23.3r 14RX86 W84 C~52Tx 2014 10 28.31554 02 34 10.890 -09 50 42.17 23.1i 14RX86 W84 C~52Tx 2014 11 21.24784 02 32 10.233 -09 58 57.64 23.4r 14RX86 W84 C~52Tx 2015 12 05.21464 02 38 06.693 -09 49 07.91 23.1i 14RX86 W84 C~52Tx 2015 12 05.21601 02 38 06.680 -09 49 07.65 23.7r 14RX86 W84 C~52Tx 2016 10 23.24033 02 48 34.192 -09 25 03.30 23.3r 14RX86 W84 C~52Tx 2016 10 28.21465 02 48 09.173 -09 27 40.90 23.0i 14RX86 W84 C~52Tx 2016 12 30.05631 02 43 35.424 -09 33 04.39 23.8z 14RX86 W84 C~52Tx 2017 08 25.40761 02 58 35.326 -08 30 33.26 23.0i 14RX86 W84 C~52Tx 2017 09 14.35913 02 58 05.193 -08 45 34.71 22.8z 14RX86 W84 C~52Tx 2017 10 21.24374 02 55 44.394 -09 11 22.40 23.0i 14RX86 W84 C~52Tx 2017 10 21.24511 02 55 44.395 -09 11 22.39 23.5r 14RX86 W84 C~52Tx 2017 11 22.16316 02 53 01.837 -09 24 08.92 23.4r 14RX86 W84 C~52Tx 2017 11 22.16453 02 53 01.834 -09 24 08.65 24.0g 14RX86 W84 C~52Tx 2017 11 28.15353 02 52 32.562 -09 25 03.97 23.1z 14RX86 W84 C~52Tx 2022 10 29.382020 03 29 55.856 -08 06 04.26 23.5G 14RX86 G37 C~5z2h 2022 10 29.430000 03 29 55.644 -08 06 05.61 14RX86 G37 C~5z2h 2022 10 29.478440 03 29 55.346 -08 06 06.33 14RX86 G37 C~5z2h
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 0.02 0.00 0.07
2 0.0573 0.00 0.01 0.00 -0.18
3 0.1476 0.00 0.05 0.00 0.17
4 0.1477 0.00 -0.14 0.00 -0.02
5 0.2133 0.00 0.05 0.00 -0.12
6 1.2508 0.00 0.13 0.00 -0.12
7 1.2508 0.00 0.02 0.00 0.14
8 2.1352 0.00 -0.05 0.00 0.08
9 2.1488 0.00 -0.10 0.00 -0.14
10 2.3209 0.00 -0.01 0.00 -0.20
11 2.9735 0.00 -0.05 0.00 0.15
12 3.0281 0.00 0.05 0.00 0.23
13 3.1291 0.00 -0.07 0.00 -0.06
14 3.1291 0.00 0.05 0.00 0.00
15 3.2165 0.00 0.01 0.00 -0.06
16 3.2165 0.00 0.07 0.00 0.23
17 3.2329 0.00 0.08 0.00 -0.04
18 8.1507 0.00 0.01 0.00 -0.40
19 8.1508 0.00 0.42 0.00 -0.25
20 8.1509 0.00 -0.44 0.00 0.55
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.
14RX86 quality flag:3 Type: SCATEXTD SCATEXTD SCATEXTD axisobj 45.711 45.711 45.711 ecceobj 0.179 0.179 0.179 incobj 26.555 26.555 26.555 qmin 36.841 36.877 36.876 qmax 54.137 54.089 54.167 amean 45.309 45.313 45.313 amin 44.932 44.928 44.928 amax 45.749 45.762 45.748 emean 0.168 0.168 0.168 emin 0.153 0.152 0.152 emax 0.184 0.183 0.184 imean 25.707 25.724 25.717 imin 25.288 25.326 25.305 imax 26.056 26.078 26.067 excite_mean 0.465 0.465 0.465 fracstop 1.000 1.000 1.000 cjmean 2.844 2.844 2.844 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 179.7 179.8 180.0 kozaiamp 179.9 180.0 179.9