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: 14WR510 # Created Sat Apr 20 01:16:49 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 37 observations of 37 # Arc: 10.99y # First observation: 2010/12/05 # Last observation: 2021/12/01 # Chi-squared of fit: 24.70 DOF: 68 RMS: 0.14 # Min/Max residuals: -0.46 0.32 # Exact a, adot, b, bdot, g, gdot: 2.047588E-05 4.661298E-02 -2.536700E-06 -6.531534E-03 3.579202E-02 8.550659E-04 # Covariance matrix: 4.1373E-13 -1.3991E-13 -4.0197E-14 1.6446E-14 7.0051E-14 -1.9114E-13 -1.3991E-13 5.8755E-14 1.6653E-14 -7.4860E-15 -4.8050E-15 8.9425E-14 -4.0197E-14 1.6653E-14 1.3468E-13 -2.4273E-14 -9.8875E-15 2.6986E-14 1.6446E-14 -7.4860E-15 -2.4273E-14 6.4218E-15 4.4028E-16 -1.2566E-14 7.0051E-14 -4.8050E-15 -9.8875E-15 4.4028E-16 1.4701E-13 7.8527E-15 -1.9114E-13 8.9425E-14 2.6986E-14 -1.2566E-14 7.8527E-15 1.5153E-13 # lat0 lon0 xBary yBary zBary JD0 -7.978980 76.034847 0.048792 -0.136578 -0.974448 2455535.864896 # Heliocentric elements and errors Epoch: 2455536.5000 = 2010/12/06 Mean Anomaly: 2.60473 +/- 0.001 Argument of Peri: 219.59375 +/- 0.002 Long of Asc Node: 212.18640 +/- 0.000 Inclination: 11.07624 +/- 0.000 Eccentricity: 0.26900202 +/- 0.0000 Semi-Major Axis: 39.52632199 +/- 0.0027 Time of Perihelion: 2454879.7683 +/- 0.3 Perihelion: 28.89366135 +/- 0.0026 Aphelion: 50.15898263 +/- 0.0039 Period (y) 248.5065 +/- 0.03 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 6.96578622 +/- 0.0001 Ecliptic Y 27.79326292 +/- 0.0003 Ecliptic Z -3.87832593 +/- 0.0000 Ecliptic XDOT -0.00346185 +/- 0.0000 Ecliptic YDOT 0.00086231 +/- 0.0000 Ecliptic ZDOT -0.00050386 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 28.91415698 +/- 0.0003 Geocenter to KBO 27.93921155 +/- 0.0003 # Hcoef: 7.46
The following table shows the complete astrometric record for 14WR510. 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 (14WR510) followed by the observatory code and reference code for the source of the astrometry.
2010 12 05.36413 05 02 45.693 +14 46 09.42 22.0G 14WR510 F51 C~2qbb 2010 12 05.40558 05 02 45.397 +14 46 08.70 21.9G 14WR510 F51 C~2qbb 2011 12 02.55578 05 14 15.333 +14 39 28.57 22.4G 14WR510 F51 C~2qbb 2012 02 10.30804 05 07 48.090 +14 36 35.98 22.2G 14WR510 F51 C~2qbb 2013 01 17.28291 05 20 16.337 +14 25 50.55 22.7G 14WR510 F51 C~2qbb 2013 01 18.23377 05 20 11.332 +14 25 53.69 21.9G 14WR510 F51 C~2qbb 2013 01 18.24527 05 20 11.277 +14 25 53.91 21.8G 14WR510 F51 C~2qbb 2013 04 04.24915 05 19 48.534 +14 42 22.16 22.8G 14WR510 F51 C~2qbb 2013 04 04.25376 05 19 48.561 +14 42 22.30 22.8G 14WR510 F51 C~2qbb 2013 04 04.25839 05 19 48.579 +14 42 22.19 23.1G 14WR510 F51 C~2qbb 2013 04 04.26301 05 19 48.600 +14 42 22.24 22.4G 14WR510 F51 C~2qbb 2013 11 27.38502 05 36 55.018 +14 19 37.73 21.7w 14WR510 F51 C~1vXv 2013 11 27.40027 05 36 54.914 +14 19 37.55 22.1w 14WR510 F51 C~1vXv 2013 11 27.41563 05 36 54.817 +14 19 37.43 22.2w 14WR510 F51 C~1vXv 2014 02 20.28564 05 29 12.658 +14 20 32.85 22.5w 14WR510 F51 C~1vXv 2014 02 20.29718 05 29 12.626 +14 20 32.96 22.1w 14WR510 F51 C~1vXv 2014 02 20.30861 05 29 12.614 +14 20 33.03 22.2w 14WR510 F51 C~1vXv 2014 02 20.32007 05 29 12.602 +14 20 33.44 22.2w 14WR510 F51 C~1vXv 2014 11 26.40219 05 48 00.345 +14 06 31.41 21.9G 14WR510 F51 C~2qbb 2014 11 26.41522 05 48 00.244 +14 06 31.21 21.8G 14WR510 F51 C~2qbb 2014 11 28.53704 05 47 46.782 +14 06 04.95 21.9w 14WR510 F51 C~1vXv 2014 11 28.55126 05 47 46.672 +14 06 04.70 22.1w 14WR510 F51 C~1vXv 2014 11 28.56542 05 47 46.583 +14 06 04.41 22.1w 14WR510 F51 C~1vXv 2014 11 28.57959 05 47 46.486 +14 06 04.41 21.9w 14WR510 F51 C~1vXv 2014 12 12.51720 05 46 12.769 +14 03 46.58 21.8G 14WR510 F51 C~2qbb 2014 12 12.53025 05 46 12.678 +14 03 46.38 21.7G 14WR510 F51 C~2qbb 2015 01 17.24880 05 42 14.832 +14 03 00.19 22.1w 14WR510 F51 C~1vXv 2015 01 17.26193 05 42 14.744 +14 03 00.27 22.2w 14WR510 F51 C~1vXv 2015 01 17.27508 05 42 14.676 +14 03 00.43 22.2w 14WR510 F51 C~1vXv 2015 10 19.51348 06 01 34.999 +14 02 04.46 21.7G 14WR510 F51 C~2qbb 2015 10 19.52470 06 01 34.962 +14 02 04.11 21.1G 14WR510 F51 C~2qbb 2015 10 19.53591 06 01 34.943 +14 02 04.08 21.6G 14WR510 F51 C~2qbb 2017 12 20.49152 06 17 39.345 +13 13 31.70 21.8R 14WR510 G37 C~2Uxq 2017 12 20.50467 06 17 39.249 +13 13 31.84 14WR510 G37 C~2Uxq 2021 12 01.427170 07 01 07.170 +11 47 39.73 22.2G 14WR510 G37 C~5J6g 2021 12 01.466530 07 01 07.011 +11 47 39.49 14WR510 G37 C~5J6g 2021 12 01.506330 07 01 06.788 +11 47 39.18 14WR510 G37 C~5J6g
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 -0.07
2 0.0001 0.00 0.02 0.00 -0.19
3 0.9916 0.00 0.03 0.00 0.07
4 1.1826 0.00 -0.22 0.00 0.26
5 2.1189 0.00 0.28 0.00 -0.38
6 2.1215 0.00 -0.06 0.00 -0.06
7 2.1215 0.00 0.03 0.00 0.12
8 2.3296 0.00 -0.04 0.00 0.15
9 2.3296 0.00 0.03 0.00 0.20
10 2.3296 0.00 -0.04 0.00 0.01
11 2.3296 0.00 -0.06 0.00 -0.02
12 2.9788 0.00 0.06 0.00 0.08
13 2.9789 0.00 0.01 0.00 0.10
14 2.9789 0.00 0.08 0.00 0.18
15 3.2113 0.00 0.04 0.00 -0.04
16 3.2113 0.00 -0.16 0.00 -0.08
17 3.2113 0.00 -0.07 0.00 -0.17
18 3.2114 0.00 0.03 0.00 0.09
19 3.9755 0.00 -0.09 0.00 0.05
20 3.9755 0.00 -0.35 0.00 0.01
21 3.9813 0.00 0.13 0.00 0.11
22 3.9813 0.00 -0.13 0.00 0.04
23 3.9814 0.00 -0.07 0.00 -0.08
24 3.9814 0.00 -0.14 0.00 0.09
25 4.0196 0.00 0.26 0.00 0.01
26 4.0196 0.00 0.28 0.00 -0.09
27 4.1174 0.00 0.07 0.00 -0.02
28 4.1174 0.00 -0.09 0.00 -0.01
29 4.1175 0.00 0.05 0.00 0.08
30 4.8710 0.00 0.06 0.00 -0.12
31 4.8711 0.00 -0.14 0.00 -0.24
32 4.8711 0.00 -0.07 0.00 -0.04
33 7.0421 0.00 0.07 0.00 -0.19
34 7.0421 0.00 0.00 0.00 -0.02
35 10.9899 0.00 -0.46 0.00 0.05
36 10.9900 0.00 0.32 0.00 0.07
37 10.9901 0.00 0.18 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.
14WR510 quality flag:3 Type: 3:2E 3:2E 3:2E axisobj 39.790 39.790 39.790 ecceobj 0.273 0.273 0.273 incobj 11.060 11.060 11.060 qmin 27.534 27.534 27.533 qmax 51.890 51.889 51.892 amean 39.454 39.454 39.454 amin 39.060 39.059 39.061 amax 39.927 39.929 39.926 emean 0.252 0.252 0.252 emin 0.197 0.197 0.197 emax 0.301 0.301 0.301 imean 12.452 12.452 12.452 imin 9.330 9.330 9.330 imax 15.561 15.561 15.561 excite_mean 0.334 0.334 0.334 fracstop 1.000 1.000 1.000 cjmean 2.924 2.924 2.924 libcent 0 179.9 179.9 179.9 libamp 0 46.7 46.7 46.7 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 273.4 273.4 273.4 kozaiamp 55.5 55.5 55.5