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: 14WK510 # Created Tue Apr 1 01:10:14 2025 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 36 observations of 36 # Arc: 11.06y # First observation: 2010/11/09 # Last observation: 2021/12/01 # Chi-squared of fit: 26.37 DOF: 66 RMS: 0.15 # Min/Max residuals: -0.53 0.42 # Exact a, adot, b, bdot, g, gdot: 1.947711E-05 3.577984E-02 2.472912E-06 3.976114E-03 2.958105E-02 1.863027E-03 # Covariance matrix: 1.8864E-13 -9.7559E-14 1.1650E-14 -7.0488E-15 -1.0621E-13 -2.0259E-13 -9.7559E-14 7.8406E-14 -1.1003E-14 6.3185E-15 1.1405E-13 1.8157E-13 1.1650E-14 -1.1003E-14 1.0766E-13 -2.3488E-14 -1.8477E-14 -2.8087E-14 -7.0488E-15 6.3185E-15 -2.3488E-14 8.7393E-15 8.4215E-15 1.7346E-14 -1.0621E-13 1.1405E-13 -1.8477E-14 8.4215E-15 2.8033E-13 2.4176E-13 -2.0259E-13 1.8157E-13 -2.8087E-14 1.7346E-14 2.4176E-13 4.9858E-13 # lat0 lon0 xBary yBary zBary JD0 -8.941194 73.429106 0.438565 -0.137673 -0.875086 2455510.041346 # Heliocentric elements and errors Epoch: 2455510.5000 = 2010/11/10 Mean Anomaly: 5.04141 +/- 0.003 Argument of Peri: 295.26302 +/- 0.005 Long of Asc Node: 126.93343 +/- 0.001 Inclination: 10.69425 +/- 0.000 Eccentricity: 0.30915362 +/- 0.0001 Semi-Major Axis: 50.02401873 +/- 0.0048 Time of Perihelion: 2453700.7632 +/- 1.0 Perihelion: 34.55891216 +/- 0.0042 Aphelion: 65.48912530 +/- 0.0068 Period (y) 353.8149 +/- 0.05 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 10.20077405 +/- 0.0002 Ecliptic Y 32.73081969 +/- 0.0006 Ecliptic Z -5.25400304 +/- 0.0001 Ecliptic XDOT -0.00310940 +/- 0.0000 Ecliptic YDOT 0.00116887 +/- 0.0000 Ecliptic ZDOT 0.00033673 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 34.68378643 +/- 0.0005 Geocenter to KBO 33.80543044 +/- 0.0006 # Hcoef: 6.89
The following table shows the complete astrometric record for 14WK510. 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 (14WK510) followed by the observatory code and reference code for the source of the astrometry.
2010 11 09.54058 04 52 37.206 +13 32 03.59 22.3G 14WK510 F51 C~2rYG 2010 11 09.55875 04 52 37.103 +13 32 03.31 22.5G 14WK510 F51 C~2rYG 2010 11 09.57696 04 52 37.027 +13 32 03.02 14WK510 F51 C~2rYG 2010 11 11.54347 04 52 26.911 +13 31 36.44 22.3G 14WK510 F51 C~2rYG 2010 11 17.51975 04 51 54.915 +13 30 19.91 22.3G 14WK510 F51 C~2rYG 2011 09 07.61501 05 03 00.813 +14 13 32.13 22.4G 14WK510 F51 C~2rYG 2011 09 10.57847 05 03 04.793 +14 13 00.21 21.7G 14WK510 F51 C~2rYG 2011 10 26.43063 05 01 57.864 +14 02 40.87 22.2w 14WK510 F51 C~1vXu 2011 10 26.44514 05 01 57.814 +14 02 40.54 22.4w 14WK510 F51 C~1vXu 2011 10 26.44579 05 01 57.804 +14 02 40.66 22.7w 14WK510 F51 C~1vXu 2011 10 26.45972 05 01 57.751 +14 02 40.47 22.5w 14WK510 F51 C~1vXu 2011 10 26.46039 05 01 57.749 +14 02 40.44 22.6w 14WK510 F51 C~1vXu 2011 10 26.47430 05 01 57.691 +14 02 40.14 22.4w 14WK510 F51 C~1vXu 2011 10 26.47498 05 01 57.691 +14 02 40.14 22.4w 14WK510 F51 C~1vXu 2013 04 05.26049 05 02 59.094 +14 42 09.58 22.8G 14WK510 F51 C~2rYG 2013 09 21.58472 05 19 25.914 +15 00 20.05 22.4G 14WK510 F51 C~2rYG 2013 11 27.36448 05 15 52.135 +14 47 54.91 22.2w 14WK510 F51 C~1vXu 2013 11 27.37971 05 15 52.043 +14 47 54.84 22.3w 14WK510 F51 C~1vXu 2013 11 27.39496 05 15 51.948 +14 47 54.72 22.4w 14WK510 F51 C~1vXu 2013 11 27.41030 05 15 51.872 +14 47 54.51 22.5w 14WK510 F51 C~1vXu 2014 02 27.27828 05 09 35.056 +14 55 17.99 22.7G 14WK510 F51 C~2rYG 2014 11 26.40766 05 24 16.366 +15 12 03.61 22.5w 14WK510 F51 C~1vXu 2014 11 26.42066 05 24 16.280 +15 12 03.86 22.3w 14WK510 F51 C~1vXu 2014 11 26.43361 05 24 16.208 +15 12 03.72 22.4w 14WK510 F51 C~1vXu 2014 12 12.48869 05 22 42.773 +15 10 43.53 22.5G 14WK510 F51 C~2rYG 2015 01 17.24193 05 19 26.515 +15 11 40.10 22.3w 14WK510 F51 C~1vXu 2015 01 17.25509 05 19 26.464 +15 11 40.20 22.4w 14WK510 F51 C~1vXu 2015 01 17.26825 05 19 26.394 +15 11 40.25 22.4w 14WK510 F51 C~1vXu 2015 01 17.28135 05 19 26.334 +15 11 40.50 22.3w 14WK510 F51 C~1vXu 2015 01 19.37433 05 19 16.952 +15 11 54.58 22.7G 14WK510 F51 C~2rYG 2015 01 19.38741 05 19 16.915 +15 11 54.61 22.5G 14WK510 F51 C~2rYG 2015 01 19.41357 05 19 16.787 +15 11 54.86 21.9G 14WK510 F51 C~2rYG 2016 01 26.42059 05 27 01.882 +15 36 05.35 22.6G 14WK510 F51 C~2rYG 2017 03 21.22291 05 34 07.343 +16 10 21.44 20.9G 14WK510 F51 C~2rYG 2021 12 01.459950 06 20 58.946 +17 23 14.76 22.6G 14WK510 G37 C~5J6g 2021 12 01.499480 06 20 58.689 +17 23 14.54 14WK510 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 -0.07 0.00 -0.08
2 0.0000 0.00 -0.20 0.00 -0.11
3 0.0001 0.00 0.08 0.00 -0.15
4 0.0055 0.00 0.05 0.00 -0.20
5 0.0218 0.00 0.05 0.00 -0.02
6 0.8270 0.00 -0.03 0.00 0.01
7 0.8351 0.00 0.04 0.00 0.24
8 0.9607 0.00 -0.04 0.00 0.07
9 0.9607 0.00 0.07 0.00 -0.06
10 0.9607 0.00 -0.04 0.00 0.07
11 0.9608 0.00 -0.01 0.00 0.07
12 0.9608 0.00 0.00 0.00 0.05
13 0.9608 0.00 -0.04 0.00 -0.05
14 0.9608 0.00 -0.00 0.00 -0.05
15 2.4031 0.00 -0.09 0.00 0.06
16 2.8667 0.00 -0.21 0.00 -0.13
17 3.0495 0.00 0.11 0.00 -0.02
18 3.0495 0.00 0.06 0.00 0.02
19 3.0496 0.00 -0.04 0.00 0.01
20 3.0496 0.00 0.15 0.00 -0.09
21 3.3011 0.00 0.18 0.00 0.09
22 4.0462 0.00 0.07 0.00 0.08
23 4.0462 0.00 -0.11 0.00 0.42
24 4.0463 0.00 -0.08 0.00 0.36
25 4.0902 0.00 -0.03 0.00 0.03
26 4.1881 0.00 0.03 0.00 -0.07
27 4.1881 0.00 0.19 0.00 -0.05
28 4.1882 0.00 0.05 0.00 -0.09
29 4.1882 0.00 0.07 0.00 0.07
30 4.1939 0.00 -0.18 0.00 0.03
31 4.1940 0.00 0.15 0.00 -0.03
32 4.1940 0.00 -0.02 0.00 0.04
33 5.2125 0.00 0.02 0.00 -0.05
34 6.3619 0.00 -0.44 0.00 -0.53
35 11.0607 0.00 0.42 0.00 0.13
36 11.0608 0.00 -0.31 0.00 -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.
14WK510 quality flag:3 Type: SCATNEAR SCATNEAR SCATNEAR axisobj 50.405 50.405 50.405 ecceobj 0.314 0.314 0.314 incobj 10.687 10.687 10.687 qmin 33.664 33.920 34.030 qmax 66.381 66.227 66.252 amean 49.394 49.199 49.738 amin 48.251 48.127 49.053 amax 50.430 50.405 50.407 emean 0.299 0.293 0.301 emin 0.279 0.269 0.287 emax 0.318 0.315 0.315 imean 9.045 9.031 9.741 imin 7.432 7.685 8.998 imax 10.172 10.242 10.567 excite_mean 0.338 0.332 0.345 fracstop 1.000 1.000 1.000 cjmean 3.023 3.027 3.021 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 188.5 184.0 172.2 kozaiamp 179.9 180.0 180.0