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: 14WM517 # Created Sat Apr 27 01:16:46 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 45 observations of 45 # Arc: 5.03y # First observation: 2014/11/23 # Last observation: 2019/12/04 # Chi-squared of fit: 44.10 DOF: 84 RMS: 0.18 # Min/Max residuals: -0.51 0.53 # Exact a, adot, b, bdot, g, gdot: 1.383910E-05 1.938071E-02 -1.751856E-06 -3.259968E-03 2.147149E-02 1.072288E-03 # Covariance matrix: 1.1911E-13 -6.9200E-14 -3.5336E-15 6.9070E-15 -2.6764E-14 -4.6597E-13 -6.9200E-14 1.5577E-13 1.3714E-14 -2.2427E-14 -1.5564E-14 1.5238E-12 -3.5336E-15 1.3714E-14 9.7066E-14 -2.9543E-14 -2.7686E-15 1.4469E-13 6.9070E-15 -2.2427E-14 -2.9543E-14 1.5759E-14 1.3776E-15 -2.3886E-13 -2.6764E-14 -1.5564E-14 -2.7686E-15 1.3776E-15 8.9057E-14 -1.0284E-13 -4.6597E-13 1.5238E-12 1.4469E-13 -2.3886E-13 -1.0284E-13 1.6222E-11 # lat0 lon0 xBary yBary zBary JD0 -17.462036 27.170108 -0.543666 -0.247401 -0.786998 2456984.818227 # Heliocentric elements and errors Epoch: 2456984.5000 = 2014/11/23 Mean Anomaly: 80.84151 +/- 0.056 Argument of Peri: 154.05108 +/- 0.050 Long of Asc Node: 147.19282 +/- 0.001 Inclination: 19.50618 +/- 0.000 Eccentricity: 0.06300588 +/- 0.0002 Semi-Major Axis: 47.65346205 +/- 0.0042 Time of Perihelion: 2430002.6318 +/- 19.1 Perihelion: 44.65101377 +/- 0.0107 Aphelion: 50.65591032 +/- 0.0109 Period (y) 328.9651 +/- 0.04 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 40.00745931 +/- 0.0005 Ecliptic Y 21.14891484 +/- 0.0003 Ecliptic Z -13.97555442 +/- 0.0002 Ecliptic XDOT -0.00112762 +/- 0.0000 Ecliptic YDOT 0.00219616 +/- 0.0000 Ecliptic ZDOT -0.00043745 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 47.36227958 +/- 0.0005 Geocenter to KBO 46.57339440 +/- 0.0006 # Hcoef: 7.41
The following table shows the complete astrometric record for 14WM517. 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 (14WM517) followed by the observatory code and reference code for the source of the astrometry.
2014 11 23.317449 02 05 47.646 -05 51 24.88 23.9i 14WM517 568 C~2Tu9 2014 11 23.436477 02 05 47.203 -05 51 25.84 23.7i 14WM517 568 C~2Tu9 2014 11 23.459204 02 05 47.125 -05 51 25.98 23.7i 14WM517 568 C~2Tu9 2014 11 23.474241 02 05 47.065 -05 51 26.21 23.7i 14WM517 568 C~2Tu9 2014 11 28.363340 02 05 30.116 -05 51 59.60 24.1r 14WM517 568 C~2Tu9 2014 11 28.382242 02 05 30.055 -05 51 59.73 24.2r 14WM517 568 C~2Tu9 2014 11 28.403031 02 05 29.981 -05 51 59.75 24.3r 14WM517 568 C~2Tu9 2014 11 28.419743 02 05 29.920 -05 51 59.90 24.3r 14WM517 568 C~2Tu9 2014 11 28.457239 02 05 29.793 -05 52 00.07 23.8i 14WM517 568 C~2Tu9 2014 11 28.463420 02 05 29.768 -05 52 00.07 24.0i 14WM517 568 C~2Tu9 2014 11 28.474502 02 05 29.731 -05 52 00.22 23.4i 14WM517 568 C~2Tu9 2014 11 28.479935 02 05 29.722 -05 52 00.17 23.9i 14WM517 568 C~2Tu9 2016 08 15.413247 02 19 49.04 -04 42 32.1 23.9r 14WM517 W84 C~2b7x 2016 08 25.389451 02 19 39.38 -04 47 14.2 23.7i 14WM517 W84 C~2b7x 2016 08 25.393432 02 19 39.37 -04 47 14.5 23.7z 14WM517 W84 C~2b7x 2016 09 22.172506 02 18 35.93 -05 01 35.7 24.0r 14WM517 W84 C~2b7x 2016 11 02.061951 02 15 59.86 -05 19 54.0 24.1r 14WM517 W84 C~2b7x 2016 11 02.064312 02 15 59.88 -05 19 54.0 23.5i 14WM517 W84 C~2b7x 2016 11 09.059589 02 15 31.28 -05 22 01.3 23.2i 14WM517 W84 C~2b7x 2017 08 17.374372 02 24 08.49 -04 29 59.3 23.8z 14WM517 W84 C~2b7x 2017 08 17.405716 02 24 08.47 -04 30 00.2 24.5r 14WM517 W84 C~2b7x 2017 08 18.283969 02 24 07.90 -04 30 24.3 23.9i 14WM517 W84 C~2b7x 2017 08 24.386360 02 24 02.14 -04 33 16.9 24.1r 14WM517 W84 C~2b7x 2017 08 24.415295 02 24 02.11 -04 33 17.5 24.0i 14WM517 W84 C~2b7x 2017 08 25.363711 02 24 00.97 -04 33 45.1 24.0z 14WM517 W84 C~2b7x 2017 09 13.333774 02 23 24.67 -04 43 24.3 23.8z 14WM517 W84 C~2b7x 2017 09 14.217344 02 23 22.40 -04 43 52.4 24.6r 14WM517 W84 C~2b7x 2017 09 19.271041 02 23 08.48 -04 46 31.1 24.1i 14WM517 W84 C~2b7x 2017 09 19.307707 02 23 08.40 -04 46 31.7 23.6z 14WM517 W84 C~2b7x 2017 09 23.249196 02 22 56.54 -04 48 35.2 24.3z 14WM517 W84 C~2b7x 2017 09 23.298316 02 22 56.38 -04 48 37.2 24.9g 14WM517 W84 C~2b7x 2017 09 23.310902 02 22 56.34 -04 48 37.1 24.3r 14WM517 W84 C~2b7x 2017 09 25.179441 02 22 50.44 -04 49 35.4 24.1i 14WM517 W84 C~2b7x 2017 10 02.287746 02 22 26.45 -04 53 11.7 24.1i 14WM517 W84 C~2b7x 2017 10 10.131962 02 21 57.61 -04 57 00.5 23.3z 14WM517 W84 C~2b7x 2017 12 22.048258 02 17 34.05 -05 11 49.9 23.6i 14WM517 W84 C~2b7x 2018 01 04.092506 02 17 12.07 -05 09 15.1 23.4i 14WM517 W84 C~2b7x 2018 01 04.099115 02 17 12.09 -05 09 14.9 23.6z 14WM517 W84 C~2b7x 2019 10 27.43225 02 29 36.52 -04 37 00.2 24.4i 14WM517 T09 C~7bKK 2019 10 27.45055 02 29 36.43 -04 37 00.7 24.2i 14WM517 T09 C~7bKK 2019 10 27.46883 02 29 36.36 -04 37 00.9 24.4i 14WM517 T09 C~7bKK 2019 12 04.33301 02 27 08.03 -04 45 40.3 25.4z 14WM517 T09 C~7bKK 2019 12 04.35514 02 27 07.94 -04 45 40.5 24.8z 14WM517 T09 C~7bKK 2019 12 04.40339 02 27 07.77 -04 45 40.5 24.9i 14WM517 T09 C~7bKK 2019 12 04.44735 02 27 07.62 -04 45 40.8 24.2i 14WM517 T09 C~7bKK
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 0.13 0.00 -0.09
2 0.0003 0.00 0.00 0.00 -0.06
3 0.0004 0.00 0.07 0.00 -0.01
4 0.0004 0.00 -0.01 0.00 -0.12
5 0.0138 0.00 0.03 0.00 -0.05
6 0.0139 0.00 0.09 0.00 -0.07
7 0.0139 0.00 0.05 0.00 0.02
8 0.0140 0.00 -0.01 0.00 -0.04
9 0.0141 0.00 0.00 0.00 -0.02
10 0.0141 0.00 -0.06 0.00 0.02
11 0.0141 0.00 -0.04 0.00 -0.08
12 0.0141 0.00 0.10 0.00 0.00
13 1.7278 0.00 -0.16 0.00 -0.27
14 1.7552 0.00 -0.06 0.00 0.23
15 1.7552 0.00 -0.13 0.00 0.04
16 1.8312 0.00 0.21 0.00 0.36
17 1.9432 0.00 -0.51 0.00 0.22
18 1.9432 0.00 -0.06 0.00 0.27
19 1.9623 0.00 -0.32 0.00 -0.29
20 2.7325 0.00 -0.04 0.00 0.05
21 2.7326 0.00 -0.01 0.00 0.00
22 2.7350 0.00 0.17 0.00 -0.06
23 2.7517 0.00 -0.10 0.00 -0.18
24 2.7518 0.00 -0.01 0.00 0.05
25 2.7544 0.00 0.05 0.00 0.03
26 2.8063 0.00 0.32 0.00 0.47
27 2.8088 0.00 0.24 0.00 0.09
28 2.8226 0.00 -0.09 0.00 -0.02
29 2.8227 0.00 0.34 0.00 0.53
30 2.8335 0.00 0.10 0.00 0.11
31 2.8336 0.00 0.04 0.00 -0.37
32 2.8337 0.00 0.04 0.00 0.13
33 2.8388 0.00 0.03 0.00 -0.24
34 2.8582 0.00 -0.03 0.00 0.00
35 2.8797 0.00 -0.41 0.00 -0.21
36 3.0793 0.00 0.17 0.00 0.04
37 3.1151 0.00 -0.11 0.00 0.02
38 3.1151 0.00 0.31 0.00 0.12
39 4.9257 0.00 -0.03 0.00 -0.14
40 4.9258 0.00 -0.23 0.00 -0.22
41 4.9258 0.00 -0.13 0.00 -0.01
42 5.0295 0.00 0.27 0.00 0.02
43 5.0295 0.00 0.06 0.00 -0.11
44 5.0297 0.00 -0.00 0.00 0.05
45 5.0298 0.00 0.01 0.00 -0.11
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.
14WM517 quality flag:1 Type: SCATNEAR 2:1E SCATEXTD axisobj 48.090 48.090 48.090 ecceobj 0.067 0.067 0.067 incobj 19.464 19.464 19.464 qmin 38.049 39.818 39.989 qmax 58.133 56.297 55.900 amean 47.797 47.797 47.797 amin 47.302 47.366 47.369 amax 48.384 48.293 48.288 emean 0.104 0.092 0.082 emin 0.001 0.000 0.001 emax 0.201 0.166 0.160 imean 17.919 17.927 18.048 imin 16.078 16.699 16.622 imax 19.147 18.817 19.098 excite_mean 0.327 0.323 0.323 fracstop 1.000 1.000 1.000 cjmean 3.012 3.015 3.015 libcent 0 -180.0 173.9 -180.0 libamp 0 -180.0 144.2 -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 257.7 200.3 234.0 kozaiamp 179.9 180.0 179.9