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: 14WN510
# Created Sun Nov 24 02:10:08 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 75 observations of 75
# Arc: 12.14y
# First observation: 2012/02/16
# Last observation: 2024/04/09
# Chi-squared of fit: 80.20 DOF: 144 RMS: 0.18
# Min/Max residuals: -0.56 0.48
# Exact a, adot, b, bdot, g, gdot:
1.679666E-05 2.652227E-02 3.041299E-06 4.291436E-03 2.413627E-02 -7.956545E-03
# Covariance matrix:
9.7669E-14 -3.3117E-14 7.7498E-15 -4.1144E-15 -3.0019E-15 -7.6965E-14
-3.3117E-14 1.6080E-14 -4.0711E-15 2.2705E-15 8.6330E-15 4.2549E-14
7.7498E-15 -4.0711E-15 5.3483E-14 -9.3921E-15 3.0945E-16 -1.2958E-14
-4.1144E-15 2.2705E-15 -9.3921E-15 2.6164E-15 8.6994E-16 7.0646E-15
-3.0019E-15 8.6330E-15 3.0945E-16 8.6994E-16 6.6781E-14 1.6999E-14
-7.6965E-14 4.2549E-14 -1.2958E-14 7.0646E-15 1.6999E-14 1.3228E-13
# lat0 lon0 xBary yBary zBary JD0
7.232434 164.198414 0.288683 0.119178 -0.939063 2455974.024756
# Heliocentric elements and errors
Epoch: 2455974.5000 = 2012/02/17
Mean Anomaly: 344.47950 +/- 0.002
Argument of Peri: 88.95800 +/- 0.003
Long of Asc Node: 126.59069 +/- 0.000
Inclination: 11.59218 +/- 0.000
Eccentricity: 0.51307897 +/- 0.0000
Semi-Major Axis: 76.00670862 +/- 0.0069
Time of Perihelion: 2466409.1917 +/- 31.6
Perihelion: 37.00926463 +/- 0.0044
Aphelion: 115.00415261 +/- 0.0108
Period (y) 662.6529 +/- 0.09
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -40.37790753 +/- 0.0004
Ecliptic Y 11.72869885 +/- 0.0001
Ecliptic Z 5.21612472 +/- 0.0001
Ecliptic XDOT 0.00009661 +/- 0.0000
Ecliptic YDOT -0.00315107 +/- 0.0000
Ecliptic ZDOT 0.00036939 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 42.36937954 +/- 0.0004
Geocenter to KBO 41.43166823 +/- 0.0004
# Hcoef: 6.25
The following table shows the complete astrometric record for 14WN510. 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 (14WN510) followed by the observatory code and reference code for the source of the astrometry.
2012 02 16.52399 11 13 10.729 +12 52 59.01 22.3w 14WN510 F51 C~2dYx 2012 02 16.52547 11 13 10.728 +12 52 59.04 22.5w 14WN510 F51 C~2dYx 2012 02 16.53866 11 13 10.677 +12 52 59.27 22.6w 14WN510 F51 C~2dYx 2012 02 16.54011 11 13 10.661 +12 52 59.62 22.4w 14WN510 F51 C~2dYx 2012 02 16.55338 11 13 10.616 +12 52 59.90 22.6w 14WN510 F51 C~2dYx 2012 02 16.55484 11 13 10.608 +12 53 00.05 22.5w 14WN510 F51 C~2dYx 2012 02 16.56809 11 13 10.554 +12 53 00.54 22.5w 14WN510 F51 C~2dYx 2012 02 16.56954 11 13 10.533 +12 53 00.57 22.6w 14WN510 F51 C~2dYx 2012 03 13.38998 11 11 18.192 +13 06 13.60 22.4G 14WN510 F51 C~2r7Z 2012 03 28.32875 11 10 14.373 +13 12 41.87 21.7G 14WN510 F51 C~2r7Z 2013 02 14.39999 11 19 26.347 +12 29 33.67 23.0G 14WN510 F51 C~2r7Z 2013 02 14.41455 11 19 26.284 +12 29 34.56 22.5G 14WN510 F51 C~2r7Z 2013 02 14.42917 11 19 26.220 +12 29 34.84 23.3G 14WN510 F51 C~2r7Z 2013 02 14.44392 11 19 26.156 +12 29 35.30 22.3G 14WN510 F51 C~2r7Z 2013 03 03.48800 11 18 13.658 +12 38 39.86 21.9G 14WN510 F51 C~2r7Z 2013 06 04.28507 11 14 02.625 +12 57 37.66 22.1G 14WN510 F51 C~2r7Z 2014 03 20.48721 11 23 14.906 +12 23 31.93 22.5G 14WN510 F51 C~2r7Z 2014 11 22.64259 11 33 01.098 +11 16 18.07 22.2G 14WN510 F51 C~2r7Z 2014 11 26.59493 11 33 12.420 +11 16 02.94 22.3w 14WN510 F51 C~1vXv 2014 11 26.60748 11 33 12.434 +11 16 02.92 22.4w 14WN510 F51 C~1vXv 2014 11 26.61998 11 33 12.495 +11 16 03.00 22.4w 14WN510 F51 C~1vXv 2014 11 30.58898 11 33 22.412 +11 15 57.68 22.6G 14WN510 F51 C~2r7Z 2014 11 30.60090 11 33 22.443 +11 15 57.69 22.5G 14WN510 F51 C~2r7Z 2014 11 30.61283 11 33 22.475 +11 15 57.40 22.7G 14WN510 F51 C~2r7Z 2014 11 30.62476 11 33 22.491 +11 15 58.02 22.8G 14WN510 F51 C~2r7Z 2014 12 09.61452 11 33 39.796 +11 16 22.38 23.1G 14WN510 F51 C~2r7Z 2015 01 27.62275 11 33 03.616 +11 31 47.68 23.4G 14WN510 F51 C~2r7Z 2015 01 29.63642 11 32 57.834 +11 32 47.93 22.4G 14WN510 F51 C~2r7Z 2015 02 16.40726 11 31 55.924 +11 42 12.25 22.2w 14WN510 F51 C~1vXv 2015 02 16.41869 11 31 55.861 +11 42 12.62 22.0w 14WN510 F51 C~1vXv 2015 02 16.43013 11 31 55.833 +11 42 12.97 22.2w 14WN510 F51 C~1vXv 2015 02 16.44158 11 31 55.789 +11 42 13.27 22.3w 14WN510 F51 C~1vXv 2015 03 24.47994 11 29 18.997 +12 01 00.45 22.2w 14WN510 F51 C~1vXv 2015 03 24.49143 11 29 18.954 +12 01 00.80 22.4w 14WN510 F51 C~1vXv 2015 03 24.50291 11 29 18.927 +12 01 01.07 22.1w 14WN510 F51 C~1vXv 2015 03 24.51436 11 29 18.846 +12 01 01.33 22.2w 14WN510 F51 C~1vXv 2015 03 25.49401 11 29 14.589 +12 01 27.94 22.5w 14WN510 F51 C~1vXv 2015 03 25.50550 11 29 14.538 +12 01 28.10 22.3w 14WN510 F51 C~1vXv 2015 03 25.51696 11 29 14.481 +12 01 28.77 22.3w 14WN510 F51 C~1vXv 2015 04 16.41497 11 27 47.180 +12 09 33.93 22.5w 14WN510 F51 C~1vXv 2015 04 16.42663 11 27 47.133 +12 09 34.17 22.3w 14WN510 F51 C~1vXv 2015 04 16.43826 11 27 47.090 +12 09 34.35 22.1w 14WN510 F51 C~1vXv 2015 04 18.43817 11 27 40.181 +12 10 06.77 22.5G 14WN510 F51 C~2r7Z 2016 01 13.51037 11 39 57.603 +10 59 51.46 22.5G 14WN510 F51 C~2r7Z 2016 03 01.40367 11 37 24.090 +11 24 21.64 22.2G 14WN510 F51 C~2r7Z 2016 03 11.38042 11 36 39.765 +11 29 43.75 22.5G 14WN510 F51 C~2r7Z 2016 03 29.30827 11 35 20.166 +11 38 21.44 23.6G 14WN510 F51 C~2r7Z 2016 03 29.32075 11 35 20.102 +11 38 21.64 22.2G 14WN510 F51 C~2r7Z 2016 03 29.33329 11 35 20.051 +11 38 21.73 22.0G 14WN510 F51 C~2r7Z 2016 03 29.34590 11 35 19.971 +11 38 22.12 22.3G 14WN510 F51 C~2r7Z 2016 04 05.30936 11 34 50.777 +11 41 11.88 21.8G 14WN510 F51 C~2r7Z 2016 04 22.38249 11 33 47.914 +11 46 28.93 22.4G 14WN510 F51 C~2r7Z 2016 05 20.34671 11 32 45.549 +11 49 10.02 23.2G 14WN510 F51 C~2r7Z 2017 01 30.47965 11 45 45.897 +10 41 35.50 22.1G 14WN510 F51 C~2r7Z 2017 01 30.49153 11 45 45.860 +10 41 35.66 22.2G 14WN510 F51 C~2r7Z 2017 01 30.50344 11 45 45.803 +10 41 36.55 21.5G 14WN510 F51 C~2r7Z 2017 01 30.51542 11 45 45.795 +10 41 36.78 21.7G 14WN510 F51 C~2r7Z 2017 02 16.56904 11 44 48.337 +10 50 45.09 22.0G 14WN510 F51 C~2r7Z 2017 03 20.29755 11 42 31.286 +11 07 59.95 22.1G 14WN510 F51 C~2r7Z 2017 03 20.30921 11 42 31.232 +11 08 00.32 22.2G 14WN510 F51 C~2r7Z 2017 03 20.32086 11 42 31.177 +11 08 00.68 22.4G 14WN510 F51 C~2r7Z 2017 03 20.33250 11 42 31.132 +11 08 01.13 22.4G 14WN510 F51 C~2r7Z 2017 04 20.27979 11 40 23.787 +11 20 11.20 22.8G 14WN510 F51 C~2r7Z 2017 04 20.29190 11 40 23.747 +11 20 11.62 22.6G 14WN510 F51 C~2r7Z 2017 04 20.30409 11 40 23.689 +11 20 11.57 22.4G 14WN510 F51 C~2r7Z 2017 05 09.35373 11 39 29.133 +11 23 33.81 23.2G 14WN510 F51 C~2r7Z 2018 04 10.17446 11 47 36.288 +10 50 10.64 22.5R 14WN510 G37 C~2dYx 2018 04 10.22689 11 47 36.110 +10 50 11.94 14WN510 G37 C~2dYx 2021 02 07.48805 12 11 58.899 +08 51 47.04 22.1w 14WN510 F51 C~4ZEi 2021 02 07.49852 12 11 58.857 +08 51 47.51 22.1w 14WN510 F51 C~4ZEi 2021 02 07.50901 12 11 58.843 +08 51 47.52 22.4w 14WN510 F51 C~4ZEi 2021 02 07.51951 12 11 58.791 +08 51 48.30 22.3w 14WN510 F51 C~4ZEi 2024 04 09.311389 12 28 29.770 +07 51 15.79 21.8w 14WN510 F52 C~7xPi 2024 04 09.322554 12 28 29.728 +07 51 15.88 21.7w 14WN510 F52 C~7xPi 2024 04 09.333686 12 28 29.688 +07 51 16.29 21.9w 14WN510 F52 C~7xPi
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 0.09 0.00 -0.09
2 0.0000 0.00 0.17 0.00 -0.11
3 0.0000 0.00 0.23 0.00 -0.30
4 0.0000 0.00 0.08 0.00 0.01
5 0.0001 0.00 0.24 0.00 -0.13
6 0.0001 0.00 0.21 0.00 -0.03
7 0.0001 0.00 0.23 0.00 0.04
8 0.0001 0.00 0.01 0.00 0.02
9 0.0708 0.00 -0.32 0.00 0.09
10 0.1117 0.00 -0.45 0.00 0.26
11 0.9962 0.00 -0.15 0.00 -0.33
12 0.9963 0.00 -0.20 0.00 0.09
13 0.9963 0.00 -0.27 0.00 -0.10
14 0.9964 0.00 -0.33 0.00 -0.12
15 1.0430 0.00 -0.42 0.00 -0.02
16 1.2971 0.00 0.00 0.00 -0.17
17 2.0889 0.00 0.06 0.00 -0.16
18 2.7656 0.00 -0.18 0.00 0.25
19 2.7764 0.00 0.33 0.00 0.04
20 2.7764 0.00 0.04 0.00 0.05
21 2.7764 0.00 0.47 0.00 0.16
22 2.7873 0.00 -0.14 0.00 -0.04
23 2.7873 0.00 -0.09 0.00 -0.04
24 2.7874 0.00 -0.01 0.00 -0.33
25 2.7874 0.00 -0.18 0.00 0.29
26 2.8120 0.00 -0.07 0.00 -0.16
27 2.9462 0.00 -0.15 0.00 -0.19
28 2.9517 0.00 0.12 0.00 0.13
29 3.0004 0.00 0.06 0.00 0.02
30 3.0004 0.00 -0.20 0.00 0.02
31 3.0004 0.00 0.07 0.00 -0.01
32 3.0005 0.00 0.10 0.00 -0.09
33 3.0991 0.00 -0.07 0.00 0.09
34 3.0992 0.00 0.05 0.00 0.13
35 3.0992 0.00 0.41 0.00 0.09
36 3.0992 0.00 -0.04 0.00 0.04
37 3.1019 0.00 0.20 0.00 0.20
38 3.1019 0.00 0.19 0.00 0.05
39 3.1020 0.00 0.10 0.00 0.41
40 3.1619 0.00 0.20 0.00 0.21
41 3.1620 0.00 0.12 0.00 0.26
42 3.1620 0.00 0.10 0.00 0.24
43 3.1675 0.00 -0.11 0.00 -0.10
44 3.9069 0.00 -0.20 0.00 0.01
45 4.0380 0.00 0.04 0.00 -0.04
46 4.0653 0.00 -0.22 0.00 0.04
47 4.1144 0.00 0.26 0.00 0.21
48 4.1144 0.00 0.12 0.00 0.09
49 4.1145 0.00 0.18 0.00 -0.14
50 4.1145 0.00 -0.19 0.00 -0.08
51 4.1336 0.00 -0.06 0.00 0.12
52 4.1803 0.00 0.09 0.00 0.11
53 4.2569 0.00 -0.01 0.00 -0.18
54 4.9554 0.00 0.06 0.00 0.16
55 4.9554 0.00 0.03 0.00 -0.04
56 4.9555 0.00 -0.31 0.00 0.48
57 4.9555 0.00 0.09 0.00 0.35
58 5.0022 0.00 -0.26 0.00 -0.25
59 5.0890 0.00 -0.01 0.00 -0.09
60 5.0891 0.00 -0.03 0.00 -0.07
61 5.0891 0.00 -0.05 0.00 -0.05
62 5.0891 0.00 0.07 0.00 0.05
63 5.1739 0.00 0.03 0.00 -0.19
64 5.1739 0.00 0.07 0.00 0.03
65 5.1739 0.00 -0.15 0.00 -0.21
66 5.2261 0.00 -0.07 0.00 -0.17
67 6.1455 0.00 -0.56 0.00 -0.26
68 6.1457 0.00 0.03 0.00 -0.13
69 8.9773 0.00 0.13 0.00 -0.17
70 8.9773 0.00 -0.03 0.00 -0.04
71 8.9774 0.00 0.23 0.00 -0.37
72 8.9774 0.00 -0.07 0.00 0.07
73 12.1445 0.00 -0.15 0.00 0.18
74 12.1446 0.00 -0.01 0.00 -0.03
75 12.1446 0.00 0.16 0.00 0.08
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.
14WN510 quality flag:3 Type: SCATNEAR SCATNEAR SCATNEAR axisobj 75.773 75.772 75.773 ecceobj 0.511 0.511 0.511 incobj 11.597 11.597 11.597 qmin 36.273 36.274 36.267 qmax 118.877 118.888 118.826 amean 76.079 76.139 76.136 amin 74.374 74.244 74.374 amax 77.960 77.957 77.934 emean 0.508 0.509 0.509 emin 0.491 0.491 0.491 emax 0.525 0.525 0.525 imean 10.852 10.886 10.774 imin 9.967 9.981 9.929 imax 11.675 11.676 11.675 excite_mean 0.542 0.543 0.542 fracstop 1.000 1.000 1.000 cjmean 3.084 3.084 3.084 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 177.1 180.0 178.9 kozaiamp 180.0 180.0 179.9