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: 14UO228
# Created Fri Nov 22 02:10:06 2024
# Orbit generated from Bernstein formalism
# Fitting 34 observations of 35
# Arc: 4.06y
# First observation: 2013/08/09
# Last observation: 2017/08/30
Preliminary a, adot, b, bdot, g, gdot:
-0.000110 0.030437 0.000015 0.003427 0.028043 0.000000
# Chi-squared of fit: 12.41 DOF: 62 RMS: 0.11
# Min/Max residuals: -0.29 0.26
# Exact a, adot, b, bdot, g, gdot:
1.649672E-05 3.032665E-02 1.304142E-06 3.423564E-03 2.805568E-02 3.388599E-03
# Covariance matrix:
1.8383E-13 -1.1173E-13 2.8905E-15 -7.9542E-15 6.6638E-14 -5.8975E-13
-1.1173E-13 2.1685E-13 -1.1065E-14 2.2826E-14 4.5564E-14 1.7302E-12
2.8905E-15 -1.1065E-14 8.7426E-14 -4.4592E-14 -4.6448E-15 -1.1154E-13
-7.9542E-15 2.2826E-14 -4.4592E-14 4.5277E-14 7.1824E-15 2.2753E-13
6.6638E-14 4.5564E-14 -4.6448E-15 7.1824E-15 1.1376E-13 5.6027E-13
-5.8975E-13 1.7302E-12 -1.1154E-13 2.2753E-13 5.6027E-13 1.7263E-11
# lat0 lon0 xBary yBary zBary JD0
2.179463 27.774202 0.960174 0.012617 -0.330654 2456514.012218
# Heliocentric elements and errors
Epoch: 2456510.5000 = 2013/08/06
Mean Anomaly: 36.54131 +/- 0.029
Argument of Peri: 332.29929 +/- 0.042
Long of Asc Node: 7.91878 +/- 0.001
Inclination: 6.83487 +/- 0.000
Eccentricity: 0.12383112 +/- 0.0001
Semi-Major Axis: 39.68350334 +/- 0.0029
Time of Perihelion: 2447242.3069 +/- 7.2
Perihelion: 34.76945058 +/- 0.0056
Aphelion: 44.59755610 +/- 0.0059
Period (y) 249.9903 +/- 0.03
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X 32.25397410 +/- 0.0004
Ecliptic Y 15.90505555 +/- 0.0002
Ecliptic Z 1.35559147 +/- 0.0000
Ecliptic XDOT -0.00110417 +/- 0.0000
Ecliptic YDOT 0.00276568 +/- 0.0000
Ecliptic ZDOT 0.00034657 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 35.98787665 +/- 0.0004
Geocenter to KBO 35.64340195 +/- 0.0004
# Hcoef: 9.00
The following table shows the complete astrometric record for 14UO228. 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 (14UO228) followed by the observatory code and reference code for the source of the astrometry.
2013 08 09.51144 01 39 57.611 +12 42 57.24 24.4r 14UO228 568 C~2SDg 2013 08 09.55415 01 39 57.557 +12 42 56.98 24.4r 14UO228 568 C~2SDg 2013 09 02.42913 01 39 02.787 +12 39 59.30 14UO228 568 C~2SDg 2013 09 02.47226 01 39 02.631 +12 39 58.12 24.9r 14UO228 568 C~2SDg 2013 09 03.44820 01 38 59.333 +12 39 44.36 24.7r 14UO228 568 C~2SDg 2013 09 03.49483 01 38 59.180 +12 39 43.75 24.5r 14UO228 568 C~2SDg 2013 10 08.49603 01 36 20.257 +12 27 01.39 24.9r 14UO228 568 C~2SDg 2013 10 30.41166 01 34 22.696 +12 16 34.15 25.1r 14UO228 568 C~2SDg 2013 10 30.49029 01 34 22.270 +12 16 31.71 23.8r 14UO228 568 C~2SDg 2013 11 28.26487 01 32 08.454 +12 03 47.82 24.6r 14UO228 568 C~2SDg 2013 12 04.38623 01 31 46.776 +12 01 37.22 24.7r 14UO228 568 C~2SDg 2013 12 29.24699 01 30 54.505 +11 55 56.14 24.4r 14UO228 568 C~2SDg 2013 12 30.33812 01 30 53.686 +11 55 48.86 24.3r 14UO228 568 C~2SDg 2013 12 30.34280 01 30 53.662 +11 55 48.88 24.3r 14UO228 568 C~2SDg 2014 01 03.24172 01 30 51.710 +11 55 29.74 24.6r 14UO228 568 C~2SDg 2014 07 26.52587 01 46 22.524 +13 29 57.92 24.8r 14UO228 568 C~2SDg 2014 07 26.56909 01 46 22.552 +13 29 58.21 25.2r 14UO228 568 C~2SDg 2014 07 26.61244 01 46 22.555 +13 29 58.70 24.6r 14UO228 568 C~2SDg 2014 08 24.53579 01 45 53.731 +13 30 15.31 24.2r 14UO228 568 C~2SDg 2014 08 30.44167 01 45 37.824 +13 29 20.14 25.0r 14UO228 568 C~2SDg 2014 08 30.54834 01 45 37.511 +13 29 19.19 24.3r 14UO228 568 C~2SDg 2014 09 18.46688 01 44 27.270 +13 24 23.53 24.6r 14UO228 568 C~2SDg 2014 09 18.50960 01 44 27.082 +13 24 22.70 24.8r 14UO228 568 C~2SDg 2014 09 23.50788 01 44 04.416 +13 22 37.96 24.8r 14UO228 568 C~2SDg 2014 10 22.29094 01 41 35.214 +13 10 11.22 24.3r 14UO228 568 C~2SDg 2014 10 22.33551 01 41 34.997 +13 10 09.75 24.3r 14UO228 568 C~2SDg 2014 10 22.38043 01 41 34.739 +13 10 08.61 24.7r 14UO228 568 C~2SDg 2014 10 23.47641 01 41 28.785 +13 09 37.39 24.0r 14UO228 568 C~2SDg 2014 10 25.49236 01 41 17.863 +13 08 39.52 24.3r 14UO228 568 C~2SDg 2014 11 20.34891 01 39 07.330 +12 56 39.53 24.8r 14UO228 568 C~2SDg 2015 02 18.23954 01 38 41.523 +12 51 18.41 24.4r 14UO228 568 C~2SDg 2015 12 07.42022 01 44 25.531 +13 38 49.71 24.6w 14UO228 568 C~2SDg 2016 09 27.46659 01 56 37.965 +14 56 36.07 24.4w 14UO228 568 C~2SDg 2017 08 25.57304 02 05 02.023 +15 49 56.22 24.6w 14UO228 568 C~2SDg 2017 08 30.59490 02 04 50.313 +15 49 27.87 25.1w 14UO228 568 C~2SDg
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 0.12 0.00 0.13
2 0.0001 -0.83 0.02 0.04 -0.09
3 0.0655 -812.38 ( 0.03) 123.86 ( 0.53)
4 0.0656 -814.94 -0.29 123.58 0.02
5 0.0683 -864.91 0.02 128.21 0.02
6 0.0684 -867.22 0.20 128.45 0.01
7 0.1642 -3312.38 0.20 262.34 -0.03
8 0.2242 -5145.79 -0.02 306.86 0.12
9 0.2244 -5152.50 -0.13 306.87 -0.00
10 0.3032 -7259.99 0.04 315.69 -0.04
11 0.3200 -7604.19 -0.13 311.20 -0.11
12 0.3881 -8444.16 -0.12 276.56 0.23
13 0.3910 -8458.04 0.26 274.23 -0.16
14 0.3911 -8458.36 -0.00 274.37 -0.00
15 0.4017 -8492.10 -0.09 267.14 0.08
16 0.9610 6262.17 0.02 621.70 0.06
17 0.9611 6262.65 0.12 621.83 -0.09
18 0.9613 6262.87 -0.04 622.27 0.07
19 1.0404 5875.42 -0.11 787.14 -0.00
20 1.0566 5638.76 -0.19 818.04 -0.12
21 1.0569 5634.15 0.06 818.77 0.00
22 1.1087 4570.66 -0.02 907.39 -0.03
23 1.1088 4567.80 0.03 907.59 -0.03
24 1.1225 4221.29 0.00 927.76 -0.01
25 1.2013 1919.55 -0.20 1010.67 0.10
26 1.2014 1916.06 0.11 1010.44 -0.25
27 1.2016 1912.14 0.02 1010.73 -0.06
28 1.2046 1819.75 0.06 1012.84 0.05
29 1.2101 1650.07 -0.05 1016.19 0.03
30 1.2809 -388.76 0.00 1032.40 -0.07
31 1.5270 -856.71 0.01 869.52 0.20
32 2.3269 4856.11 0.09 1725.92 -0.07
33 3.1347 16497.31 0.04 2366.53 -0.07
34 4.0440 24521.30 -0.12 2904.94 0.08
35 4.0577 24350.24 0.10 2935.02 0.03
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.
14UO228 quality flag:3 Type: 3:2E 3:2E 3:2E axisobj 39.898 39.907 39.888 ecceobj 0.129 0.130 0.129 incobj 6.816 6.816 6.816 qmin 34.100 34.018 34.116 qmax 45.440 45.538 45.439 amean 39.459 39.459 39.459 amin 38.994 38.986 39.008 amax 39.960 39.984 39.951 emean 0.117 0.118 0.116 emin 0.096 0.097 0.096 emax 0.138 0.140 0.138 imean 6.536 6.501 6.577 imin 5.303 5.120 5.485 imax 7.418 7.523 7.436 excite_mean 0.164 0.164 0.164 fracstop 1.000 1.000 1.000 cjmean 3.021 3.021 3.021 libcent 0 180.1 180.8 181.0 libamp 0 108.2 111.1 104.6 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 179.1 183.2 182.0 kozaiamp 180.0 180.0 180.0