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: 15KV174
# Created Thu Nov 28 02:10:21 2024
# Orbit generated from Bernstein formalism
# Fitting 38 observations of 38
# Arc: 3.24y
# First observation: 2014/05/30
# Last observation: 2017/08/26
Preliminary a, adot, b, bdot, g, gdot:
0.000135 0.028132 -0.000073 -0.011322 0.026839 0.000000
# Chi-squared of fit: 7.24 DOF: 70 RMS: 0.08
# Min/Max residuals: -0.21 0.22
# Exact a, adot, b, bdot, g, gdot:
1.660842E-05 2.831923E-02 -6.600007E-06 -1.141866E-02 2.692497E-02 -4.576164E-03
# Covariance matrix:
1.9407E-13 -2.1038E-13 -3.9714E-14 7.2226E-14 -7.0587E-14 -1.7700E-12
-2.1038E-13 3.8593E-13 9.1219E-14 -1.6788E-13 1.0620E-13 4.0823E-12
-3.9714E-14 9.1219E-14 1.4235E-13 -9.9711E-14 2.4309E-14 1.0796E-12
7.2226E-14 -1.6788E-13 -9.9711E-14 1.2062E-13 -4.1689E-14 -1.9937E-12
-7.0587E-14 1.0620E-13 2.4309E-14 -4.1689E-14 1.1443E-13 1.0622E-12
-1.7700E-12 4.0823E-12 1.0796E-12 -1.9937E-12 1.0622E-12 4.8372E-11
# lat0 lon0 xBary yBary zBary JD0
7.844757 -126.636702 -0.270684 0.133542 -0.968857 2456807.886218
# Heliocentric elements and errors
Epoch: 2456800.5000 = 2014/05/23
Mean Anomaly: 341.09117 +/- 0.022
Argument of Peri: 195.92575 +/- 0.047
Long of Asc Node: 71.95404 +/- 0.000
Inclination: 23.27094 +/- 0.000
Eccentricity: 0.29894189 +/- 0.0001
Semi-Major Axis: 52.02235771 +/- 0.0053
Time of Perihelion: 2463999.0615 +/- 8.4
Perihelion: 36.47069595 +/- 0.0085
Aphelion: 67.57401947 +/- 0.0103
Period (y) 375.2263 +/- 0.06
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -22.32338920 +/- 0.0003
Ecliptic Y -30.46863170 +/- 0.0004
Ecliptic Z 5.06906785 +/- 0.0001
Ecliptic XDOT 0.00248597 +/- 0.0000
Ecliptic YDOT -0.00147930 +/- 0.0000
Ecliptic ZDOT -0.00121362 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 38.10992879 +/- 0.0003
Geocenter to KBO 37.14023898 +/- 0.0005
# Hcoef: 8.52
The following table shows the complete astrometric record for 15KV174. 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 (15KV174) followed by the observatory code and reference code for the source of the astrometry.
2014 05 30.38544 15 31 52.700 -11 00 35.24 24.2r 15KV174 568 C~2lVL 2014 06 01.31224 15 31 42.906 -11 00 18.97 24.2r 15KV174 568 C~2lVL 2014 06 01.35552 15 31 42.673 -11 00 18.69 24.0r 15KV174 568 C~2lVL 2014 06 22.30986 15 30 05.734 -10 58 44.57 24.5r 15KV174 568 C~2lVL 2014 06 22.35268 15 30 05.561 -10 58 44.45 24.2r 15KV174 568 C~2lVL 2014 07 19.32576 15 28 42.774 -11 01 00.49 24.5r 15KV174 568 C~2lVL 2015 02 25.61666 15 43 22.540 -12 20 54.46 24.2r 15KV174 568 C~2lVL 2015 03 19.62043 15 42 59.546 -12 17 52.30 24.3r 15KV174 568 C~2lVL 2015 03 22.53917 15 42 52.822 -12 17 18.80 24.7r 15KV174 568 C~2lVL 2015 04 13.55184 15 41 38.717 -12 12 23.92 24.3r 15KV174 568 C~2lVL 2015 04 13.59295 15 41 38.541 -12 12 23.31 24.5r 15KV174 568 C~2lVL 2015 04 18.55634 15 41 16.978 -12 11 11.13 24.3r 15KV174 568 C~2lVL 2015 05 21.32236 15 38 30.782 -12 03 50.34 24.0r 15KV174 568 C~2lVL 2015 05 21.36353 15 38 30.560 -12 03 49.94 24.3r 15KV174 568 C~2lVL 2015 05 21.40471 15 38 30.344 -12 03 49.45 24.1r 15KV174 568 C~2lVL 2015 05 22.48134 15 38 24.596 -12 03 37.80 24.1r 15KV174 568 C~2lVL 2015 05 25.47177 15 38 08.744 -12 03 06.56 24.4r 15KV174 568 C~2lVL 2015 06 20.36123 15 36 01.756 -12 00 23.05 24.5r 15KV174 568 C~2lVL 2015 06 20.40209 15 36 01.572 -12 00 23.02 24.4r 15KV174 568 C~2lVL 2015 06 23.42230 15 35 48.768 -12 00 18.57 24.3r 15KV174 568 C~2lVL 2015 07 11.29546 15 34 46.000 -12 01 04.75 24.6r 15KV174 568 C~2lVL 2015 07 18.36550 15 34 28.265 -12 01 58.54 24.2r 15KV174 568 C~2lVL 2016 02 06.63317 15 48 46.929 -13 20 54.88 24.6w 15KV174 568 C~2lVL 2016 02 12.61871 15 48 59.214 -13 21 09.23 24.5w 15KV174 568 C~2lVL 2016 03 15.62688 15 48 58.808 -13 18 58.82 24.6w 15KV174 568 C~2lVL 2016 04 03.55069 15 48 09.404 -13 15 36.03 24.5w 15KV174 568 C~2lVL 2016 04 08.60024 15 47 51.012 -13 14 32.48 24.2w 15KV174 568 C~2lVL 2016 05 04.47406 15 45 52.071 -13 08 49.17 24.2w 15KV174 568 C~2lVL 2016 05 30.46201 15 43 33.840 -13 04 01.41 24.5w 15KV174 568 C~2lVL 2016 07 04.29818 15 40 56.368 -13 02 07.22 24.5w 15KV174 568 C~2lVL 2016 07 05.36646 15 40 52.707 -13 02 10.47 24.7w 15KV174 568 C~2lVL 2017 03 30.58199 15 54 23.750 -14 17 16.82 24.7w 15KV174 568 C~2lVL 2017 07 28.31194 15 45 52.170 -14 06 11.68 15KV174 568 C~2lVL 2017 08 19.27024 15 45 44.010 -14 11 33.68 24.5w 15KV174 568 C~2lVL 2017 08 19.27489 15 45 43.998 -14 11 33.73 24.7w 15KV174 568 C~2lVL 2017 08 25.27821 15 45 50.564 -14 13 30.85 24.7w 15KV174 568 C~2lVL 2017 08 26.25868 15 45 52.000 -14 13 51.17 24.2w 15KV174 568 C~2lVL 2017 08 26.26334 15 45 51.995 -14 13 51.24 24.5w 15KV174 568 C~2lVL
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 0.00 0.00 -0.02
2 0.0053 -143.86 0.03 -19.09 0.01
3 0.0054 -147.26 -0.10 -19.65 -0.09
4 0.0628 -1554.88 -0.04 -274.65 -0.04
5 0.0629 -1557.38 0.01 -275.15 0.07
6 0.1367 -2706.56 0.22 -704.34 0.15
7 0.7426 10997.35 -0.02 -2282.78 0.02
8 0.8028 10626.24 0.17 -2183.56 -0.08
9 0.8108 10522.32 -0.00 -2173.83 -0.06
10 0.8711 9394.55 -0.03 -2139.78 0.06
11 0.8712 9391.89 -0.03 -2139.79 0.07
12 0.8848 9066.96 -0.18 -2143.40 -0.04
13 0.9745 6590.61 -0.02 -2287.35 0.07
14 0.9746 6587.34 0.01 -2287.73 0.02
15 0.9747 6584.15 0.10 -2288.00 0.08
16 0.9777 6499.38 -0.05 -2296.59 -0.05
17 0.9859 6265.81 -0.03 -2321.18 0.00
18 1.0567 4415.92 -0.06 -2604.50 0.03
19 1.0569 4413.29 -0.09 -2605.11 -0.04
20 1.0651 4229.70 -0.06 -2645.57 0.01
21 1.1141 3346.16 0.04 -2910.43 0.01
22 1.1334 3106.35 -0.02 -3024.98 -0.05
23 1.6899 16467.23 -0.13 -4708.47 -0.21
24 1.7063 16646.28 0.04 -4681.88 0.05
25 1.7940 16610.62 0.12 -4555.70 -0.10
26 1.8458 15857.35 -0.03 -4521.09 0.03
27 1.8596 15579.73 0.08 -4520.04 0.07
28 1.9304 13800.86 0.02 -4581.51 -0.06
29 2.0016 11761.24 0.03 -4765.89 -0.12
30 2.0970 9490.32 0.00 -5189.58 0.07
31 2.0999 9438.95 0.08 -5205.25 -0.04
32 2.8342 22059.49 -0.01 -6925.38 0.06
33 3.1620 14598.77 0.05 -7944.00 0.04
34 3.2221 14557.19 0.16 -8285.94 -0.04
35 3.2221 14557.03 -0.06 -8286.03 -0.06
36 3.2386 14677.62 -0.02 -8378.73 0.08
37 3.2413 14702.76 -0.00 -8393.84 0.04
38 3.2413 14702.71 -0.17 -8393.92 0.02
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.
15KV174 quality flag:3 Type: SCATNEAR SCATNEAR SCATNEAR axisobj 51.671 51.683 51.659 ecceobj 0.297 0.297 0.296 incobj 23.289 23.289 23.289 qmin 35.135 35.010 35.134 qmax 69.749 69.797 69.717 amean 52.042 52.050 52.042 amin 51.518 51.490 51.518 amax 52.708 52.718 52.694 emean 0.306 0.307 0.306 emin 0.287 0.288 0.287 emax 0.324 0.325 0.324 imean 21.525 21.516 21.547 imin 20.824 20.842 20.841 imax 22.109 22.173 22.202 excite_mean 0.478 0.478 0.478 fracstop 1.000 1.000 1.000 cjmean 2.907 2.907 2.907 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 189.3 192.3 189.2 kozaiamp 180.0 179.8 180.0