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: 15RS279
# Created Wed May 8 01:17:18 2024
# Orbit generated from Bernstein formalism
# Fitting 36 observations of 36
# Arc: 2.50y
# First observation: 2015/06/23
# Last observation: 2017/12/23
Preliminary a, adot, b, bdot, g, gdot:
-0.000065 0.020221 0.000002 0.000078 0.022098 0.000000
# Chi-squared of fit: 8.59 DOF: 66 RMS: 0.09
# Min/Max residuals: -0.22 0.30
# Exact a, adot, b, bdot, g, gdot:
1.474950E-05 1.980145E-02 7.017549E-08 7.653010E-05 2.174717E-02 2.653033E-04
# Covariance matrix:
1.7082E-13 2.7420E-14 -1.6185E-15 1.0136E-15 1.4519E-13 2.4832E-12
2.7420E-14 2.7171E-13 -2.7599E-15 3.2290E-15 2.3642E-13 8.6468E-12
-1.6185E-15 -2.7599E-15 9.0647E-14 -6.0196E-14 -3.6632E-15 -1.0601E-13
1.0136E-15 3.2290E-15 -6.0196E-14 7.0729E-14 3.4031E-15 1.5088E-13
1.4519E-13 2.3642E-13 -3.6632E-15 3.4031E-15 3.2036E-13 8.8812E-12
2.4832E-12 8.6468E-12 -1.0601E-13 1.5088E-13 8.8812E-12 4.1108E-10
# lat0 lon0 xBary yBary zBary JD0
0.675475 9.882257 1.006234 -0.001588 0.142870 2457197.098238
# Heliocentric elements and errors
Epoch: 2457190.5000 = 2015/06/17
Mean Anomaly: 193.98409 +/- 1.281
Argument of Peri: 237.66943 +/- 1.282
Long of Asc Node: 298.07405 +/- 0.058
Inclination: 0.71853 +/- 0.000
Eccentricity: 0.04256688 +/- 0.0002
Semi-Major Axis: 44.02506054 +/- 0.0025
Time of Perihelion: 2506393.9542 +/- 379.6
Perihelion: 42.15105122 +/- 0.0112
Aphelion: 45.89906985 +/- 0.0112
Period (y) 292.1179 +/- 0.02
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X 45.32597542 +/- 0.0012
Ecliptic Y 6.87592635 +/- 0.0002
Ecliptic Z 0.54215190 +/- 0.0000
Ecliptic XDOT -0.00039751 +/- 0.0000
Ecliptic YDOT 0.00245538 +/- 0.0000
Ecliptic ZDOT 0.00001009 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 45.84775174 +/- 0.0012
Geocenter to KBO 45.98298706 +/- 0.0012
# Hcoef: 8.00
The following table shows the complete astrometric record for 15RS279. 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 (15RS279) followed by the observatory code and reference code for the source of the astrometry.
2015 06 23.59746 00 35 15.558 +04 32 08.38 24.9r 15RS279 568 C~2nvn 2015 07 14.54188 00 35 26.656 +04 33 40.62 25.0r 15RS279 568 C~2nvn 2015 07 19.50673 00 35 24.233 +04 33 30.21 24.6r 15RS279 568 C~2nvn 2015 08 11.49525 00 34 49.155 +04 30 07.15 24.4r 15RS279 568 C~2nvn 2015 08 11.53687 00 34 49.057 +04 30 07.15 24.5r 15RS279 568 C~2nvn 2015 09 08.40090 00 33 22.668 +04 21 12.41 24.7r 15RS279 568 C~2nvn 2015 09 08.50503 00 33 22.271 +04 21 10.07 24.6r 15RS279 568 C~2nvn 2015 09 08.54864 00 33 22.101 +04 21 08.98 24.5r 15RS279 568 C~2nvn 2015 09 09.52421 00 33 18.449 +04 20 45.92 24.6w 15RS279 568 C~2nvn 2015 09 10.46510 00 33 14.890 +04 20 23.54 24.7w 15RS279 568 C~2nvn 2015 09 16.45310 00 32 51.592 +04 17 56.66 24.9w 15RS279 568 C~2nvn 2015 10 03.37987 00 31 42.286 +04 10 35.19 25.8w 15RS279 568 C~2nvn 2015 10 07.34557 00 31 25.834 +04 08 49.63 24.2r 15RS279 568 C~2nvn 2015 10 07.36748 00 31 25.745 +04 08 49.20 24.8r 15RS279 568 C~2nvn 2015 10 07.40358 00 31 25.592 +04 08 48.23 24.6r 15RS279 568 C~2nvn 2015 11 07.24449 00 29 29.051 +03 56 10.03 24.9w 15RS279 568 C~2nvn 2015 11 07.29726 00 29 28.875 +03 56 08.96 24.9w 15RS279 568 C~2nvn 2015 11 10.38064 00 29 19.269 +03 55 05.36 24.5w 15RS279 568 C~2nvn 2015 12 07.32092 00 28 21.133 +03 48 30.92 24.7w 15RS279 568 C~2nvn 2016 01 01.24995 00 28 17.214 +03 47 41.99 24.7w 15RS279 568 C~2nvn 2016 09 05.58308 00 37 46.296 +04 49 33.77 24.7w 15RS279 568 C~2nvn 2016 09 06.53219 00 37 42.841 +04 49 12.02 24.9w 15RS279 568 C~2nvn 2016 09 06.57428 00 37 42.684 +04 49 11.21 24.8w 15RS279 568 C~2nvn 2016 09 26.55688 00 36 23.902 +04 40 54.94 25.0w 15RS279 568 C~2nvn 2016 09 26.57954 00 36 23.815 +04 40 54.41 24.9w 15RS279 568 C~2nvn 2016 09 27.48878 00 36 20.055 +04 40 30.45 24.6w 15RS279 568 C~2nvn 2016 11 03.39726 00 33 54.473 +04 24 52.44 24.7w 15RS279 568 C~2nvn 2016 11 03.46220 00 33 54.245 +04 24 51.17 25.0w 15RS279 568 C~2nvn 2016 12 29.23783 00 32 25.981 +04 14 39.96 24.1w 15RS279 568 C~2nvn 2017 01 03.25288 00 32 30.057 +04 15 01.08 24.1w 15RS279 568 C~2nvn 2017 01 28.23385 00 33 20.696 +04 20 02.77 15RS279 568 C~2nvn 2017 01 30.24057 00 33 26.825 +04 20 40.34 24.5w 15RS279 568 C~2nvn 2017 09 16.51863 00 41 22.343 +05 12 49.77 24.9w 15RS279 568 C~2nvn 2017 09 22.47204 00 40 58.486 +05 10 19.95 24.6w 15RS279 568 C~2nvn 2017 11 22.37200 00 37 14.548 +04 46 16.29 25.4w 15RS279 568 C~2nvn 2017 12 23.31121 00 36 35.563 +04 41 39.85 25.0w 15RS279 568 C~2nvn
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 -0.00
2 0.0573 188.85 0.03 19.59 -0.12
3 0.0709 151.44 0.00 24.25 -0.06
4 0.1339 -410.68 -0.07 43.76 -0.22
5 0.1340 -412.03 0.19 44.34 0.30
6 0.2103 -1810.23 -0.07 61.09 0.04
7 0.2106 -1816.61 -0.03 61.27 0.13
8 0.2107 -1819.38 -0.11 61.27 0.09
9 0.2134 -1878.67 0.03 61.58 -0.00
10 0.2159 -1936.42 0.05 61.97 0.03
11 0.2323 -2314.62 0.04 64.18 0.10
12 0.2787 -3441.67 0.03 66.93 -0.06
13 0.2895 -3709.56 -0.13 66.95 -0.04
14 0.2896 -3710.96 -0.03 67.08 0.08
15 0.2897 -3713.44 -0.05 67.09 0.08
16 0.3741 -5615.88 0.10 58.40 -0.06
17 0.3743 -5618.72 0.07 58.45 -0.00
18 0.3827 -5776.03 0.09 56.78 -0.10
19 0.4565 -6732.02 -0.05 38.07 -0.01
20 0.5247 -6805.31 -0.04 16.29 -0.11
21 1.2046 2483.14 0.04 76.46 0.03
22 1.2072 2427.10 -0.06 76.71 -0.13
23 1.2073 2424.62 -0.00 76.88 0.01
24 1.2620 1146.57 -0.04 82.70 -0.05
25 1.2621 1145.16 0.09 82.73 -0.04
26 1.2646 1084.06 0.02 82.77 -0.09
27 1.3656 -1286.32 -0.12 76.12 -0.08
28 1.3658 -1289.95 -0.08 76.30 0.11
29 1.5185 -2744.29 -0.08 34.29 0.03
30 1.5323 -2679.92 0.04 29.68 -0.08
31 1.6006 -1864.77 0.15 8.68 0.08
32 1.6061 -1765.70 0.17 7.13 0.06
33 2.2339 6001.83 0.05 96.56 0.05
34 2.2502 5614.93 0.02 98.06 0.02
35 2.4169 1969.10 -0.04 81.01 -0.03
36 2.5016 1324.54 -0.11 55.54 0.04
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.
15RS279 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 44.448 44.455 44.440 ecceobj 0.032 0.032 0.033 incobj 0.719 0.719 0.719 qmin 41.684 41.734 41.663 qmax 46.976 46.962 47.001 amean 44.225 44.233 44.218 amin 43.882 43.891 43.872 amax 44.580 44.580 44.568 emean 0.039 0.039 0.039 emin 0.024 0.024 0.024 emax 0.054 0.054 0.055 imean 2.459 2.460 2.459 imin 1.798 1.800 1.796 imax 2.983 2.981 2.984 excite_mean 0.059 0.058 0.059 fracstop 1.000 1.000 1.000 cjmean 3.100 3.100 3.100 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 175.2 175.1 175.6 kozaiamp 179.9 180.0 180.0