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: 06QP180
# Created Fri Nov 22 02:08:52 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 76 observations of 76
# Arc: 13.38y
# First observation: 2002/07/22
# Last observation: 2015/12/07
# Chi-squared of fit: 54.58 DOF: 146 RMS: 0.15
# Min/Max residuals: -0.41 0.64
# Exact a, adot, b, bdot, g, gdot:
3.457119E-05 1.690276E-01 -7.785135E-07 2.819952E-03 7.891104E-02 3.210186E-02
# Covariance matrix:
6.9099E-13 -1.6652E-12 -3.5691E-15 6.1572E-14 1.0847E-12 -9.9184E-13
-1.6652E-12 3.2701E-11 3.7589E-14 -1.0052E-12 -1.3305E-12 1.6957E-11
-3.5691E-15 3.7589E-14 3.8242E-13 -7.4643E-14 -9.1490E-15 2.0896E-14
6.1572E-14 -1.0052E-12 -7.4643E-14 4.2692E-13 9.4717E-14 -5.3578E-13
1.0847E-12 -1.3305E-12 -9.1490E-15 9.4717E-14 4.5664E-12 -1.3902E-12
-9.9184E-13 1.6957E-11 2.0896E-14 -5.3578E-13 -1.3902E-12 9.0070E-12
# lat0 lon0 xBary yBary zBary JD0
5.195794 -44.200053 0.291510 0.088504 -0.974135 2452477.850013
# Heliocentric elements and errors
Epoch: 2452478.5000 = 2002/07/23
Mean Anomaly: 3.96430 +/- 0.146
Argument of Peri: 52.63457 +/- 0.000
Long of Asc Node: 237.79561 +/- 0.000
Inclination: 4.95469 +/- 0.000
Eccentricity: 0.65187047 +/- 0.0000
Semi-Major Axis: 37.83840240 +/- 0.0000
Time of Perihelion: 2451542.3152 +/- 34.5
Perihelion: 13.17266528 +/- 0.0002
Aphelion: 62.50413951 +/- 0.0003
Period (y) 232.7595 +/- 0.00
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X 9.54589045 +/- 0.0000
Ecliptic Y -9.68382845 +/- 0.0000
Ecliptic Z 1.14764327 +/- 0.0000
Ecliptic XDOT 0.00486952 +/- 0.0000
Ecliptic YDOT 0.00343471 +/- 0.0000
Ecliptic ZDOT 0.00019851 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 13.64608714 +/- 0.0000
Geocenter to KBO 12.67244392 +/- 0.0000
# Hcoef: 9.77
The following table shows the complete astrometric record for 06QP180. 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 (06QP180) followed by the observatory code and reference code for the source of the astrometry.
2002 07 22.34927 21 06 45.70 -11 07 59.5 21. R 06QP180 644 Cy2155 2002 07 22.38387 21 06 45.34 -11 08 00.5 06QP180 644 Cy2155 2002 08 16.30486 21 01 55.11 -11 28 01.3 21. R 06QP180 644 Cy2155 2002 08 17.28709 21 01 43.82 -11 28 53.0 21. R 06QP180 644 Cy2155 2006 08 28.25805 23 06 42.75 -00 17 36.7 22.4 06QP180 705 C62217 2006 08 28.25888 23 06 42.74 -00 17 36.7 23.7 06QP180 705 C62217 2006 09 11.26639 23 04 21.62 -00 32 34.2 21.9 06QP180 705 C62217 2006 09 11.26971 23 04 21.58 -00 32 34.5 22.7 06QP180 705 C62217 2006 09 18.26234 23 03 11.64 -00 40 26.5 21.9 06QP180 705 C62217 2006 09 18.26566 23 03 11.60 -00 40 26.8 23.2 06QP180 705 C62217 2006 09 20.23075 23 02 52.33 -00 42 40.4 22.2 06QP180 705 C62217 2006 09 20.23407 23 02 52.31 -00 42 40.7 23.4 06QP180 705 C62217 2006 09 29.28994 23 01 26.99 -00 52 51.9 21.9 06QP180 705 C62217 2006 09 29.29326 23 01 26.94 -00 52 52.4 23.0 06QP180 705 C62217 2006 10 01.21351 23 01 09.86 -00 54 59.4 22.1 06QP180 705 C62217 2006 10 01.21683 23 01 09.84 -00 54 59.7 22.9 06QP180 705 C62217 2006 10 03.27779 23 00 51.90 -00 57 14.8 22.1 06QP180 705 C62217 2006 10 03.27863 23 00 51.90 -00 57 14.7 23.2 06QP180 705 C62217 2006 10 12.21284 22 59 40.50 -01 06 36.4 22.5 06QP180 705 C62217 2006 10 12.21367 22 59 40.49 -01 06 36.4 23.9 06QP180 705 C62217 2006 10 14.26195 22 59 25.72 -01 08 38.6 22.2 06QP180 705 C62217 2006 10 14.26278 22 59 25.71 -01 08 38.8 23.4 06QP180 705 C62217 2006 10 20.20259 22 58 46.80 -01 14 14.9 22.3 06QP180 705 C62217 2006 10 20.20342 22 58 46.80 -01 14 14.9 23.7 06QP180 705 C62217 2007 07 12.39105 23 36 16.75 +02 28 23.2 06QP180 304 C~00AI 2007 07 12.44698 23 36 16.62 +02 28 22.9 06QP180 304 C~00AI 2007 10 13.29157 23 24 19.81 +01 15 46.4 22.4 06QP180 705 Cy0771 2007 10 13.29489 23 24 19.77 +01 15 45.9 23.4 06QP180 705 Cy0771 2007 10 15.29648 23 24 04.16 +01 13 41.2 22.3 06QP180 705 Cy0771 2007 10 15.29897 23 24 04.13 +01 13 40.8 23.4 06QP180 705 Cy0771 2007 10 20.28110 23 23 27.60 +01 08 40.3 22.2 06QP180 705 Cy0771 2007 10 20.28442 23 23 27.59 +01 08 40.0 23.1 06QP180 705 Cy0771 2007 11 04.20314 23 22 01.95 +00 55 36.2 22.7 06QP180 705 Cy0771 2007 11 04.20397 23 22 01.96 +00 55 36.1 24.0 06QP180 705 Cy0771 2007 11 07.16112 23 21 49.77 +00 53 26.0 22.5 06QP180 705 Cy0771 2007 11 07.16444 23 21 49.73 +00 53 25.9 23.7 06QP180 705 Cy0771 2007 11 09.20262 23 21 42.35 +00 52 01.8 22.4 06QP180 705 Cy0771 2007 11 09.20511 23 21 42.34 +00 52 01.9 23.7 06QP180 705 Cy0771 2007 11 11.19820 23 21 35.92 +00 50 44.2 22.5 06QP180 705 Cy0771 2007 11 11.20152 23 21 35.93 +00 50 44.0 23.8 06QP180 705 Cy0771 2007 11 12.20034 23 21 33.01 +00 50 07.0 22.5 06QP180 705 Cy0771 2007 11 12.20366 23 21 33.01 +00 50 06.8 23.6 06QP180 705 Cy0771 2008 10 02.205191 23 48 24.67 +03 36 41.7 22.1V 06QP180 645 C~1SL8 2008 10 02.206020 23 48 24.66 +03 36 41.6 21.7V 06QP180 645 C~1SL8 2008 10 02.208508 23 48 24.65 +03 36 41.5 24.4V 06QP180 645 C~1SL8 2013 08 08.57118 01 20 51.938 +11 48 10.56 23.1r 06QP180 568 C~2WXR 2013 08 08.57598 01 20 51.916 +11 48 10.50 23.4r 06QP180 568 C~2WXR 2013 08 08.62000 01 20 51.819 +11 48 10.24 23.1r 06QP180 568 C~2WXR 2013 09 01.54122 01 19 18.469 +11 40 54.73 23.2r 06QP180 568 C~2WXR 2013 09 01.58009 01 19 18.245 +11 40 53.61 23.2r 06QP180 568 C~2WXR 2013 09 02.52849 01 19 12.901 +11 40 25.24 23.1r 06QP180 568 C~2WXR 2013 09 02.57808 01 19 12.612 +11 40 23.82 23.1r 06QP180 568 C~2WXR 2014 07 25.50098 01 34 02.971 +12 47 26.86 23.3r 06QP180 568 C~2WXR 2014 07 25.54031 01 34 03.005 +12 47 27.25 23.3r 06QP180 568 C~2WXR 2014 07 25.58207 01 34 03.027 +12 47 27.58 23.3r 06QP180 568 C~2WXR 2014 08 23.54089 01 33 18.390 +12 45 35.94 23.2r 06QP180 568 C~2WXR 2014 08 23.58776 01 33 18.209 +12 45 35.09 23.0r 06QP180 568 C~2WXR 2014 08 27.43321 01 33 02.590 +12 44 21.02 23.2r 06QP180 568 C~2WXR 2014 08 27.52904 01 33 02.170 +12 44 19.01 23.4r 06QP180 568 C~2WXR 2014 09 18.37931 01 30 57.771 +12 33 23.03 23.1r 06QP180 568 C~2WXR 2014 09 18.42403 01 30 57.455 +12 33 21.31 23.2r 06QP180 568 C~2WXR 2014 09 23.46480 01 30 21.732 +12 30 00.92 22.9r 06QP180 568 C~2WXR 2014 09 27.42812 01 29 52.27 +12 27 13.3 23.2R 06QP180 695 C~1LJh 2014 09 27.48193 01 29 51.84 +12 27 10.9 06QP180 695 C~1LJh 2014 10 22.42102 01 26 32.295 +12 07 11.07 23.2r 06QP180 568 C~2WXR 2014 10 22.46044 01 26 31.968 +12 07 09.05 23.0r 06QP180 568 C~2WXR 2014 10 22.49986 01 26 31.646 +12 07 07.00 23.0r 06QP180 568 C~2WXR 2014 10 23.41580 01 26 24.247 +12 06 20.57 23.0r 06QP180 568 C~2WXR 2014 10 25.42089 01 26 08.087 +12 04 38.78 23.1r 06QP180 568 C~2WXR 2014 11 19.22807 01 23 06.783 +11 44 34.50 23.1r 06QP180 568 C~2WXR 2014 11 19.36118 01 23 05.935 +11 44 28.64 23.4r 06QP180 568 C~2WXR 2014 11 21.21074 01 22 54.560 +11 43 07.86 22.7r 06QP180 568 C~2WXR 2015 01 19.25297 01 21 13.562 +11 23 50.04 23.7r 06QP180 568 C~2WXR 2015 01 19.29899 01 21 13.713 +11 23 50.16 23.6r 06QP180 568 C~2WXR 2015 12 07.43675 01 34 05.962 +12 31 06.79 23.6w 06QP180 568 C~2WXR 2015 12 07.44917 01 34 05.904 +12 31 06.32 23.6w 06QP180 568 C~2WXR
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 -0.22 0.00 0.22
2 0.0001 0.00 0.30 0.00 0.64
3 0.0683 0.00 0.17 0.00 -0.41
4 0.0710 0.00 -0.18 0.00 -0.34
5 4.1011 0.00 -0.10 0.00 0.10
6 4.1011 0.00 -0.13 0.00 0.15
7 4.1394 0.00 -0.06 0.00 -0.12
8 4.1394 0.00 -0.14 0.00 -0.20
9 4.1586 0.00 0.03 0.00 0.01
10 4.1586 0.00 -0.07 0.00 -0.07
11 4.1639 0.00 0.05 0.00 -0.03
12 4.1640 0.00 0.24 0.00 -0.11
13 4.1887 0.00 0.01 0.00 0.07
14 4.1888 0.00 -0.29 0.00 -0.20
15 4.1940 0.00 0.03 0.00 0.02
16 4.1940 0.00 0.18 0.00 -0.06
17 4.1997 0.00 0.00 0.00 -0.11
18 4.1997 0.00 0.11 0.00 0.04
19 4.2241 0.00 0.06 0.00 0.13
20 4.2241 0.00 0.00 0.00 0.18
21 4.2297 0.00 -0.00 0.00 0.07
22 4.2297 0.00 -0.06 0.00 -0.08
23 4.2460 0.00 -0.16 0.00 0.08
24 4.2460 0.00 -0.08 0.00 0.13
25 4.9721 0.00 -0.03 0.00 0.27
26 4.9722 0.00 -0.07 0.00 -0.08
27 5.2264 0.00 -0.00 0.00 0.23
28 5.2264 0.00 -0.20 0.00 -0.06
29 5.2319 0.00 0.17 0.00 0.23
30 5.2319 0.00 0.02 0.00 -0.01
31 5.2455 0.00 -0.01 0.00 0.09
32 5.2455 0.00 0.19 0.00 -0.02
33 5.2864 0.00 -0.03 0.00 -0.04
34 5.2864 0.00 0.18 0.00 -0.11
35 5.2945 0.00 0.07 0.00 -0.09
36 5.2945 0.00 -0.33 0.00 -0.05
37 5.3001 0.00 -0.02 0.00 -0.08
38 5.3001 0.00 -0.04 0.00 0.12
39 5.3055 0.00 -0.15 0.00 0.01
40 5.3056 0.00 0.16 0.00 -0.06
41 5.3083 0.00 -0.06 0.00 0.06
42 5.3083 0.00 0.09 0.00 -0.02
43 6.1981 0.00 0.15 0.00 -0.21
44 6.1981 0.00 0.11 0.00 -0.26
45 6.1981 0.00 0.31 0.00 -0.19
46 11.0478 0.00 0.10 0.00 0.02
47 11.0478 0.00 -0.07 0.00 -0.01
48 11.0480 0.00 -0.05 0.00 0.01
49 11.1135 0.00 0.04 0.00 -0.01
50 11.1136 0.00 0.03 0.00 0.02
51 11.1162 0.00 0.04 0.00 -0.09
52 11.1163 0.00 0.07 0.00 -0.00
53 12.0086 0.00 -0.03 0.00 0.07
54 12.0087 0.00 0.07 0.00 0.05
55 12.0089 0.00 -0.02 0.00 -0.05
56 12.0881 0.00 0.02 0.00 -0.01
57 12.0883 0.00 0.08 0.00 -0.04
58 12.0988 0.00 -0.11 0.00 0.06
59 12.0991 0.00 0.03 0.00 0.04
60 12.1589 0.00 0.13 0.00 0.03
61 12.1590 0.00 0.09 0.00 -0.00
62 12.1728 0.00 0.05 0.00 0.01
63 12.1837 0.00 -0.11 0.00 0.55
64 12.1838 0.00 -0.37 0.00 0.50
65 12.2521 0.00 -0.03 0.00 -0.07
66 12.2522 0.00 -0.05 0.00 -0.08
67 12.2523 0.00 -0.00 0.00 -0.12
68 12.2548 0.00 0.04 0.00 -0.05
69 12.2603 0.00 0.01 0.00 0.06
70 12.3282 0.00 0.00 0.00 -0.08
71 12.3286 0.00 0.11 0.00 -0.07
72 12.3336 0.00 0.15 0.00 0.01
73 12.4953 0.00 -0.12 0.00 -0.08
74 12.4954 0.00 0.05 0.00 -0.35
75 13.3774 0.00 -0.09 0.00 0.03
76 13.3774 0.00 -0.13 0.00 -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.
06QP180 quality flag:3 Type: CENTAURR CENTAURR CENTAURR axisobj 38.232 38.232 38.232 ecceobj 0.655 0.655 0.655 incobj 4.955 4.955 4.955 qmin 13.011 13.011 13.011 qmax 65.288 64.974 65.247 amean 38.367 38.290 38.276 amin 37.829 37.856 37.549 amax 39.423 39.236 39.305 emean 0.653 0.652 0.652 emin 0.646 0.645 0.643 emax 0.659 0.660 0.660 imean 7.081 7.142 7.416 imin 6.092 6.092 6.092 imax 7.924 8.130 8.465 excite_mean 0.665 0.664 0.665 fracstop 0.004 0.005 0.005 cjmean 2.483 2.484 2.484 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 60.9 61.3 65.2 kozaiamp 9.5 8.5 14.5