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: 11UV410
# Created Thu Apr 25 01:13:46 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 32 observations of 32
# Arc: 8.09y
# First observation: 2005/09/28
# Last observation: 2013/11/01
# Chi-squared of fit: 13.65 DOF: 58 RMS: 0.12
# Min/Max residuals: -0.24 0.23
# Exact a, adot, b, bdot, g, gdot:
2.060727E-05 4.578423E-02 1.126311E-06 2.545454E-03 3.528576E-02 2.232871E-03
# Covariance matrix:
4.5569E-13 -1.6340E-13 6.0070E-15 -6.1234E-15 -6.2430E-14 -3.0495E-13
-1.6340E-13 1.3225E-13 -6.7054E-15 6.9290E-15 9.4393E-14 3.3892E-13
6.0070E-15 -6.7054E-15 3.5598E-13 -5.5198E-14 -4.8031E-15 -1.8624E-14
-6.1234E-15 6.9290E-15 -5.5198E-14 1.0089E-14 5.4218E-15 1.9144E-14
-6.2430E-14 9.4393E-14 -4.8031E-15 5.4218E-15 1.8848E-13 2.3548E-13
-3.0495E-13 3.3892E-13 -1.8624E-14 1.9144E-14 2.3548E-13 9.4292E-13
# lat0 lon0 xBary yBary zBary JD0
2.985529 14.443757 0.160923 0.051834 -0.991933 2453641.784087
# Heliocentric elements and errors
Epoch: 2453642.5000 = 2005/09/29
Mean Anomaly: 7.00473 +/- 0.003
Argument of Peri: 29.80498 +/- 0.006
Long of Asc Node: 332.20863 +/- 0.001
Inclination: 4.31364 +/- 0.000
Eccentricity: 0.25620733 +/- 0.0000
Semi-Major Axis: 39.24897682 +/- 0.0024
Time of Perihelion: 2451894.9497 +/- 0.9
Perihelion: 29.19310134 +/- 0.0023
Aphelion: 49.30485229 +/- 0.0033
Period (y) 245.8956 +/- 0.02
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X 28.40483327 +/- 0.0003
Ecliptic Y 7.15013759 +/- 0.0001
Ecliptic Z 1.47610275 +/- 0.0000
Ecliptic XDOT -0.00072649 +/- 0.0000
Ecliptic YDOT 0.00347415 +/- 0.0000
Ecliptic ZDOT 0.00020628 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 29.32808262 +/- 0.0003
Geocenter to KBO 28.34005251 +/- 0.0003
# Hcoef: 7.88
The following table shows the complete astrometric record for 11UV410. 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 (11UV410) followed by the observatory code and reference code for the source of the astrometry.
2005 09 28.283344 00 48 30.73 +08 26 43.8 22.5V 11UV410 645 C~1S7G 2005 09 28.284173 00 48 30.72 +08 26 43.8 22.3V 11UV410 645 C~1S7G 2005 09 28.286661 00 48 30.71 +08 26 43.7 23.3V 11UV410 645 C~1S7G 2008 11 02.362396 01 13 32.91 +11 27 35.4 22.5V 11UV410 645 C~1S7G 2008 11 02.363225 01 13 32.91 +11 27 35.4 21.9V 11UV410 645 C~1S7G 2008 11 02.365713 01 13 32.90 +11 27 35.3 23.1V 11UV410 645 C~1S7G 2011 08 29.51525 01 48 15.896 +15 05 36.54 22.6r 11UV410 568 C~1C6M 2011 08 29.55891 01 48 15.745 +15 05 36.14 22.7r 11UV410 568 C~1C6M 2011 08 29.60609 01 48 15.588 +15 05 35.74 22.7r 11UV410 568 C~1C6M 2011 09 05.54550 01 47 51.209 +15 04 13.01 22.7r 11UV410 568 C~1C6M 2011 10 24.42476 01 43 19.921 +14 42 35.96 22.5r 11UV410 568 C~1C6M 2011 10 24.46746 01 43 19.646 +14 42 34.48 22.5r 11UV410 568 C~1C6M 2011 10 24.51022 01 43 19.371 +14 42 32.98 22.5r 11UV410 568 C~1C6M 2011 10 29.32876 01 42 48.922 +14 39 44.54 22.4r 11UV410 568 C~1C6M 2011 11 24.21942 01 40 20.282 +14 25 02.73 22.6r 11UV410 568 C~1C6M 2011 11 24.22808 01 40 20.236 +14 25 02.48 22.6r 11UV410 568 C~1C6M 2011 11 24.23235 01 40 20.218 +14 25 02.36 22.6r 11UV410 568 C~1C6M 2011 11 26.44523 01 40 09.475 +14 23 53.82 22.7r 11UV410 568 C~1C6M 2012 01 24.22994 01 38 47.313 +14 10 04.55 22.7r 11UV410 568 C~1C6M 2012 01 25.24712 01 38 49.811 +14 10 11.52 22.7r 11UV410 568 C~1C6M 2012 01 26.23107 01 38 52.369 +14 10 18.95 11UV410 568 C~1C6M 2012 01 27.28902 01 38 55.236 +14 10 27.87 22.9r 11UV410 568 C~1C6M 2012 02 15.23915 01 40 10.345 +14 15 26.94 22.7r 11UV410 568 C~1C6M 2012 08 23.55493 01 58 00.002 +16 03 40.59 22.3r 11UV410 568 C~1C6M 2012 08 24.58617 01 57 57.595 +16 03 36.22 11UV410 568 C~1C6M 2012 10 17.41666 01 53 37.476 +15 45 18.50 22.5r 11UV410 568 C~1C6M 2012 10 20.51348 01 53 17.741 +15 43 37.40 22.5r 11UV410 568 C~1C6M 2013 02 06.28044 01 48 43.176 +15 10 08.40 22.8r 11UV410 568 C~1C6M 2013 02 06.28578 01 48 43.212 +15 10 08.59 22.8r 11UV410 568 C~1C6M 2013 11 01.50484 02 01 40.09 +16 34 18.6 11UV410 568 C~1CKy 2013 11 01.51119 02 01 40.05 +16 34 18.4 11UV410 568 C~1CKy 2013 11 01.51753 02 01 40.01 +16 34 18.2 11UV410 568 C~1CKy
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 -0.02 0.00 -0.00
2 0.0000 0.00 -0.09 0.00 0.03
3 0.0000 0.00 -0.01 0.00 0.01
4 3.0967 0.00 0.09 0.00 -0.11
5 3.0967 0.00 0.16 0.00 -0.08
6 3.0967 0.00 0.23 0.00 -0.09
7 5.9171 0.00 0.08 0.00 -0.00
8 5.9173 0.00 -0.05 0.00 0.01
9 5.9174 0.00 -0.09 0.00 0.07
10 5.9364 0.00 0.05 0.00 0.00
11 6.0702 0.00 -0.24 0.00 0.22
12 6.0703 0.00 -0.21 0.00 0.22
13 6.0704 0.00 -0.19 0.00 0.21
14 6.0836 0.00 -0.18 0.00 -0.06
15 6.1545 0.00 0.03 0.00 -0.00
16 6.1545 0.00 -0.00 0.00 0.02
17 6.1545 0.00 0.05 0.00 0.03
18 6.1606 0.00 0.07 0.00 0.22
19 6.3216 0.00 0.01 0.00 -0.07
20 6.3243 0.00 0.00 0.00 -0.05
21 6.3270 0.00 0.14 0.00 -0.11
22 6.3299 0.00 0.02 0.00 -0.03
23 6.3818 0.00 -0.06 0.00 0.14
24 6.9029 0.00 -0.07 0.00 -0.05
25 6.9057 0.00 0.07 0.00 -0.07
26 7.0531 0.00 -0.06 0.00 -0.08
27 7.0615 0.00 -0.11 0.00 -0.08
28 7.3593 0.00 -0.24 0.00 -0.24
29 7.3593 0.00 -0.00 0.00 -0.13
30 8.0937 0.00 0.14 0.00 -0.02
31 8.0937 0.00 0.16 0.00 -0.00
32 8.0937 0.00 0.17 0.00 0.01
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.
11UV410 quality flag:3 Type: 3:2E 3:2E 3:2E axisobj 39.831 39.831 39.831 ecceobj 0.267 0.267 0.267 incobj 4.305 4.305 4.305 qmin 28.501 28.501 28.501 qmax 51.052 51.052 51.052 amean 39.455 39.455 39.455 amin 39.011 39.011 39.011 amax 39.995 39.995 39.995 emean 0.235 0.235 0.235 emin 0.193 0.193 0.193 emax 0.277 0.277 0.277 imean 7.596 7.596 7.596 imin 4.530 4.530 4.530 imax 10.467 10.467 10.467 excite_mean 0.273 0.273 0.273 fracstop 1.000 1.000 1.000 cjmean 2.966 2.966 2.966 libcent 0 179.5 179.7 179.4 libamp 0 74.4 74.5 74.3 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 138.9 138.9 138.9 kozaiamp 180.0 180.0 180.0