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: 10FH92 # Created Wed Apr 24 01:13:17 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 40 observations of 41 # Arc: 4.58y # First observation: 2010/03/17 # Last observation: 2014/10/16 # Chi-squared of fit: 365.31 DOF: 74 RMS: 0.53 # Min/Max residuals: -1.16 1.58 # Exact a, adot, b, bdot, g, gdot: 2.553651E-05 2.967625E-01 4.557055E-05 5.291839E-01 1.754055E-01 4.845518E-02 # Covariance matrix: 5.6537E-13 -9.1551E-13 1.0807E-12 -1.6861E-12 -2.8255E-12 -5.7855E-13 -9.1551E-13 2.1483E-11 -2.5214E-12 -5.3832E-12 6.6323E-12 -3.3107E-12 1.0807E-12 -2.5214E-12 3.5597E-12 -5.4848E-12 -8.7416E-12 -1.8765E-12 -1.6861E-12 -5.3832E-12 -5.4848E-12 1.2439E-10 1.3677E-11 5.1566E-11 -2.8255E-12 6.6323E-12 -8.7416E-12 1.3677E-11 2.2856E-11 4.6988E-12 -5.7855E-13 -3.3107E-12 -1.8765E-12 5.1566E-11 4.6988E-12 2.5334E-11 # lat0 lon0 xBary yBary zBary JD0 -40.710716 -93.538894 0.999083 0.002320 0.002709 2455272.740001 # Heliocentric elements and errors Epoch: 2455272.5000 = 2010/03/17 Mean Anomaly: 359.92944 +/- 0.000 Argument of Peri: 313.99400 +/- 0.000 Long of Asc Node: 280.18450 +/- 0.000 Inclination: 61.82804 +/- 0.000 Eccentricity: 0.76375764 +/- 0.0000 Semi-Major Axis: 24.49180620 +/- 0.0000 Time of Perihelion: 2455281.1777 +/- 0.0 Perihelion: 5.78600222 +/- 0.0000 Aphelion: 43.19761019 +/- 0.0000 Period (y) 121.2103 +/- 0.00 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X -1.25962587 +/- 0.0000 Ecliptic Y -4.25069129 +/- 0.0000 Ecliptic Z -3.71827496 +/- 0.0000 Ecliptic XDOT 0.00425756 +/- 0.0000 Ecliptic YDOT -0.00622942 +/- 0.0000 Ecliptic ZDOT 0.00576773 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 5.78624436 +/- 0.0000 Geocenter to KBO 5.70104187 +/- 0.0000 # Hcoef: 11.39
The following table shows the complete astrometric record for 10FH92. 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 (10FH92) followed by the observatory code and reference code for the source of the astrometry.
2010 03 17.239235 17 35 25.55 -64 04 28.4 10FH92 C51 S~0GE1 2010 03 17.371539 17 35 29.07 -64 04 45.0 10FH92 C51 S~0GE1 2010 03 17.503843 17 35 32.42 -64 05 00.5 10FH92 C51 S~0U0z 2010 03 17.570059 17 35 34.19 -64 05 08.7 10FH92 C51 S~0U0z 2010 03 17.63627 17 35 35.85 -64 05 16.1 10FH92 C51 S~0GE1 2010 03 17.702362 17 35 37.49 -64 05 24.0 10FH92 C51 S~0GE1 2010 03 17.76858 17 35 39.21 -64 05 31.8 10FH92 C51 S~0U0z 2010 03 17.83467 17 35 40.89 -64 05 40.6 10FH92 C51 S~0GE1 2010 03 17.900882 17 35 42.58 -64 05 47.8 10FH92 C51 S~0GE1 2010 03 18.03319 17 35 45.96 -64 06 04.3 10FH92 C51 S~0U0z 2010 03 18.09940 17 35 47.56 -64 06 11.3 10FH92 C51 S~0U0z 2010 03 18.23171 17 35 51.02 -64 06 25.8 10FH92 C51 S~0GE1 2010 03 18.496314 17 35 57.382 -64 06 58.97 10FH92 C51 S~2gmv 2010 04 10.313115 17 38 27.217 -64 46 51.02 19.1R 10FH92 809 C~0GXI 2010 04 10.321771 17 38 27.107 -64 46 51.73 19.1R 10FH92 809 C~0GXI 2010 04 10.330371 17 38 26.983 -64 46 52.46 19.1R 10FH92 809 C~0GXI 2010 04 10.52031 17 38 24.78 -64 47 07.6 19.4R 10FH92 467 C~0GE1 2010 04 10.53135 17 38 24.64 -64 47 08.8 19.5R 10FH92 467 C~0GE1 2010 04 10.54301 17 38 24.47 -64 47 09.7 19.6R 10FH92 467 C~0GE1 2010 04 11.47628 17 38 12.30 -64 48 22.8 19.2R 10FH92 467 C~0GE1 2010 04 11.48727 17 38 12.14 -64 48 23.7 19.4R 10FH92 467 C~0GE1 2010 04 11.50250 17 38 11.94 -64 48 25.1 19.7R 10FH92 467 C~0GE1 2010 05 13.63760 17 17 42.73 -64 44 42.3 18.5R 10FH92 D90 C~0SWL 2010 05 13.64115 17 17 42.51 -64 44 41.5 18.5R 10FH92 D90 C~0SWL 2010 05 13.64470 17 17 42.34 -64 44 40.8 18.4R 10FH92 D90 C~0SWL 2010 06 02.64970 16 56 34.55 -63 32 09.1 10FH92 D90 C~0SWL 2010 06 02.65101 16 56 34.39 -63 32 08.7 10FH92 D90 C~0SWL 2010 06 02.66267 16 56 33.70 -63 32 05.4 18.9R 10FH92 D90 C~0SWL 2012 04 11.58849 19 37 36.92 -09 31 00.8 20.1R 10FH92 F65 C~0g7X 2012 04 11.59719 19 37 36.97 -09 30 58.5 10FH92 F65 C~0g7X 2012 04 23.392317 19 37 58.06 -08 32 59.4 20.3V 10FH92 H21 C~0g7X 2012 04 23.401458 19 37 58.04 -08 32 56.7 20.5V 10FH92 H21 C~0g7X 2012 04 23.411834 19 37 57.98 -08 32 53.9 20.0V 10FH92 H21 C~0g7X 2012 06 10.49022 19 26 45.992 -05 03 31.15 20.2r 10FH92 F51 C~0hJz 2012 06 10.50024 19 26 45.728 -05 03 29.06 20.2r 10FH92 F51 C~0hJz 2012 06 10.51100 19 26 45.456 -05 03 26.59 20.0i 10FH92 F51 C~0hJz 2012 06 10.52186 19 26 45.179 -05 03 24.23 19.8i 10FH92 F51 C~0hJz 2012 06 25.28345 19 20 11.54 -04 14 59.8 20.1V 10FH92 H06 C~0hfQ 2012 06 25.28600 19 20 11.47 -04 14 59.7 20.4V 10FH92 H06 C~0hfQ 2014 10 16.09633 19 39 32.03 +22 10 48.8 10FH92 291 C~1AZ1 2014 10 16.13690 19 39 32.15 +22 10 42.9 10FH92 291 C~1AZ1
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 0.63 0.00 0.43
2 0.0004 0.00 1.58 0.00 -0.40
3 0.0007 0.00 0.38 0.00 -0.14
4 0.0009 0.00 1.32 0.00 -0.46
5 0.0011 0.00 0.71 0.00 0.03
6 0.0013 0.00 -0.06 0.00 -0.00
7 0.0014 0.00 0.42 0.00 0.08
8 0.0016 0.00 0.45 0.00 -0.86
9 0.0018 0.00 0.68 0.00 -0.18
10 0.0022 0.00 1.47 0.00 -0.95
11 0.0024 0.00 0.64 0.00 -0.08
12 0.0027 0.00 ( 3.21) 0.00 ( 1.15)
13 0.0034 0.00 1.17 0.00 -0.60
14 0.0659 0.00 -0.29 0.00 0.21
15 0.0659 0.00 -0.22 0.00 0.23
16 0.0660 0.00 -0.37 0.00 0.22
17 0.0665 0.00 -0.61 0.00 -0.35
18 0.0665 0.00 -0.58 0.00 -0.59
19 0.0665 0.00 -0.86 0.00 -0.48
20 0.0691 0.00 -0.71 0.00 -0.34
21 0.0691 0.00 -0.77 0.00 -0.31
22 0.0692 0.00 -0.51 0.00 -0.43
23 0.1571 0.00 0.15 0.00 0.37
24 0.1572 0.00 0.03 0.00 0.74
25 0.1572 0.00 0.66 0.00 1.02
26 0.2119 0.00 -0.05 0.00 0.71
27 0.2119 0.00 -1.16 0.00 0.69
28 0.2120 0.00 0.05 0.00 0.28
29 2.0708 0.00 0.09 0.00 -0.04
30 2.0708 0.00 0.24 0.00 -0.32
31 2.1031 0.00 0.16 0.00 -0.20
32 2.1031 0.00 0.11 0.00 -0.17
33 2.1031 0.00 -0.50 0.00 -0.39
34 2.2348 0.00 0.17 0.00 -0.02
35 2.2348 0.00 -0.00 0.00 -0.09
36 2.2348 0.00 -0.02 0.00 0.05
37 2.2349 0.00 -0.07 0.00 0.07
38 2.2753 0.00 0.09 0.00 0.50
39 2.2753 0.00 0.14 0.00 0.15
40 4.5828 0.00 -0.06 0.00 0.21
41 4.5829 0.00 0.01 0.00 -0.10
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.
10FH92 quality flag:3 Type: CENTAURR CENTAURR CENTAURR axisobj 24.474 24.474 24.475 ecceobj 0.763 0.763 0.763 incobj 61.782 61.782 61.782 qmin 4.928 4.745 5.668 qmax 44.105 45.429 43.148 amean 22.185 23.449 22.949 amin 18.527 21.166 21.422 amax 24.896 25.591 24.475 emean 0.752 0.773 0.749 emin 0.731 0.753 0.732 emax 0.772 0.801 0.763 imean 63.463 62.838 63.608 imin 63.007 61.227 63.348 imax 64.057 63.728 63.896 excite_mean 1.169 1.178 1.167 fracstop 0.006 0.009 0.001 cjmean 1.872 1.798 1.830 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 299.8 293.1 312.3 kozaiamp 15.3 21.0 1.6