Orbit Fit and Astrometric record for 05GV210

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: 05GV210   
# Created Tue Oct 24 01:37:36 2017
# Orbit generated from Bernstein formalism
# Fitting   26 observations of   27
# Arc:  15.19y
# First observation: 1999/03/22
#  Last observation: 2014/05/30
Preliminary a, adot, b, bdot, g, gdot:
   0.000959   0.023823   0.000144   0.005049   0.026952   0.000000
# WARNING -- MRQMIN stopped after  23 iterations
# Chi-squared of fit:    34.72 DOF:   46 RMS:  0.20
# Min/Max residuals:    -0.46    0.38
# Exact a, adot, b, bdot, g, gdot:
  1.601520E-05  2.459129E-02  4.011475E-06  5.213750E-03  2.577786E-02  4.318801E-03
# Covariance matrix:
  3.2241E-13 -7.3316E-14  2.7808E-14 -1.1815E-14  5.2317E-14 -1.6426E-13
 -7.3316E-14  2.5604E-14 -1.1766E-14  5.0181E-15 -1.0189E-14  6.9226E-14
  2.7808E-14 -1.1766E-14  2.0246E-13 -2.3843E-14  7.6090E-15 -3.6671E-14
 -1.1815E-14  5.0181E-15 -2.3843E-14  4.3892E-15 -2.9692E-15  1.5613E-14
  5.2317E-14 -1.0189E-14  7.6090E-15 -2.9692E-15  1.8265E-13 -4.8815E-14
 -1.6426E-13  6.9226E-14 -3.6671E-14  1.5613E-14 -4.8815E-14  2.1615E-13
#      lat0       lon0       xBary       yBary       zBary        JD0
    0.992004  179.271502   -0.034607    0.017136   -1.003830  2451259.794589
# Heliocentric elements and errors
Epoch:              2451250.5000  =  1999/03/13
Mean Anomaly:           86.51794 +/-     0.027
Argument of Peri:      258.48586 +/-     0.018
Long of Asc Node:      174.78538 +/-     0.000
Inclination:            12.05272 +/-     0.000
Eccentricity:         0.17246475 +/-    0.0000
Semi-Major Axis:     39.04089569 +/-    0.0027
Time of Perihelion: 2429837.2909 +/-       6.3
Perihelion:          32.30771722 +/-    0.0023
Aphelion:            45.77407416 +/-    0.0032
Period (y)              243.9427 +/-      0.03
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -39.78015728 +/-    0.0006
Ecliptic Y            0.47111819 +/-    0.0000
Ecliptic Z            0.67179767 +/-    0.0000
Ecliptic XDOT        -0.00048438 +/-    0.0000
Ecliptic YDOT        -0.00259704 +/-    0.0000
Ecliptic ZDOT         0.00056162 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   39.78861869 +/-    0.0006
Geocenter to KBO     38.79297839 +/-    0.0006
# Hcoef:  6.75

The following table shows the complete astrometric record for 05GV210. 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 (05GV210) followed by the observatory code and reference code for the source of the astrometry.

1999 03  22.293846 11 58 54.30   +01 11 59.7   22.2V 05GV210   645  C~1ReG      
1999 03  22.294676 11 58 54.30   +01 11 59.7   21.8V 05GV210   645  C~1ReG      
1999 03  22.297164 11 58 54.28   +01 11 59.8   23.3V 05GV210   645  C~1ReG      
2000 05  05.286629 12 01 26.81   +01 16 38.8         05GV210   645  C~1ReG      
2000 05  05.287458 12 01 26.81   +01 16 38.8         05GV210   645  C~1ReG      
2000 05  05.289946 12 01 26.80   +01 16 38.8         05GV210   645  C~1ReG      
2005 04  12.31912  12 30 17.86   -00 17 27.9   22.6R 05GV210   695  Cn7074      
2005 04  12.41792  12 30 17.39   -00 17 24.7         05GV210   695  Cn7074      
2005 06  09.05184  12 27 27.07   +00 00 52.8   22.4R 05GV210   304  Cn7074      
2005 06  09.09795  12 27 27.00   +00 00 53.0         05GV210   304  Cn7074      
2005 07  09.98321  12 27 40.75   -00 01 20.7   22.5R 05GV210   304  Cn8899      
2005 07  10.05676  12 27 40.89   -00 01 21.5         05GV210   304  Cn8899      
2006 02  23.28855  12 39 07.00   -00 59 12.9   23.0R 05GV210   304  Cq7104      
2006 02  23.30749  12 39 06.93   -00 59 12.5         05GV210   304  Cq7104      
2006 03  02.41041  12 38 40.60   -00 55 44.5   22.7R 05GV210   695  Cq7104      
2006 03  02.46280  12 38 40.40   -00 55 42.8         05GV210   695  Cq7104      
2006 03  02.51517  12 38 40.20   -00 55 41.4         05GV210   695  Cq7104      
2006 04  27.08891  12 34 38.15   -00 27 04.2   22.2R 05GV210   807  Cr3594      
2006 04  28.05971  12 34 34.34   -00 26 38.7         05GV210   807  Cr3594      
2006 04  28.15286  12 34 33.95   -00 26 36.6         05GV210   807  Cr3594      
2007 02  15.30393  12 44 50.10   -01 18 58.0         05GV210   304  Cu1516      
2007 02  15.34701  12 44 49.97   -01 18 56.9         05GV210   304  Cu1516      
2008 03  03.31572  12 49 07.94   -01 27 08.1         05GV210   695  Cy7595      
2008 03  03.37725  12 49 07.68   -01 27 06.7         05GV210   695  Cy7595      
2014 05  30.20082  13 13 58.97   -02 20 59.9   23.6R 05GV210   695  C~1LJP      
2014 05  30.30231  13 13 58.68   -02 20 58.6         05GV210   695  C~1LJP      
2014 05  30.34728  13 13 58.54   -02 20 58.1         05GV210   695  C~1LJP      

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    -0.19       0.00    -0.17
  2   0.0000      0.00    -0.13       0.00    -0.17
  3   0.0000     -0.31    -0.24      -0.03    -0.20
  4   1.1225   1987.24     0.24    1166.24     0.10
  5   1.1225   1987.24     0.28    1166.24     0.09
  6   1.1225   1987.10     0.27    1166.18     0.03
  7   6.0589  28233.01     0.14    6379.88     0.34
  8   6.0592  28225.12    -0.33    6379.99     0.37
  9   6.2170  25396.24 (   0.73)   6361.43 (   0.04)
 10   6.2171  25395.18     0.38    6361.19    -0.12
 11   6.3017  25641.39    -0.25    6321.01     0.06
 12   6.3019  25643.67    -0.14    6321.12     0.28
 13   6.9267  36723.46     0.05    7278.68     0.25
 14   6.9268  36722.30     0.08    7278.62     0.11
 15   6.9462  36263.14    -0.00    7311.35     0.01
 16   6.9464  36259.61     0.06    7311.71     0.17
 17   6.9465  36256.19     0.23    7311.79     0.04
 18   7.0987  32129.54    -0.15    7429.95    -0.46
 19   7.1013  32065.41    -0.13    7430.37    -0.04
 20   7.1016  32059.05    -0.27    7429.94    -0.42
 21   7.9042  42112.63     0.09    8276.47     0.05
 22   7.9043  42110.31     0.05    8276.70     0.05
 23   8.9501  46034.72     0.02    9407.66     0.16
 24   8.9503  46030.37    -0.11    9407.36    -0.38
 25  15.1893  69662.54     0.24   15740.83     0.06
 26  15.1896  69657.50     0.04   15740.22    -0.01
 27  15.1897  69655.12    -0.21   15739.80    -0.20

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.

05GV210    quality flag:3

Type:           3:2E      3:2E      3:2E

axisobj        39.096    39.105    39.088
ecceobj         0.173     0.173     0.173
incobj         12.046    12.046    12.046
qmin           31.897    31.892    31.921
qmax           47.587    47.656    47.565
amean          39.456    39.456    39.457
amin           38.992    39.004    38.979
amax           39.980    39.984    39.996
emean           0.173     0.173     0.172
emin            0.153     0.153     0.151
emax            0.192     0.193     0.191
imean          11.618    11.574    11.664
imin           11.024    10.957    11.087
imax           12.300    12.257    12.312
excite_mean     0.265     0.265     0.266
fracstop        1.000     1.000     1.000
cjmean          2.972     2.972     2.972

libcent 0       180.8     180.4     179.4
libamp  0        97.7      94.5     100.7
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       177.7     175.3     179.8
kozaiamp        179.9     180.0     180.0