Orbit Fit and Astrometric record for 15VV167

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: 15VV167   
# Created Wed May  8 01:17:33 2024
# Orbit generated from Bernstein formalism
# Fitting     27 observations of     27
# Arc:   2.35y
# First observation: 2015/08/11
#  Last observation: 2017/12/16
Preliminary a, adot, b, bdot, g, gdot:
  -0.000138   0.028085  -0.000017   0.005788   0.026424   0.000000
# Chi-squared of fit:     5.29 DOF:     48 RMS:  0.08
# Min/Max residuals:    -0.15    0.20
# Exact a, adot, b, bdot, g, gdot:
  1.725462E-05  2.750919E-02  3.206617E-06  5.667884E-03  2.604216E-02 -9.936973E-04
# Covariance matrix:
  2.1864E-13  3.3164E-14 -1.4399E-15  2.5722E-14  1.6284E-13  2.2790E-12
  3.3164E-14  4.7365E-13 -2.9158E-14  1.4408E-13  3.0433E-13  1.2406E-11
 -1.4399E-15 -2.9158E-14  1.0684E-13 -9.1756E-14 -1.8522E-14 -1.1741E-12
  2.5722E-14  1.4408E-13 -9.1756E-14  1.8203E-13  1.0720E-13  5.4280E-12
  1.6284E-13  3.0433E-13 -1.8522E-14  1.0720E-13  3.1783E-13  9.2843E-12
  2.2790E-12  1.2406E-11 -1.1741E-12  5.4280E-12  9.2843E-12  4.6609E-10
#      lat0       lon0       xBary       yBary       zBary        JD0
   -2.891702   50.700023    1.015168    0.002057    0.038289  2457246.085349
# Heliocentric elements and errors
Epoch:              2457240.5000  =  2015/08/06
Mean Anomaly:          337.87164 +/-     0.219
Argument of Peri:       15.44553 +/-     0.306
Long of Asc Node:       63.01980 +/-     0.001
Inclination:            11.93668 +/-     0.001
Eccentricity:         0.14469042 +/-    0.0004
Semi-Major Axis:     44.12428969 +/-    0.0052
Time of Perihelion: 2463821.0425 +/-      65.0
Perihelion:          37.73992758 +/-    0.0180
Aphelion:            50.50865180 +/-    0.0185
Period (y)              293.1061 +/-      0.05
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           25.04764895 +/-    0.0005
Ecliptic Y           29.00438287 +/-    0.0006
Ecliptic Z           -1.93702377 +/-    0.0000
Ecliptic XDOT        -0.00228711 +/-    0.0000
Ecliptic YDOT         0.00176796 +/-    0.0000
Ecliptic ZDOT         0.00060044 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   38.37174748 +/-    0.0006
Geocenter to KBO     38.39927840 +/-    0.0008
# Hcoef:  8.67

The following table shows the complete astrometric record for 15VV167. 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 (15VV167) followed by the observatory code and reference code for the source of the astrometry.

2015 08  11.58456  03 16 13.595  +15 08 15.50  24.6w 15VV167   568  C~2lVk      
2015 09  06.63168  03 16 11.225  +15 07 31.28  24.9w 15VV167   568  C~2lVk      
2015 09  12.52133  03 16 01.223  +15 06 46.04  24.6w 15VV167   568  C~2lVk      
2015 10  07.45992  03 14 44.378  +15 01 36.99  25.3w 15VV167   568  C~2lVk      
2015 10  08.46335  03 14 40.261  +15 01 21.36  24.4w 15VV167   568  C~2lVk      
2015 10  08.52236  03 14 40.009  +15 01 20.42  24.5w 15VV167   568  C~2lVk      
2015 11  07.36952  03 12 14.512  +14 52 33.79  24.3r 15VV167   568  C~2lVk      
2015 11  07.41164  03 12 14.286  +14 52 33.05  24.2r 15VV167   568  C~2lVk      
2015 11  07.45387  03 12 14.057  +14 52 32.27  24.2r 15VV167   568  C~2lVk      
2015 11  17.38710  03 11 20.696  +14 49 32.44  24.9w 15VV167   568  C~2lVk      
2015 11  17.43381  03 11 20.457  +14 49 31.57  25.5w 15VV167   568  C~2lVk      
2015 12  06.39596  03 09 42.774  +14 44 26.22  24.6w 15VV167   568  C~2lVk      
2015 12  13.33048  03 09 10.550  +14 42 55.21  24.7w 15VV167   568  C~2lVk      
2015 12  13.38903  03 09 10.293  +14 42 54.51  25.0w 15VV167   568  C~2lVk      
2016 01  01.38342  03 07 58.439  +14 40 07.10  24.6w 15VV167   568  C~2lVk      
2016 01  02.34977  03 07 55.550  +14 40 02.32  24.7w 15VV167   568  C~2lVk      
2016 01  07.33018  03 07 42.019  +14 39 43.32  24.6w 15VV167   568  C~2lVk      
2016 02  05.27611  03 07 12.720  +14 41 29.13  25.0w 15VV167   568  C~2lVk      
2016 02  10.29646  03 07 16.701  +14 42 25.40  25.9w 15VV167   568  C~2lVk      
2016 09  07.56785  03 22 11.487  +15 51 03.55  24.7w 15VV167   568  C~2lVk      
2016 09  27.50655  03 21 23.874  +15 47 59.34  24.8w 15VV167   568  C~2lVk      
2017 01  02.42106  03 13 54.492  +15 24 43.89  24.7w 15VV167   568  C~2lVk      
2017 01  26.29235  03 13 10.028  +15 24 37.93  24.8w 15VV167   568  C~2lVk      
2017 01  26.30729  03 13 10.022  +15 24 38.07  24.7w 15VV167   568  C~2lVk      
2017 01  26.33541  03 13 10.004  +15 24 38.23  24.4w 15VV167   568  C~2lVk      
2017 12  16.35926  03 21 06.495  +16 11 35.15  24.2w 15VV167   568  C~2lVk      
2017 12  16.37785  03 21 06.397  +16 11 34.87  24.6w 15VV167   568  C~2lVk      

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    -0.11       0.00     0.05
     2   0.0713    -44.67    -0.15     -33.73     0.18
     3   0.0874   -196.30    -0.04     -39.58     0.05
     4   0.1557  -1351.44     0.07     -46.30    -0.14
     5   0.1585  -1413.10     0.01     -45.72    -0.05
     6   0.1586  -1416.87    -0.03     -45.66    -0.05
     7   0.2403  -3590.02     0.08       3.13    -0.01
     8   0.2405  -3593.37     0.13       3.28     0.00
     9   0.2406  -3596.78     0.15       3.41    -0.00
    10   0.2678  -4390.73    -0.01      35.73     0.01
    11   0.2679  -4394.30     0.20      35.81    -0.09
    12   0.3198  -5842.02    -0.02     120.14    -0.05
    13   0.3388  -6317.19    -0.05     157.94    -0.01
    14   0.3390  -6320.97     0.08     158.27    -0.04
    15   0.3910  -7371.27    -0.10     277.88    -0.05
    16   0.3936  -7412.98    -0.15     284.60     0.05
    17   0.4072  -7607.42    -0.13     319.37    -0.00
    18   0.4865  -7988.65     0.08     536.40     0.11
    19   0.5002  -7917.71    -0.03     574.96     0.08
    20   1.0759   5661.73     0.01    1148.64    -0.00
    21   1.1305   4949.87    -0.00    1145.49     0.01
    22   1.3959  -1683.19     0.02    1481.78    -0.03
    23   1.4612  -2305.02    -0.06    1645.80    -0.07
    24   1.4613  -2305.06     0.02    1645.96    -0.02
    25   1.4613  -2305.27     0.06    1646.18     0.00
    26   2.3485   5069.29     0.08    2578.92     0.03
    27   2.3485   5067.85    -0.12    2579.01     0.02

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.

15VV167    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        44.573    44.581    44.564
ecceobj         0.150     0.150     0.150
incobj         11.906    11.906    11.906
qmin           37.017    37.046    36.948
qmax           51.628    51.615    51.777
amean          44.187    44.187    44.187
amin           43.806    43.807    43.808
amax           44.595    44.602    44.625
emean           0.146     0.146     0.148
emin            0.133     0.134     0.134
emax            0.158     0.158     0.161
imean          10.349    10.313    10.248
imin            9.672     9.603     9.515
imax           10.981    10.969    10.895
excite_mean     0.231     0.231     0.231
fracstop        1.000     1.000     1.000
cjmean          3.039     3.039     3.039

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       173.6     174.8     172.8
kozaiamp        180.0     180.0     179.9