Orbit Fit and Astrometric record for 13VW71

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: 13VW71    
# Created Tue Apr  1 01:09:54 2025
# Orbit generated from Bernstein formalism
# Fitting     23 observations of     23
# Arc:   4.91y
# First observation: 2013/10/13
#  Last observation: 2018/09/09
Preliminary a, adot, b, bdot, g, gdot:
  -0.000059   0.022459  -0.000004   0.000302   0.023851   0.000000
# Chi-squared of fit:    10.57 DOF:     40 RMS:  0.12
# Min/Max residuals:    -0.23    0.22
# Exact a, adot, b, bdot, g, gdot:
  1.507519E-05  2.240245E-02  7.470285E-07  3.010897E-04  2.341715E-02 -2.071273E-04
# Covariance matrix:
  2.9823E-13 -1.6979E-13  8.1118E-16 -1.4255E-15 -3.6068E-14 -9.8408E-13
 -1.6979E-13  2.3127E-13 -1.9015E-15  2.8957E-15  1.3576E-13  1.9684E-12
  8.1118E-16 -1.9015E-15  2.4149E-13 -6.3720E-14 -3.1128E-15 -1.8970E-14
 -1.4255E-15  2.8957E-15 -6.3720E-14  2.2870E-14  2.4664E-15  2.7660E-14
 -3.6068E-14  1.3576E-13 -3.1128E-15  2.4664E-15  4.8355E-13  1.4957E-12
 -9.8408E-13  1.9684E-12 -1.8970E-14  2.7660E-14  1.4957E-12  1.8704E-11
#      lat0       lon0       xBary       yBary       zBary        JD0
   -1.422114    2.054883   -0.300433   -0.023493   -0.950816  2456578.598308
# Heliocentric elements and errors
Epoch:              2456570.5000  =  2013/10/05
Mean Anomaly:          338.08755 +/-     0.816
Argument of Peri:      321.69667 +/-     0.838
Long of Asc Node:       63.16844 +/-     0.012
Inclination:             1.59485 +/-     0.000
Eccentricity:         0.01236793 +/-    0.0001
Semi-Major Axis:     44.16106747 +/-    0.0049
Time of Perihelion: 2463094.9857 +/-     243.1
Perihelion:          43.61488656 +/-    0.0068
Aphelion:            44.70724838 +/-    0.0069
Period (y)              293.4726 +/-      0.05
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           43.60233424 +/-    0.0013
Ecliptic Y            1.86816187 +/-    0.0001
Ecliptic Z           -1.05982079 +/-    0.0000
Ecliptic XDOT        -0.00012340 +/-    0.0000
Ecliptic YDOT         0.00261525 +/-    0.0000
Ecliptic ZDOT         0.00003593 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   43.65520358 +/-    0.0013
Geocenter to KBO     42.70373599 +/-    0.0013
# Hcoef:  6.95

The following table shows the complete astrometric record for 13VW71. 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 (13VW71) followed by the observatory code and reference code for the source of the astrometry.

2013 10  13.09753  00 09 48.191  -00 29 15.64  23.2z 13VW71    W84  C~55OH      
2013 10  13.114352 00 09 48.12   -00 29 16.0   22.9i 13VW71    W84  C~55OH      
2013 11  08.140185 00 08 15.42   -00 38 42.9   23.5r 13VW71    W84  C~55OH      
2013 11  23.095000 00 07 39.81   -00 42 05.5   22.9i 13VW71    W84  C~55OH      
2014 08  18.307326 00 18 12.95   +00 26 40.8   23.2i 13VW71    W84  C~55OH      
2014 10  02.252106 00 15 15.73   +00 07 13.5   23.2i 13VW71    W84  C~55OH      
2014 11  15.10154  00 12 36.147  -00 09 09.34  23.1z 13VW71    W84  C~55OH      
2016 09  09.32882  00 26 12.041  +01 20 30.17  23.4i 13VW71    W84  C~55OH      
2016 09  11.17158  00 26 04.653  +01 19 41.55  22.8z 13VW71    W84  C~55OH      
2016 10  02.18024  00 24 35.557  +01 10 05.58  23.0i 13VW71    W84  C~55OH      
2016 10  02.18163  00 24 35.555  +01 10 05.93  23.1r 13VW71    W84  C~55OH      
2016 11  30.10104  00 21 19.733  +00 50 19.10  23.5r 13VW71    W84  C~55OH      
2016 11  30.10240  00 21 19.726  +00 50 19.08  23.5i 13VW71    W84  C~55OH      
2017 09  27.193241 00 29 39.08   +01 43 59.6   23.1r 13VW71    W84  C~55OH      
2017 09  27.194606 00 29 39.07   +01 43 59.7   23.0i 13VW71    W84  C~55OH      
2017 10  22.18433  00 27 53.509  +01 32 54.50  24.4r 13VW71    W84  C~55OH      
2017 10  22.185185 00 27 53.50   +01 32 54.3   23.3i 13VW71    W84  C~55OH      
2017 10  27.17431  00 27 34.129  +01 30 54.82  22.9z 13VW71    W84  C~55OH      
2017 10  29.13345  00 27 26.811  +01 30 10.00  22.6z 13VW71    W84  C~55OH      
2017 10  29.146169 00 27 26.76   +01 30 10.0   22.7z 13VW71    W84  C~55OH      
2018 09  09.32306  00 35 35.512  +02 23 33.50  23.1i 13VW71    W84  C~55OH      
2018 09  09.32445  00 35 35.498  +02 23 33.50  22.7r 13VW71    W84  C~55OH      
2018 09  09.32583  00 35 35.503  +02 23 33.51  23.9g 13VW71    W84  C~55OH      

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     0.01       0.00    -0.11
     2   0.0000     -1.12     0.02       0.09    -0.04
     3   0.0713  -1502.35    -0.08      32.61     0.14
     4   0.1122  -2073.03     0.10      58.99    -0.04
     5   0.8466   8286.09     0.05      69.53     0.21
     6   0.9696   5379.62    -0.23      55.31     0.12
     7   1.0897   2791.40     0.03     105.27    -0.16
     8   2.9082  16191.79    -0.11     178.33    -0.06
     9   2.9133  16070.06     0.22     177.69    -0.10
    10   2.9708  14607.03    -0.08     179.65    -0.20
    11   2.9708  14607.14     0.14     179.98     0.13
    12   3.1321  11427.80     0.13     257.69    -0.09
    13   3.1321  11427.70     0.06     257.72    -0.07
    14   3.9565  19626.43    -0.01     240.34    -0.05
    15   3.9565  19626.33    -0.01     240.49     0.11
    16   4.0249  17895.34    -0.08     257.86     0.22
    17   4.0249  17895.14    -0.23     257.73     0.09
    18   4.0385  17578.79    -0.23     263.35    -0.09
    19   4.0439  17459.43     0.07     265.76    -0.12
    20   4.0439  17458.72     0.14     266.07     0.16
    21   4.9068  25543.20     0.05     303.45    -0.07
    22   4.9068  25543.00    -0.06     303.54     0.02
    23   4.9069  25543.07     0.11     303.52    -0.00

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.

13VW71    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        44.417    44.432    44.403
ecceobj         0.018     0.018     0.018
incobj          1.594     1.594     1.594
qmin           42.642    42.668    42.653
qmax           45.947    45.954    45.893
amean          44.199    44.213    44.185
amin           43.858    43.879    43.840
amax           44.542    44.562    44.525
emean           0.017     0.017     0.017
emin            0.001     0.002     0.000
emax            0.032     0.031     0.031
imean           0.891     0.892     0.891
imin            0.152     0.156     0.148
imax            1.318     1.317     1.319
excite_mean     0.024     0.024     0.024
fracstop        1.000     1.000     1.000
cjmean          3.103     3.103     3.103

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       189.5     189.4     189.8
kozaiamp        180.0     180.0     180.0