Orbit Fit and Astrometric record for 21LV43

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: 21LV43    
# Created Fri Nov 22 02:11:10 2024
# Orbit generated from Bernstein formalism
# Fitting     21 observations of     21
# Arc:   1.37y
# First observation: 2021/06/09
#  Last observation: 2022/10/23
Preliminary a, adot, b, bdot, g, gdot:
  -0.000045   0.028053  -0.000002  -0.000682   0.026273   0.000000
# Chi-squared of fit:     0.98 DOF:     36 RMS:  0.04
# Min/Max residuals:    -0.08    0.09
# Exact a, adot, b, bdot, g, gdot:
  1.689647E-05  2.832505E-02 -4.037747E-07 -7.179963E-04  2.656250E-02  7.526621E-03
# Covariance matrix:
  3.4577E-13  1.2740E-12  1.6381E-14 -2.4900E-13  1.4564E-12  1.8526E-10
  1.2740E-12  1.2079E-11  1.5879E-13 -2.4197E-12  1.2338E-11  1.7854E-09
  1.6381E-14  1.5879E-13  1.4120E-13 -1.4299E-13  1.6364E-13  2.4829E-11
 -2.4900E-13 -2.4197E-12 -1.4299E-13  6.9362E-13 -2.4932E-12 -3.7865E-10
  1.4564E-12  1.2338E-11  1.6364E-13 -2.4932E-12  1.2804E-11  1.8404E-09
  1.8526E-10  1.7854E-09  2.4829E-11 -3.7865E-10  1.8404E-09  2.7864E-07
#      lat0       lon0       xBary       yBary       zBary        JD0
    0.906548  -72.700823    0.494457    0.013754   -0.882779  2459374.942811
# Heliocentric elements and errors
Epoch:              2459370.5000  =  2021/06/05
Mean Anomaly:           37.16845 +/-     0.751
Argument of Peri:       82.00741 +/-     1.497
Long of Asc Node:      138.35483 +/-     0.018
Inclination:             1.68120 +/-     0.001
Eccentricity:         0.30671376 +/-    0.0192
Semi-Major Axis:     47.80749793 +/-    0.6298
Time of Perihelion: 2446904.8639 +/-      51.9
Perihelion:          33.14428025 +/-    1.0154
Aphelion:            62.47071561 +/-    1.2319
Period (y)              330.5615 +/-      6.53
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           10.99206979 +/-    0.0015
Ecliptic Y          -36.93435700 +/-    0.0048
Ecliptic Z            0.59569787 +/-    0.0001
Ecliptic XDOT         0.00302404 +/-    0.0000
Ecliptic YDOT         0.00013356 +/-    0.0001
Ecliptic ZDOT        -0.00006191 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   38.53994267 +/-    0.0047
Geocenter to KBO     37.64705610 +/-    0.0051
# Hcoef:  9.99

The following table shows the complete astrometric record for 21LV43. 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 (21LV43) followed by the observatory code and reference code for the source of the astrometry.

2021 06  09.44201  19 14 30.203  -21 25 16.08  26.1r 21LV43    266  C~6Ip1      
2021 06  09.52601  19 14 29.807  -21 25 16.76  26.1r 21LV43    266  C~6Ip1      
2021 06  09.61426  19 14 29.390  -21 25 17.45  26.1r 21LV43    266  C~6Ip1      
2021 06  17.43605  19 13 51.614  -21 26 23.00  26.3r 21LV43    266  C~6Ip1      
2021 06  17.50053  19 13 51.285  -21 26 23.57  26.3r 21LV43    266  C~6Ip1      
2021 06  17.57953  19 13 50.881  -21 26 24.25  26.3r 21LV43    266  C~6Ip2      
2021 07  05.35106  19 12 17.050  -21 29 10.58  26.4r 21LV43    266  C~6Ip2      
2021 07  05.44091  19 12 16.552  -21 29 11.47  26.4r 21LV43    266  C~6Ip2      
2021 07  05.52517  19 12 16.085  -21 29 12.29  26.4r 21LV43    266  C~6Ip2      
2021 09  06.23258  19 07 39.347  -21 38 02.84  26.5r 21LV43    266  C~6Ip2      
2021 09  06.31281  19 07 39.158  -21 38 03.27  26.5r 21LV43    266  C~6Ip2      
2021 09  06.39352  19 07 38.968  -21 38 03.67  26.5r 21LV43    266  C~6Ip2      
2022 10  20.21696  19 14 26.795  -21 30 06.11  25.2V 21LV43    266  C~7um7      
2022 10  20.26058  19 14 26.890  -21 30 06.00  25.2V 21LV43    266  C~7um7      
2022 10  20.29842  19 14 26.973  -21 30 05.90  25.2V 21LV43    266  C~7um7      
2022 10  21.20926  19 14 29.086  -21 30 03.80  25.4V 21LV43    266  C~7um7      
2022 10  21.25420  19 14 29.189  -21 30 03.68  25.4V 21LV43    266  C~7um7      
2022 10  21.29846  19 14 29.290  -21 30 03.55  25.4V 21LV43    266  C~7um7      
2022 10  23.20599  19 14 34.016  -21 29 58.42  25.5V 21LV43    266  C~7um7      
2022 10  23.25093  19 14 34.128  -21 29 58.27  25.5V 21LV43    266  C~7um7      
2022 10  23.29489  19 14 34.238  -21 29 58.13  25.5V 21LV43    266  C~7um7      

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    -0.00
     2   0.0002     -5.57     0.00       0.03    -0.01
     3   0.0005    -11.43    -0.00       0.08    -0.01
     4   0.0219   -542.95     0.01       1.81     0.02
     5   0.0221   -547.58     0.02       1.82     0.02
     6   0.0223   -553.26     0.01       1.86     0.02
     7   0.0709  -1873.69    -0.02       0.28     0.01
     8   0.0712  -1880.70    -0.02       0.25     0.01
     9   0.0714  -1887.27    -0.02       0.25     0.00
    10   0.2431  -5785.10     0.00     -63.78    -0.03
    11   0.2433  -5787.77     0.01     -63.90    -0.03
    12   0.2435  -5790.45     0.00     -63.99    -0.03
    13   1.3628    -84.03    -0.04    -281.64     0.09
    14   1.3630    -82.70    -0.04    -281.70     0.09
    15   1.3631    -81.54    -0.04    -281.75     0.09
    16   1.3656    -52.02    -0.01    -283.41    -0.01
    17   1.3657    -50.58     0.00    -283.47    -0.01
    18   1.3658    -49.16    -0.01    -283.52    -0.01
    19   1.3710     16.91     0.05    -286.82    -0.08
    20   1.3711     18.48     0.05    -286.87    -0.07
    21   1.3713     20.02     0.04    -286.92    -0.08

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.

21LV43    quality flag:2

Type:           2:1E  SCATNEAR  SCATNEAR

axisobj        47.091    49.420    45.204
ecceobj         0.300     0.352     0.248
incobj          1.682     1.683     1.680
qmin           32.348    31.653    32.127
qmax           64.545    78.560    61.107
amean          47.797    52.531    43.957
amin           47.045    48.276    41.085
amax           48.688    55.651    47.452
emean           0.311     0.376     0.229
emin            0.296     0.317     0.169
emax            0.326     0.412     0.288
imean           1.076     3.837     4.419
imin            0.860     0.865     0.871
imax            1.281     7.566     7.244
excite_mean     0.311     0.383     0.244
fracstop        1.000     1.000     1.000
cjmean          3.024     3.012     3.030

libcent 0       179.6    -180.0    -180.0
libamp  0       156.1    -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        97.3     179.0     179.5
kozaiamp         52.1     180.0     180.0