Orbit Fit and Astrometric record for 21LO44

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: 21LO44    
# Created Wed May  8 01:18:43 2024
# Orbit generated from Bernstein formalism
# Fitting     21 observations of     21
# Arc:   1.28y
# First observation: 2020/05/26
#  Last observation: 2021/09/06
Preliminary a, adot, b, bdot, g, gdot:
  -0.000006   0.029827  -0.000008  -0.009985   0.029007   0.000000
# Chi-squared of fit:     0.27 DOF:     36 RMS:  0.02
# Min/Max residuals:    -0.03    0.04
# Exact a, adot, b, bdot, g, gdot:
  1.621121E-05  2.992437E-02 -5.613307E-06 -1.006366E-02  2.915991E-02  7.908193E-03
# Covariance matrix:
  2.1557E-13  1.6004E-12  9.7641E-15 -6.5546E-13  1.7681E-12  5.6957E-11
  1.6004E-12  5.9669E-11  3.2863E-13 -2.2138E-11  6.0467E-11  1.9237E-09
  9.7641E-15  3.2863E-13  1.6528E-13 -2.6864E-13  3.3323E-13  1.0696E-11
 -6.5546E-13 -2.2138E-11 -2.6864E-13  8.5052E-12 -2.2470E-11 -7.1929E-10
  1.7681E-12  6.0467E-11  3.3323E-13 -2.2470E-11  6.1588E-11  1.9525E-09
  5.6957E-11  1.9237E-09  1.0696E-11 -7.1929E-10  1.9525E-09  6.2502E-08
#      lat0       lon0       xBary       yBary       zBary        JD0
    2.103428  -74.248367    0.659381    0.027900   -0.763120  2458995.943811
# Heliocentric elements and errors
Epoch:              2458990.5000  =  2020/05/21
Mean Anomaly:           50.47161 +/-     0.338
Argument of Peri:       96.47244 +/-     0.423
Long of Asc Node:      110.83419 +/-     0.001
Inclination:            18.51700 +/-     0.003
Eccentricity:         0.25022759 +/-    0.0080
Semi-Major Axis:     39.51337137 +/-    0.1581
Time of Perihelion: 2446271.3179 +/-      37.8
Perihelion:          29.62603573 +/-    0.3371
Aphelion:            49.40070702 +/-    0.3724
Period (y)              248.3844 +/-      1.49
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X            8.88157733 +/-    0.0025
Ecliptic Y          -33.90446329 +/-    0.0089
Ecliptic Z            1.25857544 +/-    0.0003
Ecliptic XDOT         0.00292309 +/-    0.0000
Ecliptic YDOT         0.00001871 +/-    0.0000
Ecliptic ZDOT        -0.00091723 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   35.07105728 +/-    0.0086
Geocenter to KBO     34.29366273 +/-    0.0092
# Hcoef:  9.59

The following table shows the complete astrometric record for 21LO44. 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 (21LO44) followed by the observatory code and reference code for the source of the astrometry.

2020 05  26.44301  19 07 18.387  -20 25 13.69  25.3r 21LO44    266  C~7um8      
2020 05  26.50149  19 07 18.135  -20 25 14.30  25.3r 21LO44    266  C~7um8      
2020 05  26.55599  19 07 17.898  -20 25 14.86  25.3r 21LO44    266  C~7um8      
2020 05  29.44698  19 07 05.329  -20 25 45.00  24.6r 21LO44    266  C~7um8      
2020 05  29.53371  19 07 04.933  -20 25 45.94  24.6r 21LO44    266  C~7um8      
2020 05  29.61905  19 07 04.542  -20 25 46.85  24.6r 21LO44    266  C~7um8      
2020 05  31.44139  19 06 56.280  -20 26 06.57  24.7r 21LO44    266  C~7um8      
2020 05  31.53101  19 06 55.857  -20 26 07.57  24.7r 21LO44    266  C~7um8      
2020 05  31.61814  19 06 55.446  -20 26 08.52  24.7r 21LO44    266  C~7um8      
2021 06  09.44201  19 13 47.593  -20 49 43.95  25.3r 21LO44    266  C~6Ip3      
2021 06  09.52601  19 13 47.160  -20 49 45.08  25.3r 21LO44    266  C~6Ip3      
2021 06  09.61426  19 13 46.705  -20 49 46.24  25.3r 21LO44    266  C~6Ip3      
2021 06  17.43605  19 13 05.427  -20 51 34.91  25.1r 21LO44    266  C~6Ip3      
2021 06  17.50053  19 13 05.068  -20 51 35.84  25.1r 21LO44    266  C~6Ip3      
2021 06  17.57953  19 13 04.627  -20 51 36.96  25.1r 21LO44    266  C~6Ip3      
2021 07  05.35106  19 11 22.167  -20 56 06.38  24.7r 21LO44    266  C~6Ip3      
2021 07  05.43951  19 11 21.632  -20 56 07.79  24.7r 21LO44    266  C~6Ip3      
2021 07  05.52517  19 11 21.114  -20 56 09.13  24.7r 21LO44    266  C~6Ip3      
2021 09  06.23258  19 06 19.915  -21 11 32.15  25.3r 21LO44    266  C~6Ip3      
2021 09  06.31281  19 06 19.710  -21 11 33.07  25.3r 21LO44    266  C~6Ip3      
2021 09  06.39352  19 06 19.505  -21 11 33.98  25.3r 21LO44    266  C~6Ip3      

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     0.00       0.00     0.03
     2   0.0002     -3.59     0.01      -0.20     0.03
     3   0.0003     -6.96     0.01      -0.37     0.03
     4   0.0082   -185.94    -0.02      -9.98    -0.03
     5   0.0085   -191.58    -0.02     -10.28    -0.03
     6   0.0087   -197.14    -0.02     -10.55    -0.03
     7   0.0137   -314.77     0.01     -16.81    -0.00
     8   0.0139   -320.79     0.01     -17.12    -0.00
     9   0.0142   -326.64     0.02     -17.40    -0.00
    10   1.0376   5248.95     0.01   -2116.66     0.04
    11   1.0379   5242.78     0.01   -2117.02     0.04
    12   1.0381   5236.30     0.02   -2117.37     0.04
    13   1.0595   4648.26    -0.03   -2153.05    -0.03
    14   1.0597   4643.15    -0.01   -2153.35    -0.03
    15   1.0599   4636.87    -0.01   -2153.69    -0.03
    16   1.1086   3178.26     0.00   -2244.72    -0.01
    17   1.1088   3170.64     0.00   -2245.21    -0.02
    18   1.1091   3163.27     0.01   -2245.66    -0.02
    19   1.2807  -1132.64     0.00   -2666.51     0.00
    20   1.2810  -1135.59     0.00   -2667.10     0.01
    21   1.2812  -1138.54    -0.01   -2667.68     0.01

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.

21LO44    quality flag:2

Type:           3:2E  CENTAURR  CENTAURR

axisobj        38.937    39.535    38.386
ecceobj         0.244     0.263     0.224
incobj         18.577    18.567    18.586
qmin           29.077    28.630    28.720
qmax           50.615    50.988    49.232
amean          39.456    38.905    34.966
amin           38.911    37.585    30.841
amax           40.092    40.116    40.299
emean           0.236     0.223     0.094
emin            0.200     0.179     0.007
emax            0.264     0.273     0.239
imean          17.833    18.268    17.486
imin           16.834    16.829    15.048
imax           19.124    19.270    19.365
excite_mean     0.387     0.386     0.319
fracstop        1.000     0.023     0.989
cjmean          2.881     2.877     2.906

libcent 0       178.7    -180.0    -180.0
libamp  0       138.1    -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       234.5     135.4     185.7
kozaiamp        107.7      37.6     179.9