Orbit Fit and Astrometric record for 21LA44

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: 21LA44    
# 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:
  -0.000035   0.026563  -0.000003  -0.002121   0.026408   0.000000
# Chi-squared of fit:     0.69 DOF:     36 RMS:  0.03
# Min/Max residuals:    -0.07    0.07
# Exact a, adot, b, bdot, g, gdot:
  1.589548E-05  2.669112E-02 -1.326556E-06 -2.172887E-03  2.658909E-02 -5.055850E-03
# Covariance matrix:
  3.2886E-13  6.2933E-13  3.7188E-14 -5.6720E-13  1.2175E-12  1.6188E-10
  6.2933E-13  3.3805E-12  1.8899E-13 -2.8838E-12  5.5405E-12  8.2069E-10
  3.7188E-14  1.8899E-13  1.5164E-13 -3.0866E-13  3.4469E-13  5.6776E-11
 -5.6720E-13 -2.8838E-12 -3.0866E-13  3.2287E-12 -5.2605E-12 -8.6673E-10
  1.2175E-12  5.5405E-12  3.4469E-13 -5.2605E-12  9.7426E-12  1.4957E-09
  1.6188E-10  8.2069E-10  5.6776E-11 -8.6673E-10  1.4957E-09  2.4603E-07
#      lat0       lon0       xBary       yBary       zBary        JD0
    1.134490  -72.018316    0.504939    0.017148   -0.876766  2459374.942811
# Heliocentric elements and errors
Epoch:              2459370.5000  =  2021/06/05
Mean Anomaly:          290.10209 +/-     1.679
Argument of Peri:      259.54319 +/-     0.199
Long of Asc Node:      120.62909 +/-     0.006
Inclination:             4.77585 +/-     0.002
Eccentricity:         0.20162756 +/-    0.0183
Semi-Major Axis:     39.70752186 +/-    0.2993
Time of Perihelion: 2477115.2249 +/-     376.2
Perihelion:          31.70139112 +/-    0.7656
Aphelion:            47.71365260 +/-    0.8114
Period (y)              250.2173 +/-      2.83
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           11.40689610 +/-    0.0013
Ecliptic Y          -36.76014312 +/-    0.0042
Ecliptic Z            0.74466704 +/-    0.0001
Ecliptic XDOT         0.00246037 +/-    0.0000
Ecliptic YDOT         0.00134644 +/-    0.0000
Ecliptic ZDOT        -0.00023419 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   38.49649243 +/-    0.0040
Geocenter to KBO     37.60941027 +/-    0.0044
# Hcoef:  7.42

The following table shows the complete astrometric record for 21LA44. 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 (21LA44) followed by the observatory code and reference code for the source of the astrometry.

2021 06  09.44201  19 17 16.874  -21 06 24.62  23.8r 21LA44    266  C~6Ip2      
2021 06  09.52601  19 17 16.476  -21 06 25.37  23.8r 21LA44    266  C~6Ip2      
2021 06  09.61426  19 17 16.058  -21 06 26.15  23.8r 21LA44    266  C~6Ip2      
2021 06  17.43605  19 16 38.126  -21 07 39.75  23.6r 21LA44    266  C~6Ip2      
2021 06  17.50053  19 16 37.795  -21 07 40.39  23.6r 21LA44    266  C~6Ip2      
2021 06  17.57953  19 16 37.389  -21 07 41.15  23.6r 21LA44    266  C~6Ip2      
2021 07  05.35106  19 15 02.841  -21 10 48.24  23.7r 21LA44    266  C~6Ip2      
2021 07  05.43951  19 15 02.346  -21 10 49.23  23.7r 21LA44    266  C~6Ip2      
2021 07  05.52517  19 15 01.866  -21 10 50.17  23.7r 21LA44    266  C~6Ip2      
2021 09  05.23105  19 10 21.109  -21 21 04.54  23.8r 21LA44    266  C~6Ip2      
2021 09  05.31314  19 10 20.895  -21 21 05.11  23.8r 21LA44    266  C~6Ip2      
2021 09  05.39641  19 10 20.680  -21 21 05.66  23.8r 21LA44    266  C~6Ip2      
2022 10  20.21696  19 16 40.276  -21 19 26.65  22.6V 21LA44    266  C~7um8      
2022 10  20.26058  19 16 40.367  -21 19 26.58  22.6V 21LA44    266  C~7um8      
2022 10  20.29842  19 16 40.447  -21 19 26.52  22.6V 21LA44    266  C~7um8      
2022 10  21.20926  19 16 42.477  -21 19 25.20  23.1V 21LA44    266  C~7um8      
2022 10  21.25420  19 16 42.576  -21 19 25.13  23.1V 21LA44    266  C~7um8      
2022 10  21.29846  19 16 42.674  -21 19 25.05  23.1V 21LA44    266  C~7um8      
2022 10  23.20599  19 16 47.260  -21 19 21.92  22.5V 21LA44    266  C~7um8      
2022 10  23.25093  19 16 47.368  -21 19 21.83  22.5V 21LA44    266  C~7um8      
2022 10  23.29489  19 16 47.476  -21 19 21.73  22.5V 21LA44    266  C~7um8      

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     0.01
     2   0.0002     -5.62    -0.01      -0.01     0.02
     3   0.0005    -11.52    -0.01      -0.01     0.01
     4   0.0219   -547.36     0.00      -3.39    -0.01
     5   0.0221   -552.03     0.01      -3.42    -0.01
     6   0.0223   -557.77     0.00      -3.43     0.00
     7   0.0709  -1893.56     0.00     -17.83     0.01
     8   0.0712  -1900.55     0.00     -17.92     0.01
     9   0.0714  -1907.33    -0.00     -17.99     0.00
    10   0.2404  -5879.40     0.00    -139.21    -0.02
    11   0.2406  -5882.44    -0.00    -139.42    -0.02
    12   0.2408  -5885.49    -0.00    -139.60    -0.01
    13   1.3628   -609.91     0.04    -708.16    -0.03
    14   1.3630   -608.64     0.03    -708.26    -0.03
    15   1.3631   -607.53     0.04    -708.34    -0.03
    16   1.3656   -579.23    -0.07    -710.74     0.07
    17   1.3657   -577.85    -0.07    -710.85     0.07
    18   1.3658   -576.48    -0.07    -710.95     0.06
    19   1.3710   -512.54     0.04    -716.23    -0.03
    20   1.3711   -511.04     0.02    -716.34    -0.03
    21   1.3713   -509.53     0.04    -716.44    -0.03

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.

21LA44    quality flag:2

Type:           3:2E  CENTAURR      3:2E

axisobj        39.281    39.876    38.870
ecceobj         0.203     0.247     0.159
incobj          4.786     4.780     4.792
qmin           31.034    29.812    32.376
qmax           48.277    67.096    47.650
amean          39.456    46.825    39.460
amin           39.106    38.754    38.745
amax           39.875    49.118    40.220
emean           0.197     0.338     0.161
emin            0.180     0.224     0.131
emax            0.211     0.368     0.185
imean           3.064     4.989     3.190
imin            2.686     2.752     1.308
imax            3.744     8.906     4.779
excite_mean     0.204     0.350     0.171
fracstop        1.000     0.187     1.000
cjmean          3.004     2.979     3.019

libcent 0       180.8    -180.0     182.3
libamp  0        33.8    -180.0     169.6
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       193.2     161.4     179.8
kozaiamp        180.0     179.7     180.0