Orbit Fit and Astrometric record for 21LX44

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: 21LX44    
# Created Sun Dec 22 02:11:18 2024
# Orbit generated from Bernstein formalism
# Fitting     19 observations of     19
# Arc:   1.50y
# First observation: 2021/04/23
#  Last observation: 2022/10/23
Preliminary a, adot, b, bdot, g, gdot:
  -0.000128   0.029920  -0.000005  -0.001440   0.027786   0.000000
# Chi-squared of fit:     0.87 DOF:     32 RMS:  0.04
# Min/Max residuals:    -0.20    0.04
# Exact a, adot, b, bdot, g, gdot:
  1.680211E-05  2.950050E-02  1.482522E-07 -1.475088E-03  2.762073E-02  4.253433E-03
# Covariance matrix:
  1.3136E-12  5.2236E-13  1.0615E-13 -8.2792E-13  3.3736E-12  3.1680E-10
  5.2236E-13  7.4705E-13  3.7845E-14 -3.2994E-13  1.6948E-12  1.2846E-10
  1.0615E-13  3.7845E-14  2.0479E-13 -2.4541E-13  3.6404E-13  3.8696E-11
 -8.2792E-13 -3.2994E-13 -2.4541E-13  9.4385E-13 -2.7769E-12 -2.8970E-10
  3.3736E-12  1.6948E-12  3.6404E-13 -2.7769E-12  1.0687E-11  1.0586E-09
  3.1680E-10  1.2846E-10  3.8696E-11 -2.8970E-10  1.0586E-09  1.1008E-07
#      lat0       lon0       xBary       yBary       zBary        JD0
    1.498970  -72.594481    0.973619    0.006763   -0.264144  2459327.797186
# Heliocentric elements and errors
Epoch:              2459320.5000  =  2021/04/16
Mean Anomaly:           47.03078 +/-     1.240
Argument of Peri:       91.62503 +/-     2.274
Long of Asc Node:      133.79281 +/-     0.009
Inclination:             3.17523 +/-     0.001
Eccentricity:         0.14159198 +/-    0.0105
Semi-Major Axis:     39.83710451 +/-    0.1276
Time of Perihelion: 2447322.4754 +/-     310.9
Perihelion:          34.19648981 +/-    0.4334
Aphelion:            45.47771920 +/-    0.4439
Period (y)              251.4432 +/-      1.21
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X            9.98425764 +/-    0.0012
Ecliptic Y          -35.08360002 +/-    0.0041
Ecliptic Z            0.94710308 +/-    0.0001
Ecliptic XDOT         0.00292347 +/-    0.0000
Ecliptic YDOT         0.00047568 +/-    0.0000
Ecliptic ZDOT        -0.00013533 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   36.48892154 +/-    0.0040
Geocenter to KBO     36.20469186 +/-    0.0043
# Hcoef:  6.92

The following table shows the complete astrometric record for 21LX44. 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 (21LX44) followed by the observatory code and reference code for the source of the astrometry.

2021 04  23.296385 19 14 37.95   -20 49 12.0         21LX44    W84  C~6pyQ      
2021 06  09.44201  19 12 18.227  -20 52 25.83  23.1r 21LX44    266  C~6Ip3      
2021 06  09.52601  19 12 17.807  -20 52 26.52  23.1r 21LX44    266  C~6Ip3      
2021 06  09.61426  19 12 17.366  -20 52 27.22  23.1r 21LX44    266  C~6Ip3      
2021 06  17.43605  19 11 37.401  -20 53 34.73  23.0r 21LX44    266  C~6Ip3      
2021 06  17.50053  19 11 37.052  -20 53 35.32  23.0r 21LX44    266  C~6Ip3      
2021 06  17.57953  19 11 36.626  -20 53 36.03  23.0r 21LX44    266  C~6Ip3      
2021 09  06.23258  19 05 07.037  -21 06 29.04  23.5r 21LX44    266  C~6Ip3      
2021 09  06.31281  19 05 06.842  -21 06 29.57  23.5r 21LX44    266  C~6Ip3      
2021 09  06.39352  19 05 06.648  -21 06 30.09  23.5r 21LX44    266  C~6Ip3      
2022 10  20.21696  19 12 21.803  -21 01 45.89  22.2V 21LX44    266  C~7um8      
2022 10  20.26058  19 12 21.906  -21 01 45.83  22.2V 21LX44    266  C~7um8      
2022 10  20.29842  19 12 21.996  -21 01 45.77  22.2V 21LX44    266  C~7um8      
2022 10  21.20926  19 12 24.285  -21 01 44.56  21.9V 21LX44    266  C~7um8      
2022 10  21.25420  19 12 24.396  -21 01 44.49  21.9V 21LX44    266  C~7um8      
2022 10  21.29846  19 12 24.507  -21 01 44.41  21.9V 21LX44    266  C~7um8      
2022 10  23.20599  19 12 29.620  -21 01 41.40  22.1V 21LX44    266  C~7um8      
2022 10  23.25093  19 12 29.741  -21 01 41.31  22.1V 21LX44    266  C~7um8      
2022 10  23.29489  19 12 29.861  -21 01 41.21  22.1V 21LX44    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     0.02       0.00    -0.20
     2   0.1291  -1967.54    -0.00      53.53     0.03
     3   0.1293  -1973.46    -0.00      53.57     0.03
     4   0.1295  -1979.69     0.00      53.64     0.04
     5   0.1510  -2543.90    -0.00      55.64     0.02
     6   0.1511  -2548.82    -0.01      55.65     0.02
     7   0.1514  -2554.84    -0.01      55.68     0.02
     8   0.3722  -8067.50     0.00     -70.39     0.02
     9   0.3724  -8070.28     0.00     -70.61     0.03
    10   0.3726  -8073.04     0.01     -70.82     0.02
    11   1.4919  -1987.14    -0.00    -508.45    -0.03
    12   1.4920  -1985.70    -0.00    -508.57    -0.03
    13   1.4921  -1984.45    -0.00    -508.67    -0.03
    14   1.4946  -1952.49     0.00    -511.43     0.03
    15   1.4948  -1950.94    -0.00    -511.56     0.02
    16   1.4949  -1949.39     0.01    -511.67     0.03
    17   1.5001  -1877.97     0.00    -517.56    -0.00
    18   1.5002  -1876.28    -0.01    -517.68    -0.01
    19   1.5003  -1874.60    -0.00    -517.79    -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.

21LX44    quality flag:1

Type:           3:2E  CENTAURR  SCATNEAR

axisobj        39.328    39.947    38.790
ecceobj         0.135     0.164     0.105
incobj          3.180     3.182     3.177
qmin           33.167    30.136    32.319
qmax           46.291    62.237    47.767
amean          39.458    42.488    39.367
amin           38.986    31.851    38.709
amax           39.965    47.348    40.264
emean           0.141     0.239     0.143
emin            0.121     0.007     0.096
emax            0.159     0.319     0.188
imean           2.562     1.961     2.415
imin            1.663     0.383     0.678
imax            3.380     4.049     3.914
excite_mean     0.148     0.242     0.149
fracstop        1.000     0.514     1.000
cjmean          3.027     3.012     3.026

libcent 0       180.2    -180.0    -180.0
libamp  0       103.8    -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       183.5     179.8     177.9
kozaiamp        180.0     179.8     180.0