Orbit Fit and Astrometric record for 21LM44

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: 21LM44    
# Created Wed May  8 01:18:43 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:
  -0.000027   0.018648  -0.000000  -0.000033   0.021277   0.000000
# Chi-squared of fit:     0.15 DOF:     36 RMS:  0.01
# Min/Max residuals:    -0.02    0.04
# Exact a, adot, b, bdot, g, gdot:
  1.382924E-05  1.869142E-02 -1.129028E-08 -4.049495E-05  2.142166E-02 -3.956222E-04
# Covariance matrix:
  3.4901E-13 -2.3619E-13  7.9085E-15 -1.1946E-13  1.2321E-12  2.3162E-10
 -2.3619E-13  1.4345E-12 -2.1014E-14  3.2476E-13 -2.0030E-12 -5.8804E-10
  7.9085E-15 -2.1014E-14  1.3930E-13 -1.1685E-13  6.3608E-14  1.4862E-11
 -1.1946E-13  3.2476E-13 -1.1685E-13  2.9760E-13 -9.6865E-13 -2.2728E-10
  1.2321E-12 -2.0030E-12  6.3608E-14 -9.6865E-13  8.5578E-12  1.8338E-09
  2.3162E-10 -5.8804E-10  1.4862E-11 -2.2728E-10  1.8338E-09  4.2488E-07
#      lat0       lon0       xBary       yBary       zBary        JD0
    1.367274  -73.026769    0.489427    0.020919   -0.885438  2459374.942811
# Heliocentric elements and errors
Epoch:              2459370.5000  =  2021/06/05
Mean Anomaly:          205.49210 +/-    20.471
Argument of Peri:      253.02695 +/-    20.477
Long of Asc Node:      191.60597 +/-     0.055
Inclination:             1.34634 +/-     0.000
Eccentricity:         0.08320431 +/-    0.0121
Semi-Major Axis:     44.20606035 +/-    0.0856
Time of Perihelion: 2505445.9222 +/-    6103.1
Perihelion:          40.52792546 +/-    0.5398
Aphelion:            47.88419523 +/-    0.5421
Period (y)              293.9212 +/-      0.85
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           13.42238709 +/-    0.0018
Ecliptic Y          -45.63038260 +/-    0.0061
Ecliptic Z            1.11395724 +/-    0.0002
Ecliptic XDOT         0.00227570 +/-    0.0000
Ecliptic YDOT         0.00075274 +/-    0.0001
Ecliptic ZDOT        -0.00000657 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   47.57660342 +/-    0.0059
Geocenter to KBO     46.68173018 +/-    0.0064
# Hcoef:  8.06

The following table shows the complete astrometric record for 21LM44. 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 (21LM44) followed by the observatory code and reference code for the source of the astrometry.

2021 06  09.44201  19 12 52.060  -21 00 18.12  25.1r 21LM44    266  C~6Ip2      
2021 06  09.52741  19 12 51.720  -21 00 18.64  25.1r 21LM44    266  C~6Ip2      
2021 06  09.61426  19 12 51.374  -21 00 19.15  25.1r 21LM44    266  C~6Ip2      
2021 06  17.43605  19 12 19.550  -21 01 09.08  25.4r 21LM44    266  C~6Ip2      
2021 06  17.50053  19 12 19.274  -21 01 09.52  25.4r 21LM44    266  C~6Ip2      
2021 06  17.57953  19 12 18.935  -21 01 10.04  25.4r 21LM44    266  C~6Ip2      
2021 07  05.35106  19 11 00.324  -21 03 19.52  25.7r 21LM44    266  C~6Ip2      
2021 07  05.43951  19 10 59.915  -21 03 20.22  25.7r 21LM44    266  C~6Ip2      
2021 07  05.52517  19 10 59.518  -21 03 20.87  25.7r 21LM44    266  C~6Ip2      
2021 09  06.23258  19 07 06.277  -21 10 40.04  25.6r 21LM44    266  C~6Ip2      
2021 09  06.31281  19 07 06.111  -21 10 40.42  25.6r 21LM44    266  C~6Ip2      
2021 09  06.39352  19 07 05.945  -21 10 40.79  25.6r 21LM44    266  C~6Ip2      
2022 10  20.21696  19 11 29.109  -21 04 43.13  24.1V 21LM44    266  C~7um8      
2022 10  20.26058  19 11 29.182  -21 04 43.06  24.1V 21LM44    266  C~7um8      
2022 10  20.29842  19 11 29.246  -21 04 43.01  24.1V 21LM44    266  C~7um8      
2022 10  21.20926  19 11 30.879  -21 04 41.75  23.9V 21LM44    266  C~7um8      
2022 10  21.25420  19 11 30.958  -21 04 41.68  23.9V 21LM44    266  C~7um8      
2022 10  21.29846  19 11 31.036  -21 04 41.60  23.9V 21LM44    266  C~7um8      
2022 10  23.20599  19 11 34.697  -21 04 38.67  24.2V 21LM44    266  C~7um8      
2022 10  23.25093  19 11 34.784  -21 04 38.58  24.2V 21LM44    266  C~7um8      
2022 10  23.29489  19 11 34.870  -21 04 38.49  24.2V 21LM44    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    -0.01       0.00    -0.00
     2   0.0002     -4.79    -0.00       0.08    -0.00
     3   0.0005     -9.66    -0.00       0.17    -0.00
     4   0.0219   -458.03     0.00       5.87     0.01
     5   0.0221   -461.92     0.01       5.91     0.01
     6   0.0223   -466.69     0.01       5.98     0.01
     7   0.0709  -1574.86    -0.01      12.30     0.01
     8   0.0712  -1580.63    -0.00      12.31    -0.00
     9   0.0714  -1586.23    -0.00      12.34    -0.00
    10   0.2431  -4879.82    -0.00     -37.20    -0.01
    11   0.2433  -4882.17     0.00     -37.31    -0.00
    12   0.2435  -4884.52     0.00     -37.41    -0.01
    13   1.3628  -1185.12    -0.02    -119.79    -0.02
    14   1.3630  -1184.10    -0.02    -119.84    -0.02
    15   1.3631  -1183.21    -0.02    -119.90    -0.02
    16   1.3656  -1160.37     0.03    -121.45     0.03
    17   1.3657  -1159.26     0.03    -121.51     0.03
    18   1.3658  -1158.17     0.02    -121.57     0.04
    19   1.3710  -1106.95    -0.00    -124.93    -0.02
    20   1.3711  -1105.73    -0.00    -124.99    -0.01
    21   1.3713  -1104.53    -0.00    -125.04    -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.

21LM44    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        43.760    44.145    43.744
ecceobj         0.093     0.149     0.088
incobj          1.349     1.348     1.349
qmin           38.751    36.130    38.920
qmax           49.516    52.922    49.309
amean          43.970    44.312    43.957
amin           43.610    43.919    43.606
amax           44.358    44.751    44.343
emean           0.099     0.157     0.094
emin            0.080     0.133     0.075
emax            0.116     0.183     0.112
imean           2.476     2.820     2.450
imin            1.332     1.221     1.361
imax            3.371     4.235     3.331
excite_mean     0.108     0.165     0.103
fracstop        1.000     1.000     1.000
cjmean          3.087     3.071     3.088

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       184.8     190.6     184.1
kozaiamp        179.9     180.0     180.0