Orbit Fit and Astrometric record for 21LP44

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: 21LP44    
# Created Fri Nov 22 02:11:10 2024
# Orbit generated from Bernstein formalism
# Fitting     24 observations of     24
# Arc:   1.28y
# First observation: 2020/05/26
#  Last observation: 2021/09/06
Preliminary a, adot, b, bdot, g, gdot:
   0.000010   0.034600  -0.000002  -0.002514   0.029080   0.000000
# Chi-squared of fit:     0.25 DOF:     42 RMS:  0.02
# Min/Max residuals:    -0.03    0.04
# Exact a, adot, b, bdot, g, gdot:
  1.870150E-05  3.410615E-02 -1.326445E-06 -2.485291E-03  2.867523E-02 -8.216248E-03
# Covariance matrix:
  2.5890E-13  3.9073E-12  3.1295E-15 -3.2613E-13  3.4174E-12  1.1367E-10
  3.9073E-12  1.7345E-10  1.3204E-13 -1.3898E-11  1.4648E-10  4.8437E-09
  3.1295E-15  1.3204E-13  1.6345E-13 -1.5643E-13  1.1110E-13  3.7111E-12
 -3.2613E-13 -1.3898E-11 -1.5643E-13  1.3222E-12 -1.1738E-11 -3.8905E-10
  3.4174E-12  1.4648E-10  1.1110E-13 -1.1738E-11  1.2398E-10  4.0909E-09
  1.1367E-10  4.8437E-09  3.7111E-12 -3.8905E-10  4.0909E-09  1.3560E-07
#      lat0       lon0       xBary       yBary       zBary        JD0
    1.853670  -74.104972    0.661290    0.024520   -0.761582  2458995.943811
# Heliocentric elements and errors
Epoch:              2458990.5000  =  2020/05/21
Mean Anomaly:          340.78074 +/-     0.443
Argument of Peri:      206.31334 +/-     1.195
Long of Asc Node:      128.37307 +/-     0.006
Inclination:             4.53313 +/-     0.001
Eccentricity:         0.43389492 +/-    0.0107
Semi-Major Axis:     56.18742388 +/-    0.6620
Time of Perihelion: 2467203.2999 +/-     121.2
Perihelion:          31.80798597 +/-    0.7074
Aphelion:            80.56686179 +/-    1.1229
Period (y)              421.1792 +/-      7.44
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X            9.12426887 +/-    0.0037
Ecliptic Y          -34.44319879 +/-    0.0130
Ecliptic Z            1.12807157 +/-    0.0004
Ecliptic XDOT         0.00292737 +/-    0.0000
Ecliptic YDOT         0.00164205 +/-    0.0000
Ecliptic ZDOT        -0.00026277 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   35.64910618 +/-    0.0126
Geocenter to KBO     34.87330886 +/-    0.0135
# Hcoef:  9.21

The following table shows the complete astrometric record for 21LP44. 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 (21LP44) followed by the observatory code and reference code for the source of the astrometry.

2020 05  26.44301  19 08 02.282  -20 39 07.01  25.1r 21LP44    266  C~6VLq      
2020 05  26.50149  19 08 02.043  -20 39 07.36  25.1r 21LP44    266  C~6VLq      
2020 05  26.55599  19 08 01.819  -20 39 07.69  25.1r 21LP44    266  C~6VLq      
2020 05  29.44698  19 07 49.921  -20 39 25.31  24.4r 21LP44    266  C~6VLq      
2020 05  29.53371  19 07 49.545  -20 39 25.87  24.4r 21LP44    266  C~6VLq      
2020 05  29.61905  19 07 49.174  -20 39 26.40  24.4r 21LP44    266  C~6VLq      
2020 05  31.44139  19 07 41.336  -20 39 38.22  24.5r 21LP44    266  C~6VLq      
2020 05  31.52961  19 07 40.941  -20 39 38.82  24.5r 21LP44    266  C~6VLq      
2020 05  31.61814  19 07 40.544  -20 39 39.40  24.5r 21LP44    266  C~6VLq      
2021 06  09.44201  19 15 29.523  -20 34 51.66  24.6r 21LP44    266  C~6Ip3      
2021 06  09.52601  19 15 29.107  -20 34 52.41  24.6r 21LP44    266  C~6Ip3      
2021 06  09.61426  19 15 28.669  -20 34 53.17  24.6r 21LP44    266  C~6Ip3      
2021 06  17.43605  19 14 48.965  -20 36 06.43  24.5r 21LP44    266  C~6Ip3      
2021 06  17.50053  19 14 48.618  -20 36 07.07  24.5r 21LP44    266  C~6Ip3      
2021 06  17.57953  19 14 48.193  -20 36 07.84  24.5r 21LP44    266  C~6Ip3      
2021 07  05.34556  19 13 09.081  -20 39 19.09  24.9r 21LP44    266  C~6Ip3      
2021 07  05.35106  19 13 09.044  -20 39 19.18  24.2r 21LP44    266  C~6Ip3      
2021 07  05.39262  19 13 08.805  -20 39 19.64  24.9r 21LP44    266  C~6Ip3      
2021 07  05.43532  19 13 08.554  -20 39 20.14  24.9r 21LP44    266  C~6Ip3      
2021 07  05.43951  19 13 08.525  -20 39 20.21  24.2r 21LP44    266  C~6Ip3      
2021 07  05.52517  19 13 08.021  -20 39 21.18  24.2r 21LP44    266  C~6Ip3      
2021 09  06.23258  19 08 15.288  -20 50 34.24  24.9r 21LP44    266  C~6Ip3      
2021 09  06.31281  19 08 15.091  -20 50 34.87  24.9r 21LP44    266  C~6Ip3      
2021 09  06.39352  19 08 14.895  -20 50 35.48  24.9r 21LP44    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     0.02       0.00    -0.01
     2   0.0002     -3.37     0.03       0.04    -0.00
     3   0.0003     -6.53     0.02       0.08    -0.01
     4   0.0082   -174.45    -0.01       2.00    -0.02
     5   0.0085   -179.76    -0.01       2.05    -0.02
     6   0.0087   -184.99    -0.02       2.13    -0.01
     7   0.0137   -295.63    -0.01       3.15     0.02
     8   0.0139   -301.20    -0.01       3.20     0.02
     9   0.0142   -306.81    -0.00       3.27     0.02
    10   1.0376   6265.08    -0.00    -513.46     0.00
    11   1.0379   6259.18    -0.00    -513.45     0.00
    12   1.0381   6252.98    -0.01    -513.42     0.01
    13   1.0595   5690.21    -0.01    -515.11     0.00
    14   1.0597   5685.29    -0.00    -515.13     0.00
    15   1.0599   5679.27     0.00    -515.14     0.00
    16   1.1086   4274.08     0.04    -530.23     0.02
    17   1.1086   4273.56    -0.03    -530.26     0.01
    18   1.1087   4270.17     0.04    -530.30     0.02
    19   1.1088   4266.61     0.04    -530.36     0.02
    20   1.1088   4266.20    -0.03    -530.38     0.00
    21   1.1091   4259.05    -0.03    -530.46     0.00
    22   1.2807    101.07    -0.00    -703.82    -0.02
    23   1.2810     98.26    -0.00    -704.12    -0.03
    24   1.2812     95.46    -0.00    -704.40    -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.

21LP44    quality flag:2

Type:         5:2EEE  CENTAURR  CENTAURR

axisobj        55.183    56.323    54.256
ecceobj         0.428     0.449     0.408
incobj          4.539     4.542     4.536
qmin           31.190    30.097    29.717
qmax           81.106    89.710    82.907
amean          55.462    56.265    51.993
amin           54.773    49.144    40.381
amax           56.394    60.478    57.457
emean           0.427     0.448     0.388
emin            0.417     0.382     0.257
emax            0.438     0.483     0.443
imean           3.144     2.318     2.152
imin            3.065     1.524     0.768
imax            3.248     3.124     4.573
excite_mean     0.430     0.450     0.390
fracstop        1.000     0.024     0.123
cjmean          2.994     2.977     2.998

libcent 0       180.6    -180.0    -180.0
libamp  0        71.6    -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       181.8     290.1     231.5
kozaiamp        179.9      70.1     178.5