Orbit Fit and Astrometric record for 21LO43

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: 21LO43    
# Created Wed May  8 01:18:42 2024
# Orbit generated from Bernstein formalism
# Fitting      8 observations of      8
# Arc:   0.84y
# First observation: 2021/06/06
#  Last observation: 2022/04/08
Preliminary a, adot, b, bdot, g, gdot:
  -0.000019   0.011076  -0.000005   0.002936   0.015758   0.000000
# Chi-squared of fit:     5.18 DOF:     10 RMS:  0.14
# Min/Max residuals:    -0.21    0.33
# Exact a, adot, b, bdot, g, gdot:
  1.159853E-05  1.103137E-02  2.752744E-06  2.960220E-03  1.602867E-02  5.463105E-03
# Covariance matrix:
  7.1063E-13 -1.3626E-12 -4.4422E-15  2.2839E-14  5.4724E-13  8.3794E-12
 -1.3626E-12  6.9126E-10 -1.1768E-11  1.2135E-10  3.7065E-10  4.6031E-08
 -4.4422E-15 -1.1768E-11  6.4540E-13 -2.7309E-12 -6.3830E-12 -7.8899E-10
  2.2839E-14  1.2135E-10 -2.7309E-12  2.3093E-11  6.5740E-11  8.1312E-09
  5.4724E-13  3.7065E-10 -6.3830E-12  6.5740E-11  2.0246E-10  2.4936E-08
  8.3794E-12  4.6031E-08 -7.8899E-10  8.1312E-09  2.4936E-08  3.0843E-06
#      lat0       lon0       xBary       yBary       zBary        JD0
   -0.491473 -121.108847   -0.277951   -0.008522   -0.972984  2459371.594141
# Heliocentric elements and errors
Epoch:              2459370.5000  =  2021/06/05
Mean Anomaly:           65.42039 +/-    24.111
Argument of Peri:      242.39378 +/-     7.249
Long of Asc Node:      240.95157 +/-     0.001
Inclination:            15.04344 +/-     0.007
Eccentricity:         0.43191872 +/-    0.1121
Semi-Major Axis:     63.28129458 +/-    7.5206
Time of Perihelion: 2425956.9891 +/-   10778.2
Perihelion:          35.94891874 +/-    8.2825
Aphelion:            90.61367042 +/-   12.8964
Period (y)              503.4093 +/-     89.74
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -32.48915055 +/-    0.0286
Ecliptic Y          -54.39608624 +/-    0.0474
Ecliptic Z           -0.53493803 +/-    0.0004
Ecliptic XDOT         0.00113453 +/-    0.0002
Ecliptic YDOT        -0.00176907 +/-    0.0003
Ecliptic ZDOT         0.00049742 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   63.36217531 +/-    0.0433
Geocenter to KBO     62.38820143 +/-    0.0554
# Hcoef:  6.48

The following table shows the complete astrometric record for 21LO43. 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 (21LO43) followed by the observatory code and reference code for the source of the astrometry.

2021 06  06.09334  15 46 12.371  -20 23 28.55  24.8r 21LO43    807  C~6DKi      
2021 06  07.08147  15 46 09.163  -20 23 16.83  24.6r 21LO43    807  C~6DKi      
2021 09  02.00133  15 44 13.960  -20 14 10.53  24.7r 21LO43    304  C~6DKi      
2021 09  02.99310  15 44 15.220  -20 14 12.78  24.4r 21LO43    304  C~6DKi      
2021 09  03.07903  15 44 15.320  -20 14 13.06  24.5r 21LO43    304  C~6DKi      
2022 03  07.35915  15 52 55.736  -20 36 10.07  24.3r 21LO43    304  C~6DKi      
2022 04  08.29179  15 52 06.092  -20 32 56.30  24.2r 21LO43    304  C~6DKi      
2022 04  08.33743  15 52 05.988  -20 32 55.99  24.3r 21LO43    304  C~6DKi      

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    -0.15       0.00     0.03
     2   0.0027    -46.58     0.23       1.54    -0.21
     3   0.2407  -1747.82     0.00     176.61     0.33
     4   0.2434  -1730.03     0.01     178.36     0.03
     5   0.2436  -1728.60    -0.09     178.40    -0.11
     6   0.7509   5700.40    -0.20     470.54     0.00
     7   0.8383   4977.62     0.03     513.69    -0.01
     8   0.8385   4976.13     0.17     513.69    -0.07

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.

21LO43    quality flag:0

Type:      ERR2LARGE ERR2LARGE ERR2LARGE

axisobj         0.000     0.000     0.000
ecceobj        -1.000    -1.000    -1.000
incobj         -1.000    -1.000    -1.000
qmin            0.000     0.000     0.000
qmax            0.000     0.000     0.000
amean           0.000     0.000     0.000
amin            0.000     0.000     0.000
amax            0.000     0.000     0.000
emean           0.000     0.000     0.000
emin            0.000     0.000     0.000
emax            0.000     0.000     0.000
imean           0.000     0.000     0.000
imin            0.000     0.000     0.000
imax            0.000     0.000     0.000
excite_mean     0.000     0.000     0.000
fracstop        0.000     0.000     0.000
cjmean          0.000     0.000     0.000

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         0.0       0.0       0.0
kozaiamp          0.0       0.0       0.0