Orbit Fit and Astrometric record for 22LC14

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: 22LC14    
# Created Tue Apr  1 01:11:29 2025
# Orbit generated from Bernstein formalism
# Fitting     18 observations of     18
# Arc:   1.27y
# First observation: 2022/06/02
#  Last observation: 2023/09/10
Preliminary a, adot, b, bdot, g, gdot:
   0.000001   0.030057   0.000000   0.000850   0.027542   0.000000
# Chi-squared of fit:     1.61 DOF:     30 RMS:  0.05
# Min/Max residuals:    -0.09    0.10
# Exact a, adot, b, bdot, g, gdot:
  1.720992E-05  2.988106E-02  4.323055E-08  8.614290E-04  2.740850E-02  4.952259E-03
# Covariance matrix:
  2.5900E-13  6.2483E-13 -1.1846E-14  3.2391E-13  1.2457E-12  3.1334E-10
  6.2483E-13  4.4722E-12 -2.1316E-14  5.0326E-13  4.9561E-12  4.7648E-10
 -1.1846E-14 -2.1316E-14  1.5771E-13 -9.2336E-13 -1.3528E-12 -7.9493E-10
  3.2391E-13  5.0326E-13 -9.2336E-13  2.3910E-11  3.9146E-11  2.3070E-08
  1.2457E-12  4.9561E-12 -1.3528E-12  3.9146E-11  6.8789E-11  3.8148E-08
  3.1334E-10  4.7648E-10 -7.9493E-10  2.3070E-08  3.8148E-08  2.2490E-05
#      lat0       lon0       xBary       yBary       zBary        JD0
    0.593212  -72.696577    0.599974    0.008209   -0.818864  2459732.944521
# Heliocentric elements and errors
Epoch:              2459730.5000  =  2022/05/31
Mean Anomaly:           34.05998 +/-    14.727
Argument of Peri:      328.04922 +/-    29.297
Long of Asc Node:      267.08932 +/-     0.079
Inclination:             1.75433 +/-     0.007
Eccentricity:         0.21280829 +/-    0.1428
Semi-Major Axis:     44.28738569 +/-    2.9909
Time of Perihelion: 2449545.5152 +/-    4281.4
Perihelion:          34.86266271 +/-    6.7489
Aphelion:            53.71210868 +/-    7.2913
Period (y)              294.7327 +/-     29.86
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           10.53155295 +/-    0.0033
Ecliptic Y          -35.79409199 +/-    0.0105
Ecliptic Z            0.37781902 +/-    0.0001
Ecliptic XDOT         0.00299836 +/-    0.0001
Ecliptic YDOT         0.00042537 +/-    0.0005
Ecliptic ZDOT         0.00009105 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   37.31317966 +/-    0.0102
Geocenter to KBO     36.48503007 +/-    0.0110
# Hcoef: 10.32

The following table shows the complete astrometric record for 22LC14. 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 (22LC14) followed by the observatory code and reference code for the source of the astrometry.

2022 06  02.44372  19 14 41.577  -21 43 52.98  26.1r 22LC14    266  C~6IpZ      
2022 06  02.53086  19 14 41.192  -21 43 53.58  26.1r 22LC14    266  C~6IpZ      
2022 06  02.61096  19 14 40.837  -21 43 54.11  26.1r 22LC14    266  C~6IpZ      
2022 06  03.44086  19 14 37.240  -21 43 59.76  26.0r 22LC14    266  C~6IpZ      
2022 06  03.52767  19 14 36.850  -21 44 00.36  26.0r 22LC14    266  C~6IpZ      
2022 06  03.61505  19 14 36.458  -21 44 00.95  26.0r 22LC14    266  C~6IpZ      
2022 06  29.45230  19 12 25.362  -21 47 29.39  26.0r 22LC14    266  C~6IpZ      
2022 06  29.51813  19 12 24.990  -21 47 29.97  26.0r 22LC14    266  C~6IpZ      
2022 06  29.58257  19 12 24.627  -21 47 30.53  26.0r 22LC14    266  C~6IpZ      
2022 06  30.45132  19 12 19.808  -21 47 38.39  25.7r 22LC14    266  C~6IpZ      
2022 06  30.52034  19 12 19.417  -21 47 39.01  25.7r 22LC14    266  C~6IpZ      
2022 06  30.58668  19 12 19.042  -21 47 39.59  25.7r 22LC14    266  C~6IpZ      
2023 09  09.22891  19 14 12.953  -21 41 16.78        22LC14    266  C~8ecH      
2023 09  09.32430  19 14 12.729  -21 41 17.20        22LC14    266  C~8ecH      
2023 09  09.41985  19 14 12.507  -21 41 17.59        22LC14    266  C~8ecH      
2023 09  10.22905  19 14 10.771  -21 41 21.30        22LC14    266  C~8ecH      
2023 09  10.32490  19 14 10.555  -21 41 21.71        22LC14    266  C~8ecH      
2023 09  10.42059  19 14 10.342  -21 41 22.08        22LC14    266  C~8ecH      

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     0.09
     2   0.0002     -5.40     0.00       0.09     0.09
     3   0.0005    -10.37    -0.01       0.19     0.08
     4   0.0027    -60.80     0.01       0.97    -0.00
     5   0.0030    -66.27    -0.00       1.06     0.00
     6   0.0032    -71.76     0.00       1.17    -0.01
     7   0.0739  -1909.82     0.00      23.53    -0.03
     8   0.0741  -1915.04     0.00      23.60    -0.03
     9   0.0743  -1920.12     0.01      23.67    -0.03
    10   0.0767  -1987.71    -0.01      24.17    -0.06
    11   0.0769  -1993.19    -0.00      24.23    -0.06
    12   0.0771  -1998.44    -0.00      24.30    -0.06
    13   1.2698   -375.84    -0.02     205.59     0.09
    14   1.2700   -378.99    -0.04     205.57     0.09
    15   1.2703   -382.11    -0.06     205.57     0.10
    16   1.2725   -406.58     0.07     204.96    -0.09
    17   1.2728   -409.62     0.04     204.93    -0.09
    18   1.2730   -412.61     0.01     204.94    -0.08

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.

22LC14    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