Orbit Fit and Astrometric record for 20UG74

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: 20UG74    
# Created Tue Apr  1 01:11:22 2025
# Orbit generated from Bernstein formalism
# Fitting      8 observations of      8
# Arc:   0.96y
# First observation: 2020/10/20
#  Last observation: 2021/10/06
Preliminary a, adot, b, bdot, g, gdot:
   0.000003   0.024660  -0.000001  -0.000408   0.024710   0.000000
# Chi-squared of fit:     0.80 DOF:     10 RMS:  0.06
# Min/Max residuals:    -0.08    0.10
# Exact a, adot, b, bdot, g, gdot:
  1.559907E-05  2.462014E-02 -7.477668E-07 -4.069585E-04  2.452857E-02 -1.112014E-05
# Covariance matrix:
  8.6980E-13  5.9297E-11 -1.8556E-14 -9.7514E-13  4.2056E-11  2.4014E-09
  5.9297E-11  7.1219E-09 -2.2088E-12 -1.1632E-10  5.0068E-09  2.8631E-07
 -1.8556E-14 -2.2088E-12  3.6939E-13 -3.6347E-13 -1.5580E-12 -8.8880E-11
 -9.7514E-13 -1.1632E-10 -3.6347E-13  2.7598E-12 -8.1786E-11 -4.6768E-09
  4.2056E-11  5.0068E-09 -1.5580E-12 -8.1786E-11  3.5310E-09  2.0146E-07
  2.4014E-09  2.8631E-07 -8.8880E-11 -4.6768E-09  2.0146E-07  1.1514E-05
#      lat0       lon0       xBary       yBary       zBary        JD0
   -2.756728   -6.494019   -0.551988   -0.039769   -0.824769  2459142.505034
# Heliocentric elements and errors
Epoch:              2459140.5000  =  2020/10/18
Mean Anomaly:           11.86074 +/-   104.329
Argument of Peri:      237.82134 +/-   120.548
Long of Asc Node:      102.83713 +/-     0.182
Inclination:             2.84969 +/-     0.003
Eccentricity:         0.06830937 +/-    0.0304
Semi-Major Axis:     44.57397101 +/-    0.0999
Time of Perihelion: 2455559.2901 +/-   31500.8
Perihelion:          41.52915130 +/-    1.3592
Aphelion:            47.61879072 +/-    1.3602
Period (y)              297.5981 +/-      1.00
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           41.34939415 +/-    0.0980
Ecliptic Y           -4.15630487 +/-    0.0112
Ecliptic Z           -1.96085665 +/-    0.0047
Ecliptic XDOT         0.00031466 +/-    0.0004
Ecliptic YDOT         0.00273595 +/-    0.0000
Ecliptic ZDOT        -0.00004553 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   41.60399290 +/-    0.0974
Geocenter to KBO     40.76879089 +/-    0.0988
# Hcoef:  8.49

The following table shows the complete astrometric record for 20UG74. 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 (20UG74) followed by the observatory code and reference code for the source of the astrometry.

2020 10  20.004233 23 40 31.788  -05 06 34.94  24.6r 20UG74    W84  C~7XOQ      
2020 10  20.172968 23 40 31.158  -05 06 38.69  24.6r 20UG74    W84  C~7XOQ      
2020 10  22.003924 23 40 24.611  -05 07 16.61  24.6r 20UG74    W84  C~7XOQ      
2020 10  22.173214 23 40 23.996  -05 07 20.16  24.6r 20UG74    W84  C~7XOQ      
2021 09  09.073508 23 48 42.565  -04 15 36.21  24.6r 20UG74    W84  C~7XOQ      
2021 09  09.192572 23 48 42.043  -04 15 39.83  24.6r 20UG74    W84  C~7XOQ      
2021 10  06.002765 23 46 43.666  -04 28 22.37  24.6r 20UG74    W84  C~7XOQ      
2021 10  06.167954 23 46 42.947  -04 28 26.82  24.6r 20UG74    W84  C~7XOQ      

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     0.06       0.00     0.10
     2   0.0005    -10.13    -0.06       0.29    -0.04
     3   0.0055   -114.96     0.05       4.30     0.01
     4   0.0059   -124.80    -0.05       4.68    -0.06
     5   0.8873   7952.14    -0.03    -115.70     0.08
     6   0.8876   7943.52     0.03    -115.90    -0.08
     7   0.9610   6013.58     0.05    -108.29     0.03
     8   0.9614   6001.94    -0.05    -108.09    -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.

20UG74    quality flag:1

Type:      CLASSICAL   REMOVED CLASSICAL

axisobj        44.477    52.318    44.334
ecceobj         0.067     0.378     0.063
incobj          2.853     2.863     2.851
qmin           40.760    30.180    40.507
qmax           48.213    73.470    48.102
amean          44.344    46.838    44.197
amin           43.991    40.695    43.854
amax           44.720    52.967    44.570
emean           0.063     0.328     0.064
emin            0.047     0.245     0.048
emax            0.078     0.390     0.079
imean           1.304     1.640     1.378
imin            0.642     0.578     0.627
imax            1.919     2.756     2.027
excite_mean     0.067     0.329     0.069
fracstop        1.000     0.157     1.000
cjmean          3.100     2.997     3.098

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       157.9     190.6     169.2
kozaiamp        179.8     179.5     180.0