Orbit Fit and Astrometric record for 20UT74

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: 20UT74    
# 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   0.021274  -0.000000   0.001120   0.022694   0.000000
# Chi-squared of fit:    10.33 DOF:     10 RMS:  0.20
# Min/Max residuals:    -0.42    0.43
# Exact a, adot, b, bdot, g, gdot:
  1.495205E-05  2.117678E-02  7.543406E-07  1.112705E-03  2.249277E-02 -3.122252E-03
# Covariance matrix:
  8.4355E-13  5.0865E-11 -3.1963E-14  2.4222E-12  3.8894E-11  2.3885E-09
  5.0865E-11  5.5427E-09 -3.4495E-12  2.6163E-10  4.1951E-09  2.5805E-07
 -3.1963E-14 -3.4495E-12  3.7079E-13 -5.6246E-13 -2.6180E-12 -1.6073E-10
  2.4222E-12  2.6163E-10 -5.6246E-13  1.3214E-11  1.9830E-10  1.2187E-08
  3.8894E-11  4.1951E-09 -2.6180E-12  1.9830E-10  3.1867E-09  1.9553E-07
  2.3885E-09  2.5805E-07 -1.6073E-10  1.2187E-08  1.9553E-07  1.2019E-05
#      lat0       lon0       xBary       yBary       zBary        JD0
   -3.081440   -6.586443   -0.553319   -0.044395   -0.823640  2459142.505034
# Heliocentric elements and errors
Epoch:              2459140.5000  =  2020/10/18
Mean Anomaly:          296.80519 +/-     5.272
Argument of Peri:       33.50690 +/-    12.239
Long of Asc Node:       38.88802 +/-     0.047
Inclination:             4.29001 +/-     0.004
Eccentricity:         0.13849475 +/-    0.1657
Semi-Major Axis:     47.46786339 +/-    2.5479
Time of Perihelion: 2480109.4602 +/-     458.2
Perihelion:          40.89381356 +/-    8.1668
Aphelion:            54.04191321 +/-    8.3841
Period (y)              327.0452 +/-     26.33
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           44.99052630 +/-    0.1107
Ecliptic Y           -4.64282081 +/-    0.0128
Ecliptic Z           -2.38989595 +/-    0.0060
Ecliptic XDOT        -0.00006684 +/-    0.0004
Ecliptic YDOT         0.00260847 +/-    0.0000
Ecliptic ZDOT         0.00015546 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   45.29254734 +/-    0.1100
Geocenter to KBO     44.45873990 +/-    0.1116
# Hcoef:  9.11

The following table shows the complete astrometric record for 20UT74. 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 (20UT74) followed by the observatory code and reference code for the source of the astrometry.

2020 10  20.004233 23 40 42.428  -05 26 39.78  25.5r 20UT74    W84  C~7XOR      
2020 10  20.172968 23 40 41.839  -05 26 42.92  25.5r 20UT74    W84  C~7XOR      
2020 10  22.003924 23 40 35.692  -05 27 16.52  25.7r 20UT74    W84  C~7XOR      
2020 10  22.173214 23 40 35.130  -05 27 19.48  25.7r 20UT74    W84  C~7XOR      
2021 09  09.073508 23 47 50.788  -04 37 23.22  25.6r 20UT74    W84  C~7XOR      
2021 09  09.192572 23 47 50.256  -04 37 27.26  25.6r 20UT74    W84  C~7XOR      
2021 10  06.002765 23 45 59.580  -04 48 53.62  25.5r 20UT74    W84  C~7XOR      
2021 10  06.167954 23 45 58.929  -04 48 57.69  25.5r 20UT74    W84  C~7XOR      

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     0.01
     2   0.0005     -9.32    -0.03       0.61     0.03
     3   0.0055   -106.90    -0.07       6.20    -0.03
     4   0.0059   -115.78     0.11       6.82    -0.02
     5   0.8873   7051.28     0.43     163.17     0.41
     6   0.8876   7042.36    -0.42     162.64    -0.18
     7   0.9610   5249.80    -0.08     193.70     0.03
     8   0.9614   5239.25     0.08     193.85    -0.23

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.

20UT74    quality flag:1

Type:      CLASSICAL  CENTAURR CLASSICAL

axisobj        47.448    69.755    46.504
ecceobj         0.142     0.578     0.038
incobj          4.288     4.295     4.286
qmin           39.517    28.833    44.036
qmax           55.539   119.823    48.894
amean          47.261    71.358    46.349
amin           46.840    66.757    45.988
amax           47.755    74.662    46.725
emean           0.146     0.587     0.034
emin            0.131     0.562     0.022
emax            0.163     0.605     0.047
imean           3.737     4.227     3.681
imin            3.243     3.933     3.348
imax            4.248     5.250     4.014
excite_mean     0.160     0.592     0.073
fracstop        1.000     0.033     1.000
cjmean          3.110     2.905     3.124

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       171.1      87.5     174.2
kozaiamp        180.0      48.2     180.0