Orbit Fit and Astrometric record for 22UO138

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: 22UO138   
# Created Tue May  7 01:18:15 2024
# Orbit generated from Bernstein formalism
# Fitting      4 observations of      4
# Arc:  16.89d
# First observation: 2022/10/29
#  Last observation: 2022/11/15
Preliminary a, adot, b, bdot, g, gdot:
  -0.000000   0.390615  -0.000001   0.093581   0.141850   0.000000
# WARNING MRQMIN stopped after  13 iterations -- oscilliatory solution
# WARNING Fitting with energy constraint
# WARNING MRQMIN stopped after  13 iterations -- oscilliatory solution
# WARNING MRQMIN stopped after  13 iterations -- oscilliatory solution
# Chi-squared of fit:     0.54 DOF:      3 RMS:  0.06
# Min/Max residuals:    -0.04    0.07
# Exact a, adot, b, bdot, g, gdot:
  3.924361E-05  3.258151E-01  1.056371E-05  8.891294E-02  1.315211E-01 -4.438810E-02
# Covariance matrix:
  3.9634E-11  2.9745E-07  3.1438E-13  2.3734E-08  5.0354E-08 -6.4508E-07
  2.9745E-07  2.3010E-03  2.5298E-09  1.8196E-04  3.8752E-04 -5.5658E-03
  3.1438E-13  2.5298E-09  7.4298E-13  1.7784E-10  4.1866E-10 -8.2666E-09
  2.3734E-08  1.8196E-04  1.7784E-10  1.4492E-05  3.0768E-05 -4.0422E-04
  5.0354E-08  3.8752E-04  4.1866E-10  3.0768E-05  6.5414E-05 -8.9388E-04
 -6.4508E-07 -5.5658E-03 -8.2666E-09 -4.0422E-04 -8.9388E-04  2.6096E-02
#      lat0       lon0       xBary       yBary       zBary        JD0
   10.342966   19.585795   -0.275663    0.169862   -0.931810  2459881.743381
# Heliocentric elements and errors
Epoch:              2459880.5000  =  2022/10/28
Mean Anomaly:          353.78075 +/-    22.640
Argument of Peri:       51.41320 +/-    76.219
Long of Asc Node:      350.17973 +/-     3.580
Inclination:            17.31550 +/-     1.829
Eccentricity:         0.46523099 +/-    0.3707
Semi-Major Axis:     15.71143608 +/-    8.0134
Time of Perihelion: 2460273.4685 +/-    1398.6
Perihelion:           8.40198911 +/-    7.2311
Aphelion:            23.02088304 +/-   13.1067
Period (y)               62.2776 +/-     47.65
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X            7.85595018 +/-    0.4334
Ecliptic Y            3.08418743 +/-    0.1542
Ecliptic Z            1.36517240 +/-    0.0840
Ecliptic XDOT        -0.00344323 +/-    0.0032
Ecliptic YDOT         0.00598295 +/-    0.0008
Ecliptic ZDOT         0.00165484 +/-    0.0006
# Distances at JD0 (AU)
Heliocenter to KBO    8.54937782 +/-    0.4023
Geocenter to KBO      7.60334399 +/-    0.4676
# Hcoef: 13.95

The following table shows the complete astrometric record for 22UO138. 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 (22UO138) followed by the observatory code and reference code for the source of the astrometry.

2022 10  29.24258  00 56 00.796  +17 12 41.46  23.0r 22UO138   568  C~6wt8      
2022 10  29.45024  00 55 57.026  +17 12 24.78  22.9r 22UO138   568  C~6wt8      
2022 11  15.12945  00 51 37.876  +16 50 01.95  23.5G 22UO138   G37  C~6wt8      
2022 11  15.13322  00 51 37.820  +16 50 01.56  23.1G 22UO138   G37  C~6wt8      

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     0.03
     2   0.0006    -56.23     0.05       5.85    -0.02
     3   0.0462  -4001.88     0.07     240.25     0.04
     4   0.0462  -4002.78    -0.04     240.21    -0.02

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.

22UO138    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