Orbit Fit and Astrometric record for 19GU186

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: 19GU186   
# Created Wed Dec 25 02:11:02 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     20 observations of     20
# Arc:   6.15y
# First observation: 2013/02/08
#  Last observation: 2019/04/05
# Chi-squared of fit:     6.52 DOF:     34 RMS:  0.10
# Min/Max residuals:    -0.21    0.30
# Exact a, adot, b, bdot, g, gdot:
  1.725274E-05  3.380371E-02 -7.635178E-06 -1.625493E-02  3.115122E-02  1.753731E-03
# Covariance matrix:
  4.7178E-13 -1.9053E-13 -3.2448E-14  5.7091E-14 -9.6829E-14 -5.4532E-13
 -1.9053E-13  2.4590E-13  6.1771E-14 -1.0893E-13  2.4798E-13  1.0397E-12
 -3.2448E-14  6.1771E-14  4.2576E-13 -1.0225E-13  5.6595E-14  2.8315E-13
  5.7091E-14 -1.0893E-13 -1.0225E-13  6.7900E-14 -1.0137E-13 -4.9864E-13
 -9.6829E-14  2.4798E-13  5.6595E-14 -1.0137E-13  6.4068E-13  9.6284E-13
 -5.4532E-13  1.0397E-12  2.8315E-13 -4.9864E-13  9.6284E-13  4.7615E-12
#      lat0       lon0       xBary       yBary       zBary        JD0
   -0.713731  156.849946    0.288543   -0.011680   -0.942548  2456331.972678
# Heliocentric elements and errors
Epoch:              2456332.5000  =  2013/02/09
Mean Anomaly:            8.03056 +/-     0.011
Argument of Peri:      168.73724 +/-     0.019
Long of Asc Node:      334.90225 +/-     0.000
Inclination:            25.67210 +/-     0.000
Eccentricity:         0.22101618 +/-    0.0001
Semi-Major Axis:     42.22832607 +/-    0.0050
Time of Perihelion: 2454096.6260 +/-       3.2
Perihelion:          32.89518296 +/-    0.0050
Aphelion:            51.56146919 +/-    0.0069
Period (y)              274.4189 +/-      0.05
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -30.26677043 +/-    0.0008
Ecliptic Y           13.25729145 +/-    0.0003
Ecliptic Z           -0.40013644 +/-    0.0000
Ecliptic XDOT        -0.00129957 +/-    0.0000
Ecliptic YDOT        -0.00267720 +/-    0.0000
Ecliptic ZDOT        -0.00143031 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   33.04529692 +/-    0.0007
Geocenter to KBO     32.10148211 +/-    0.0008
# Hcoef:  7.92

The following table shows the complete astrometric record for 19GU186. 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 (19GU186) followed by the observatory code and reference code for the source of the astrometry.

2013 02  08.471900 10 33 15.23   +08 20 02.0         19GU186   T09  C~89Vh      
2013 02  08.507764 10 33 15.02   +08 20 03.0         19GU186   T09  C~89Vh      
2013 02  08.553361 10 33 14.77   +08 20 04.1         19GU186   T09  C~89Vh      
2016 01  13.349187 10 52 43.38   +03 29 19.7   23.0r 19GU186   W84  C~89Vh      
2017 03  25.105213 10 52 08.16   +02 20 14.6         19GU186   W84  C~89Vh      
2017 03  25.19755  10 52 07.66   +02 20 17.0   23.7V 19GU186   W84  C~89Vh      
2017 03  26.11048  10 52 02.80   +02 20 41.3         19GU186   W84  C~89Vh      
2017 03  26.18767  10 52 02.38   +02 20 43.4         19GU186   W84  C~89Vh      
2019 01  04.608368 11 09 54.71   -01 09 08.3         19GU186   T09  C~89Vh      
2019 01  08.581323 11 09 45.26   -01 09 29.3         19GU186   T09  C~89Vh      
2019 02  27.281637 11 05 58.89   -00 59 20.3   23.1i 19GU186   W84  C~89Vh      
2019 03  15.33937  11 04 25.40   -00 52 09.5   22.7y 19GU186   T09  C~870m      
2019 03  15.38407  11 04 25.12   -00 52 08.5   22.7y 19GU186   T09  C~870m      
2019 03  15.38674  11 04 25.10   -00 52 08.5   22.6y 19GU186   T09  C~870m      
2019 03  15.42746  11 04 24.88   -00 52 07.4   22.7y 19GU186   T09  C~870m      
2019 03  15.46795  11 04 24.63   -00 52 06.2   22.6y 19GU186   T09  C~870m      
2019 03  15.51887  11 04 24.35   -00 52 04.7   22.7y 19GU186   T09  C~870m      
2019 04  05.42900  11 02 31.51   -00 42 13.6   23.2r 19GU186   T09  C~870m      
2019 04  05.46261  11 02 31.35   -00 42 12.8   23.3r 19GU186   T09  C~870m      
2019 04  05.50535  11 02 31.13   -00 42 11.6   23.3r 19GU186   T09  C~870m      

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    -0.07       0.00    -0.11
     2   0.0001      0.00    -0.08       0.00     0.05
     3   0.0002      0.00     0.16       0.00     0.08
     4   2.9264      0.00    -0.12       0.00     0.03
     5   4.1222      0.00    -0.03       0.00     0.02
     6   4.1225      0.00     0.03       0.00    -0.05
     7   4.1250      0.00     0.05       0.00    -0.04
     8   4.1252      0.00     0.01       0.00     0.01
     9   5.9032      0.00     0.04       0.00    -0.12
    10   5.9141      0.00     0.09       0.00    -0.04
    11   6.0501      0.00    -0.14       0.00    -0.13
    12   6.0941      0.00     0.13       0.00     0.30
    13   6.0942      0.00    -0.15       0.00     0.04
    14   6.0942      0.00    -0.21       0.00    -0.04
    15   6.0943      0.00     0.07       0.00    -0.09
    16   6.0944      0.00    -0.12       0.00    -0.03
    17   6.0946      0.00     0.15       0.00     0.03
    18   6.1518      0.00     0.01       0.00     0.10
    19   6.1519      0.00     0.13       0.00    -0.01
    20   6.1520      0.00     0.01       0.00     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.

19GU186    quality flag:3

Type:       SCATNEAR  SCATNEAR  SCATNEAR

axisobj        42.133    42.133    42.133
ecceobj         0.219     0.219     0.219
incobj         25.714    25.714    25.714
qmin           32.490    31.534    31.581
qmax           52.874    53.805    53.735
amean          42.326    42.326    42.325
amin           41.827    41.848    41.847
amax           42.882    42.882    42.882
emean           0.189     0.198     0.197
emin            0.136     0.139     0.131
emax            0.234     0.255     0.255
imean          27.236    27.065    27.041
imin           26.576    25.786    25.792
imax           27.858    28.381    28.384
excite_mean     0.496     0.497     0.496
fracstop        1.000     1.000     1.000
cjmean          2.781     2.779     2.780

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       209.8     183.7     187.4
kozaiamp        180.0     180.0     179.9