Orbit Fit and Astrometric record for 19SJ187

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: 19SJ187   
# Created Thu Apr 25 01:18:30 2024
# Orbit generated from Bernstein formalism
# Fitting      6 observations of      6
# Arc:   1.94y
# First observation: 2019/09/26
#  Last observation: 2021/09/03
Preliminary a, adot, b, bdot, g, gdot:
  -0.000008   0.012174  -0.000019   0.003170   0.016294   0.000000
# Chi-squared of fit:     0.92 DOF:      6 RMS:  0.07
# Min/Max residuals:    -0.10    0.09
# Exact a, adot, b, bdot, g, gdot:
  1.191092E-05  1.191436E-02  3.398855E-06  3.117938E-03  1.640496E-02 -6.927301E-03
# Covariance matrix:
  7.2971E-13 -3.0757E-12 -9.5927E-15 -5.0097E-13  1.5571E-13 -8.9715E-11
 -3.0757E-12  1.4605E-10 -6.1582E-12  3.2826E-11  4.7749E-11  5.1717E-09
 -9.5927E-15 -6.1582E-12  7.3183E-13 -1.6829E-12 -2.5500E-12 -2.2411E-10
 -5.0097E-13  3.2826E-11 -1.6829E-12  7.7833E-12  1.1332E-11  1.1710E-09
  1.5571E-13  4.7749E-11 -2.5500E-12  1.1332E-11  2.0105E-11  1.7411E-09
 -8.9715E-11  5.1717E-09 -2.2411E-10  1.1710E-09  1.7411E-09  1.8402E-07
#      lat0       lon0       xBary       yBary       zBary        JD0
  -15.452248  -24.237593   -0.455455   -0.237254   -0.858341  2458752.559271
# Heliocentric elements and errors
Epoch:              2458750.5000  =  2019/09/24
Mean Anomaly:          316.05628 +/-     2.992
Argument of Peri:       55.44726 +/-     0.668
Long of Asc Node:       20.91727 +/-     0.013
Inclination:            21.15234 +/-     0.004
Eccentricity:         0.50075559 +/-    0.0304
Semi-Major Axis:     73.80587758 +/-    2.9661
Time of Perihelion: 2487020.7176 +/-     894.3
Perihelion:          36.84717169 +/-    2.6885
Aphelion:           110.76458347 +/-    4.9850
Period (y)              634.0808 +/-     38.22
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           54.57700540 +/-    0.0147
Ecliptic Y          -24.07689094 +/-    0.0066
Ecliptic Z          -16.24095425 +/-    0.0044
Ecliptic XDOT        -0.00006490 +/-    0.0001
Ecliptic YDOT         0.00221456 +/-    0.0000
Ecliptic ZDOT         0.00080935 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   61.82325445 +/-    0.0132
Geocenter to KBO     60.95719028 +/-    0.0167
# Hcoef:  6.39

The following table shows the complete astrometric record for 19SJ187. 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 (19SJ187) followed by the observatory code and reference code for the source of the astrometry.

2019 09  26.05847  22 54 47.365  -23 41 36.36  24.2r 19SJ187   807  C~5JzT      
2019 09  26.25496  22 54 46.724  -23 41 38.00  24.1r 19SJ187   807  C~5JzT      
2019 11  29.05293  22 52 49.645  -23 36 33.11  24.2r 19SJ187   304  C~5JzT      
2019 11  30.05204  22 52 49.739  -23 36 14.21  24.3r 19SJ187   304  C~5JzT      
2021 09  02.20328  23 01 02.582  -22 42 39.38  24.3r 19SJ187   304  C~5JzT      
2021 09  03.15306  23 00 59.256  -22 42 56.31  24.2r 19SJ187   304  C~5JzT      

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    -0.09       0.00    -0.08
     2   0.0005     -8.73     0.09       1.98     0.08
     3   0.1752  -1366.67    -0.02     916.80     0.07
     4   0.1779  -1358.05     0.02     933.68    -0.07
     5   1.9361   6159.12     0.03    1165.67    -0.10
     6   1.9387   6110.14    -0.03    1168.88     0.09

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.

19SJ187    quality flag:1

Type:       SCATNEAR  SCATNEAR  SCATNEAR

axisobj        74.207    84.928    67.156
ecceobj         0.506     0.593     0.420
incobj         21.092    21.102    21.082
qmin           35.648    33.438    38.033
qmax          113.741   138.123    96.985
amean          73.699    84.085    66.817
amin           72.644    82.683    65.990
amax           75.195    86.176    67.903
emean           0.499     0.587     0.415
emin            0.484     0.576     0.400
emax            0.515     0.604     0.430
imean          21.435    21.310    21.251
imin           20.631    20.266    20.713
imax           22.291    21.825    21.891
excite_mean     0.619     0.691     0.551
fracstop        1.000     1.000     1.000
cjmean          2.932     2.878     2.977

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       194.8      98.8     166.4
kozaiamp        180.0      47.6     179.9