Orbit Fit and Astrometric record for 21QB98

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: 21QB98    
# Created Wed May  8 01:18:44 2024
# Orbit generated from Bernstein formalism
# Fitting      6 observations of      6
# Arc:   1.22y
# First observation: 2021/08/29
#  Last observation: 2022/11/19
Preliminary a, adot, b, bdot, g, gdot:
   0.000001   0.010755  -0.000001  -0.000693   0.016080   0.000000
# Chi-squared of fit:     2.11 DOF:      6 RMS:  0.10
# Min/Max residuals:    -0.15    0.17
# Exact a, adot, b, bdot, g, gdot:
  1.118541E-05  1.068588E-02 -1.157050E-06 -6.946089E-04  1.596865E-02 -6.614963E-03
# Covariance matrix:
  1.0488E-12  2.4896E-11  3.7549E-14 -1.9315E-12  3.8193E-11  2.3825E-09
  2.4896E-11  2.0716E-09  3.0189E-12 -1.5595E-10  3.1000E-09  1.9249E-07
  3.7549E-14  3.0189E-12  7.2996E-13 -8.8747E-13  4.5171E-12  2.8088E-10
 -1.9315E-12 -1.5595E-10 -8.8747E-13  1.2655E-11 -2.3340E-10 -1.4502E-08
  3.8193E-11  3.1000E-09  4.5171E-12 -2.3340E-10  4.6415E-09  2.8811E-07
  2.3825E-09  1.9249E-07  2.8088E-10 -1.4502E-08  2.8811E-07  1.7899E-05
#      lat0       lon0       xBary       yBary       zBary        JD0
    1.097396  -34.053712   -0.169889    0.018726   -0.986116  2459455.595561
# Heliocentric elements and errors
Epoch:              2459450.5000  =  2021/08/24
Mean Anomaly:          300.81575 +/-    38.527
Argument of Peri:      284.38840 +/-    16.808
Long of Asc Node:      162.29729 +/-     0.020
Inclination:             3.86707 +/-     0.005
Eccentricity:         0.52150872 +/-    0.2494
Semi-Major Axis:     64.17269885 +/-   23.6010
Time of Perihelion: 2490319.8543 +/-   10668.1
Perihelion:          30.70607657 +/-   19.5855
Aphelion:            97.63932114 +/-   39.3132
Period (y)              514.0835 +/-    283.60
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           52.79497072 +/-    0.2213
Ecliptic Y          -35.47573018 +/-    0.1496
Ecliptic Z            1.19928771 +/-    0.0051
Ecliptic XDOT         0.00009319 +/-    0.0006
Ecliptic YDOT         0.00215940 +/-    0.0004
Ecliptic ZDOT        -0.00014097 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   63.61819438 +/-    0.2017
Geocenter to KBO     62.62271887 +/-    0.2672
# Hcoef:  6.45

The following table shows the complete astrometric record for 21QB98. 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 (21QB98) followed by the observatory code and reference code for the source of the astrometry.

2021 08  29.09476  21 51 16.286  -11 50 13.75  24.4r 21QB98    807  C~6DKv      
2021 08  30.09939  21 51 13.162  -11 50 30.98  24.3r 21QB98    807  C~6DKv      
2022 09  02.23398  21 53 30.304  -11 41 03.66  24.4r 21QB98    304  C~6DKv      
2022 09  03.24759  21 53 27.143  -11 41 21.21  24.5r 21QB98    304  C~6DKv      
2022 10  16.02476  21 51 41.908  -11 51 20.98  24.3r 21QB98    304  C~6DKv      
2022 11  19.03098  21 51 22.759  -11 53 51.06  24.4r 21QB98    304  C~6DKv      

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    -0.12       0.00     0.10
     2   0.0028    -48.99     0.13      -0.78    -0.09
     3   1.0106   2038.29     0.17    -146.76     0.03
     4   1.0134   1988.65    -0.15    -147.56    -0.09
     5   1.1305    331.50    -0.12    -190.02     0.04
     6   1.2236     16.29     0.09    -236.62     0.01

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.

21QB98    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