Orbit Fit and Astrometric record for 21DR15

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: 21DR15    
# Created Thu Apr 25 01:18:46 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     21 observations of     21
# Arc:  16.74y
# First observation: 2005/03/10
#  Last observation: 2021/12/06
# Chi-squared of fit:    15.95 DOF:     36 RMS:  0.15
# Min/Max residuals:    -0.34    0.33
# Exact a, adot, b, bdot, g, gdot:
  7.790912E-06  5.439653E-03 -4.048040E-06 -3.150817E-03  1.166988E-02  2.236428E-03
# Covariance matrix:
  5.3048E-13 -9.0088E-14 -6.5326E-14  3.5215E-14 -2.0281E-13 -6.9333E-13
 -9.0088E-14  2.7356E-14  2.4593E-14 -1.3585E-14  5.1153E-14  2.6807E-13
 -6.5326E-14  2.4593E-14  3.5201E-13 -3.7088E-14  5.1197E-14  2.6208E-13
  3.5215E-14 -1.3585E-14 -3.7088E-14  9.5805E-15 -2.6148E-14 -1.4521E-13
 -2.0281E-13  5.1153E-14  5.1197E-14 -2.6148E-14  2.7038E-13  5.1215E-13
 -6.9333E-13  2.6807E-13  2.6208E-13 -1.4521E-13  5.1215E-13  2.8660E-12
#      lat0       lon0       xBary       yBary       zBary        JD0
    4.998474  145.430820   -0.405941    0.078674   -0.898471  2453439.771654
# Heliocentric elements and errors
Epoch:              2453440.5000  =  2005/03/11
Mean Anomaly:          112.45634 +/-     0.030
Argument of Peri:       22.42688 +/-     0.019
Long of Asc Node:      334.19299 +/-     0.000
Inclination:            30.37608 +/-     0.000
Eccentricity:         0.42726651 +/-    0.0001
Semi-Major Axis:     67.65083048 +/-    0.0074
Time of Perihelion: 2389952.8017 +/-      19.7
Perihelion:          38.74589646 +/-    0.0084
Aphelion:            96.55576451 +/-    0.0129
Period (y)              556.4394 +/-      0.09
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -71.27063904 +/-    0.0032
Ecliptic Y           48.61280394 +/-    0.0021
Ecliptic Z            7.46582954 +/-    0.0003
Ecliptic XDOT        -0.00120747 +/-    0.0000
Ecliptic YDOT        -0.00072489 +/-    0.0000
Ecliptic ZDOT        -0.00069062 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   86.59331485 +/-    0.0029
Geocenter to KBO     85.69044998 +/-    0.0038
# Hcoef:  3.52

The following table shows the complete astrometric record for 21DR15. 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 (21DR15) followed by the observatory code and reference code for the source of the astrometry.

2005 03  10.270911 09 57 50.76   +17 44 41.8   22.6r 21DR15    645  C~5WCx      
2005 03  10.271740 09 57 50.76   +17 44 42.1   22.5i 21DR15    645  C~5WCx      
2005 12  06.478940 10 02 00.36   +17 12 03.2   23.0r 21DR15    645  C~5WCx      
2005 12  06.482257 10 02 00.37   +17 12 03.3   23.3g 21DR15    645  C~5WCx      
2013 04  30.035817 10 03 57.41   +15 38 07.4   23.4g 21DR15    W84  C~5WCx      
2013 04  30.043112 10 03 57.40   +15 38 07.6   23.4g 21DR15    W84  C~5WCx      
2016 01  17.244632 10 10 11.07   +14 35 17.5   23.6g 21DR15    W84  C~5WCx      
2016 01  17.245846 10 10 11.08   +14 35 17.4   22.8r 21DR15    W84  C~5WCx      
2016 02  29.265745 10 08 29.01   +14 43 36.5   22.7z 21DR15    W84  C~5WCx      
2016 02  29.270989 10 08 29.01   +14 43 36.7   22.7z 21DR15    W84  C~5WCx      
2017 03  29.052341 10 08 19.10   +14 32 07.1   22.8r 21DR15    W84  C~5WCx      
2018 03  17.165605 10 09 37.78   +14 14 28.8   23.4g 21DR15    W84  C~5WCx      
2018 03  18.141881 10 09 35.63   +14 14 38.2   23.1r 21DR15    W84  C~5WCx      
2019 03  07.209111 10 10 54.20   +13 56 52.2   23.0i 21DR15    W84  C~5WCx      
2021 02  17.28970  10 13 20.863  +13 21 55.80  22.8r 21DR15    568  C~5Jzg      
2021 02  17.35720  10 13 20.694  +13 21 56.74  22.7r 21DR15    568  C~5Jzg      
2021 04  06.99144  10 11 33.799  +13 29 52.67  23.2r 21DR15    304  C~5Jzg      
2021 04  08.99105  10 11 30.559  +13 30 04.69  23.2r 21DR15    304  C~5Jzg      
2021 04  13.19509  10 11 24.133  +13 30 27.38  23.0r 21DR15    304  C~5Jzg      
2021 12  02.33674  10 16 17.730  +12 55 36.25  22.9r 21DR15    304  C~5Jzg      
2021 12  06.33769  10 16 16.432  +12 55 42.53  23.0r 21DR15    304  C~5Jzg      

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    -0.10       0.00    -0.01
     2   0.0000      0.00    -0.07       0.00     0.28
     3   0.7425      0.00     0.09       0.00    -0.13
     4   0.7425      0.00     0.28       0.00    -0.04
     5   8.1390      0.00     0.05       0.00    -0.21
     6   8.1390      0.00    -0.01       0.00    -0.01
     7  10.8555      0.00    -0.34       0.00     0.10
     8  10.8555      0.00    -0.16       0.00    -0.01
     9  10.9733      0.00    -0.14       0.00    -0.28
    10  10.9733      0.00     0.05       0.00    -0.13
    11  12.0514      0.00    -0.10       0.00     0.22
    12  13.0182      0.00    -0.03       0.00     0.04
    13  13.0209      0.00     0.03       0.00     0.29
    14  13.9902      0.00    -0.08       0.00     0.01
    15  15.9426      0.00    -0.12       0.00    -0.06
    16  15.9427      0.00    -0.14       0.00     0.07
    17  16.0759      0.00     0.10       0.00    -0.09
    18  16.0814      0.00     0.33       0.00    -0.10
    19  16.0929      0.00     0.12       0.00    -0.05
    20  16.7312      0.00    -0.07       0.00     0.08
    21  16.7421      0.00     0.31       0.00     0.04

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.

21DR15    quality flag:3

Type:       SCATNEAR  SCATNEAR  SCATNEAR

axisobj        67.544    67.544    67.544
ecceobj         0.435     0.435     0.435
incobj         30.580    30.580    30.580
qmin           36.519    36.516    36.538
qmax          100.059    99.978   100.098
amean          67.502    67.511    67.502
amin           66.706    66.706    66.692
amax           68.648    68.644    68.648
emean           0.440     0.440     0.440
emin            0.421     0.421     0.421
emax            0.458     0.458     0.458
imean          31.129    31.131    31.127
imin           30.591    30.600    30.595
imax           31.903    31.892    31.900
excite_mean     0.679     0.679     0.679
fracstop        1.000     1.000     1.000
cjmean          2.747     2.747     2.747

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       164.0     163.7     164.0
kozaiamp        140.5     140.1     140.5