Orbit Fit and Astrometric record for 14QG442

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: 14QG442   
# Created Wed Dec 25 02:09:54 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     50 observations of     50
# Arc:   8.35y
# First observation: 2014/08/19
#  Last observation: 2022/12/26
# Chi-squared of fit:    41.11 DOF:     94 RMS:  0.16
# Min/Max residuals:    -0.56    0.47
# Exact a, adot, b, bdot, g, gdot:
  1.705460E-05  2.690433E-02  5.313813E-06  8.363895E-03  2.578997E-02  7.993653E-03
# Covariance matrix:
  1.0047E-13  4.1755E-14  1.8310E-14  9.7350E-15  1.0403E-13  1.8848E-13
  4.1755E-14  1.7165E-13  1.2644E-14  4.9019E-14  1.4695E-13  8.5604E-13
  1.8310E-14  1.2644E-14  4.1994E-14 -5.0582E-15  2.9103E-14  4.5869E-14
  9.7350E-15  4.9019E-14 -5.0582E-15  2.2921E-14  3.7883E-14  2.6292E-13
  1.0403E-13  1.4695E-13  2.9103E-14  3.7883E-14  2.0515E-13  6.8419E-13
  1.8848E-13  8.5604E-13  4.5869E-14  2.6292E-13  6.8419E-13  4.5659E-12
#      lat0       lon0       xBary       yBary       zBary        JD0
  -26.201187   41.362456    0.981078   -0.114351   -0.232684  2456888.924841
# Heliocentric elements and errors
Epoch:              2456888.5000  =  2014/08/19
Mean Anomaly:           27.57814 +/-     0.004
Argument of Peri:      242.24308 +/-     0.009
Long of Asc Node:       95.98267 +/-     0.000
Inclination:            30.43182 +/-     0.000
Eccentricity:         0.36291080 +/-    0.0001
Semi-Major Axis:     53.64391399 +/-    0.0044
Time of Perihelion: 2445894.8591 +/-       2.1
Perihelion:          34.17595825 +/-    0.0049
Aphelion:            73.11186974 +/-    0.0072
Period (y)              392.9062 +/-      0.05
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           26.95219965 +/-    0.0005
Ecliptic Y           22.42739205 +/-    0.0004
Ecliptic Z          -17.11983422 +/-    0.0003
Ecliptic XDOT        -0.00102658 +/-    0.0000
Ecliptic YDOT         0.00290159 +/-    0.0000
Ecliptic ZDOT         0.00042211 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   39.01902400 +/-    0.0004
Geocenter to KBO     38.77460658 +/-    0.0007
# Hcoef:  6.69

The following table shows the complete astrometric record for 14QG442. 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 (14QG442) followed by the observatory code and reference code for the source of the astrometry.

2014 08  19.424063 03 07 35.85   -09 44 37.2   22.3i 14QG442   W84  C~352Q      
2014 08  19.424583 03 07 35.84   -09 44 36.9   22.6i 14QG442   W84  C~2Bnh      
2014 08  19.42459  03 07 35.855  -09 44 37.15  22.6i 14QG442   W84  C~4yTx      
2014 09  04.374977 03 07 25.20   -09 54 24.5   22.9g 14QG442   W84  C~352Q      
2014 09  04.37550  03 07 25.200  -09 54 24.46  22.9g 14QG442   W84  C~4yTx      
2014 09  04.376343 03 07 25.20   -09 54 24.5   22.5r 14QG442   W84  C~352Q      
2014 09  04.37687  03 07 25.198  -09 54 24.47  22.5r 14QG442   W84  C~4yTx      
2014 09  27.310683 03 06 28.63   -10 08 57.5   22.7g 14QG442   W84  C~352Q      
2014 09  27.311204 03 06 28.65   -10 08 57.2   22.8g 14QG442   W84  C~2Bnh      
2014 09  27.31121  03 06 28.632  -10 08 57.49  23.1g 14QG442   W84  C~4yTx      
2014 09  27.312060 03 06 28.63   -10 08 57.6   22.4r 14QG442   W84  C~352Q      
2014 09  27.31258  03 06 28.630  -10 08 57.57  22.6r 14QG442   W84  C~4yTx      
2014 09  27.312581 03 06 28.64   -10 08 57.4   22.6r 14QG442   W84  C~2Bnh      
2014 09  27.313426 03 06 28.61   -10 08 57.7   22.2i 14QG442   W84  C~352Q      
2014 09  27.313947 03 06 28.63   -10 08 57.5   22.5i 14QG442   W84  C~2Bnh      
2014 09  27.31395  03 06 28.615  -10 08 57.66  22.3i 14QG442   W84  C~4yTx      
2014 10  14.36212  03 05 20.574  -10 18 36.99  22.3z 14QG442   W84  C~4yTx      
2014 10  21.356875 03 04 47.98   -10 21 59.1   22.6r 14QG442   W84  C~352Q      
2014 10  21.357396 03 04 47.98   -10 21 59.4   22.6r 14QG442   W84  C~2Bnh      
2014 10  21.35740  03 04 47.984  -10 21 59.11  22.7r 14QG442   W84  C~4yTx      
2014 10  21.358241 03 04 47.98   -10 21 59.3   22.4i 14QG442   W84  C~352Q      
2014 10  21.358762 03 04 47.97   -10 21 59.5   22.8i 14QG442   W84  C~2Bnh      
2014 10  21.35877  03 04 47.975  -10 21 59.26  22.6i 14QG442   W84  C~4yTx      
2014 10  21.360984 03 04 47.96   -10 21 59.2   22.3z 14QG442   W84  C~352Q      
2014 10  21.361505 03 04 47.96   -10 21 59.2   23.1z 14QG442   W84  C~2Bnh      
2014 10  21.36151  03 04 47.960  -10 21 59.20  22.5z 14QG442   W84  C~4yTx      
2014 10  23.349977 03 04 38.32   -10 22 51.8   22.8g 14QG442   W84  C~352Q      
2014 10  23.350498 03 04 38.32   -10 22 51.9   23.4g 14QG442   W84  C~2Bnh      
2014 10  23.35050  03 04 38.323  -10 22 51.83  23.1g 14QG442   W84  C~4yTx      
2014 10  23.351331 03 04 38.32   -10 22 51.8   22.2i 14QG442   W84  C~352Q      
2014 10  23.351852 03 04 38.32   -10 22 51.8   22.3i 14QG442   W84  C~2Bnh      
2014 10  23.35186  03 04 38.316  -10 22 51.74  22.6i 14QG442   W84  C~4yTx      
2014 10  28.33621  03 04 13.576  -10 24 53.36  22.7i 14QG442   W84  C~4yTx      
2014 12  12.21368  03 00 31.239  -10 29 11.63  22.6z 14QG442   W84  C~4yTx      
2015 02  09.039525 02 58 46.39   -09 55 14.0   22.8z 14QG442   W84  C~352Q      
2015 12  19.10845  03 05 30.988  -09 32 07.70  22.7z 14QG442   W84  C~4yTx      
2016 01  02.121701 03 04 43.95   -09 26 49.4   22.5r 14QG442   W84  C~352Q      
2016 01  02.122222 03 04 43.96   -09 26 49.0   22.7r 14QG442   W84  C~2Bnh      
2016 01  02.12223  03 04 43.947  -09 26 49.38  22.5r 14QG442   W84  C~4yTx      
2016 01  02.123067 03 04 43.94   -09 26 49.5   22.6i 14QG442   W84  C~352Q      
2016 01  02.123576 03 04 43.97   -09 26 48.9   22.4i 14QG442   W84  C~2Bnh      
2016 01  02.12359  03 04 43.943  -09 26 49.47  22.3i 14QG442   W84  C~4yTy      
2016 01  02.124433 03 04 43.92   -09 26 49.4   23.2g 14QG442   W84  C~352Q      
2016 01  02.124942 03 04 43.93   -09 26 49.0   22.7g 14QG442   W84  C~2Bnh      
2016 01  02.12496  03 04 43.927  -09 26 49.38  22.9g 14QG442   W84  C~4yTy      
2017 12  20.28361  03 15 57.539  -07 42 32.69  22.4R 14QG442   G37  C~2Uxc      
2017 12  20.36026  03 15 57.233  -07 42 31.49        14QG442   G37  C~2Uxc      
2022 12  26.130200 03 40 20.882  -03 18 15.74  22.9G 14QG442   G37  C~69bF      
2022 12  26.183060 03 40 20.680  -03 18 15.16        14QG442   G37  C~69bF      
2022 12  26.246070 03 40 20.375  -03 18 14.62        14QG442   G37  C~69bF      

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    -0.07
     2   0.0000      0.00    -0.25       0.00     0.25
     3   0.0000      0.00    -0.02       0.00    -0.00
     4   0.0437      0.00     0.05       0.00    -0.11
     5   0.0437      0.00     0.06       0.00    -0.05
     6   0.0437      0.00     0.08       0.00    -0.06
     7   0.0437      0.00     0.06       0.00    -0.01
     8   0.1065      0.00    -0.01       0.00    -0.01
     9   0.1065      0.00     0.31       0.00     0.31
    10   0.1065      0.00     0.04       0.00     0.02
    11   0.1065      0.00     0.06       0.00    -0.06
    12   0.1065      0.00     0.09       0.00    -0.01
    13   0.1065      0.00     0.24       0.00     0.16
    14   0.1065      0.00    -0.17       0.00    -0.11
    15   0.1065      0.00     0.16       0.00     0.11
    16   0.1065      0.00    -0.07       0.00    -0.05
    17   0.1532      0.00     0.02       0.00     0.04
    18   0.1723      0.00    -0.09       0.00    -0.00
    19   0.1723      0.00    -0.05       0.00    -0.29
    20   0.1723      0.00     0.01       0.00     0.00
    21   0.1723      0.00     0.01       0.00    -0.17
    22   0.1723      0.00    -0.10       0.00    -0.35
    23   0.1723      0.00    -0.02       0.00    -0.11
    24   0.1723      0.00    -0.09       0.00     0.01
    25   0.1723      0.00    -0.05       0.00     0.02
    26   0.1723      0.00    -0.05       0.00     0.02
    27   0.1778      0.00    -0.09       0.00     0.04
    28   0.1778      0.00    -0.05       0.00    -0.05
    29   0.1778      0.00    -0.01       0.00     0.02
    30   0.1778      0.00     0.01       0.00     0.07
    31   0.1778      0.00     0.05       0.00     0.08
    32   0.1778      0.00    -0.01       0.00     0.14
    33   0.1914      0.00    -0.09       0.00    -0.01
    34   0.3143      0.00     0.03       0.00    -0.14
    35   0.4753      0.00     0.12       0.00    -0.20
    36   1.3325      0.00     0.02       0.00     0.04
    37   1.3708      0.00     0.05       0.00     0.02
    38   1.3708      0.00     0.22       0.00     0.40
    39   1.3708      0.00     0.02       0.00     0.02
    40   1.3708      0.00    -0.05       0.00    -0.12
    41   1.3708      0.00     0.43       0.00     0.47
    42   1.3708      0.00     0.02       0.00    -0.11
    43   1.3708      0.00    -0.29       0.00    -0.06
    44   1.3708      0.00    -0.11       0.00     0.33
    45   1.3708      0.00    -0.16       0.00    -0.05
    46   3.3371      0.00    -0.10       0.00    -0.06
    47   3.3373      0.00    -0.15       0.00    -0.08
    48   8.3524      0.00     0.29       0.00     0.20
    49   8.3525      0.00     0.34       0.00     0.04
    50   8.3527      0.00    -0.56       0.00    -0.32

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.

14QG442    quality flag:3

Type:       SCATNEAR  SCATNEAR  SCATNEAR

axisobj        54.342    54.342    54.342
ecceobj         0.371     0.371     0.371
incobj         30.446    30.446    30.446
qmin           33.145    33.199    33.093
qmax           75.164    75.271    75.422
amean          53.656    53.704    53.699
amin           53.006    53.012    53.042
amax           54.443    54.490    54.484
emean           0.359     0.359     0.360
emin            0.335     0.335     0.336
emax            0.381     0.382     0.384
imean          28.974    29.028    28.952
imin           28.304    28.369    28.259
imax           29.968    29.924    29.929
excite_mean     0.603     0.604     0.604
fracstop        1.000     1.000     1.000
cjmean          2.741     2.740     2.741

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       182.9     182.0     181.9
kozaiamp        180.0     180.0     179.9