Orbit Fit and Astrometric record for 14WN510

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: 14WN510   
# Created Sun Feb 23 02:10:12 2025
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     78 observations of     78
# Arc:  12.90y
# First observation: 2012/02/16
#  Last observation: 2025/01/08
# Chi-squared of fit:    81.67 DOF:    150 RMS:  0.18
# Min/Max residuals:    -0.56    0.49
# Exact a, adot, b, bdot, g, gdot:
  1.676986E-05  2.652229E-02  3.063046E-06  4.291430E-03  2.413626E-02 -7.956474E-03
# Covariance matrix:
  9.2041E-14 -2.9613E-14  7.4176E-15 -3.7200E-15 -5.9803E-15 -6.0765E-14
 -2.9613E-14  1.3896E-14 -3.7746E-15  1.9944E-15  1.0512E-14  3.2431E-14
  7.4176E-15 -3.7746E-15  4.6943E-14 -7.1543E-15 -1.6253E-15 -9.9272E-15
 -3.7200E-15  1.9944E-15 -7.1543E-15  1.8367E-15  1.6761E-15  5.2247E-15
 -5.9803E-15  1.0512E-14 -1.6253E-15  1.6761E-15  6.4730E-14  2.6133E-14
 -6.0765E-14  3.2431E-14 -9.9272E-15  5.2247E-15  2.6133E-14  8.4988E-14
#      lat0       lon0       xBary       yBary       zBary        JD0
    7.232434  164.198414    0.288683    0.119178   -0.939063  2455974.024756
# Heliocentric elements and errors
Epoch:              2455974.5000  =  2012/02/17
Mean Anomaly:          344.47966 +/-     0.002
Argument of Peri:       88.95758 +/-     0.003
Long of Asc Node:      126.59063 +/-     0.000
Inclination:            11.59217 +/-     0.000
Eccentricity:         0.51307886 +/-    0.0000
Semi-Major Axis:     76.00691355 +/-    0.0068
Time of Perihelion: 2466409.1230 +/-      31.3
Perihelion:          37.00937292 +/-    0.0043
Aphelion:           115.00445417 +/-    0.0107
Period (y)              662.6556 +/-      0.09
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -40.37792397 +/-    0.0004
Ecliptic Y           11.72870466 +/-    0.0001
Ecliptic Z            5.21612784 +/-    0.0001
Ecliptic XDOT         0.00009660 +/-    0.0000
Ecliptic YDOT        -0.00315107 +/-    0.0000
Ecliptic ZDOT         0.00036939 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   42.36939720 +/-    0.0004
Geocenter to KBO     41.43168588 +/-    0.0004
# Hcoef:  6.23

The following table shows the complete astrometric record for 14WN510. 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 (14WN510) followed by the observatory code and reference code for the source of the astrometry.

2012 02  16.52399  11 13 10.729  +12 52 59.01  22.3w 14WN510   F51  C~2dYx      
2012 02  16.52547  11 13 10.728  +12 52 59.04  22.5w 14WN510   F51  C~2dYx      
2012 02  16.53866  11 13 10.677  +12 52 59.27  22.6w 14WN510   F51  C~2dYx      
2012 02  16.54011  11 13 10.661  +12 52 59.62  22.4w 14WN510   F51  C~2dYx      
2012 02  16.55338  11 13 10.616  +12 52 59.90  22.6w 14WN510   F51  C~2dYx      
2012 02  16.55484  11 13 10.608  +12 53 00.05  22.5w 14WN510   F51  C~2dYx      
2012 02  16.56809  11 13 10.554  +12 53 00.54  22.5w 14WN510   F51  C~2dYx      
2012 02  16.56954  11 13 10.533  +12 53 00.57  22.6w 14WN510   F51  C~2dYx      
2012 03  13.38998  11 11 18.192  +13 06 13.60  22.4G 14WN510   F51  C~2r7Z      
2012 03  28.32875  11 10 14.373  +13 12 41.87  21.7G 14WN510   F51  C~2r7Z      
2013 02  14.39999  11 19 26.347  +12 29 33.67  23.0G 14WN510   F51  C~2r7Z      
2013 02  14.41455  11 19 26.284  +12 29 34.56  22.5G 14WN510   F51  C~2r7Z      
2013 02  14.42917  11 19 26.220  +12 29 34.84  23.3G 14WN510   F51  C~2r7Z      
2013 02  14.44392  11 19 26.156  +12 29 35.30  22.3G 14WN510   F51  C~2r7Z      
2013 03  03.48800  11 18 13.658  +12 38 39.86  21.9G 14WN510   F51  C~2r7Z      
2013 06  04.28507  11 14 02.625  +12 57 37.66  22.1G 14WN510   F51  C~2r7Z      
2014 03  20.48721  11 23 14.906  +12 23 31.93  22.5G 14WN510   F51  C~2r7Z      
2014 11  22.64259  11 33 01.098  +11 16 18.07  22.2G 14WN510   F51  C~2r7Z      
2014 11  26.59493  11 33 12.420  +11 16 02.94  22.3w 14WN510   F51  C~1vXv      
2014 11  26.60748  11 33 12.434  +11 16 02.92  22.4w 14WN510   F51  C~1vXv      
2014 11  26.61998  11 33 12.495  +11 16 03.00  22.4w 14WN510   F51  C~1vXv      
2014 11  30.58898  11 33 22.412  +11 15 57.68  22.6G 14WN510   F51  C~2r7Z      
2014 11  30.60090  11 33 22.443  +11 15 57.69  22.5G 14WN510   F51  C~2r7Z      
2014 11  30.61283  11 33 22.475  +11 15 57.40  22.7G 14WN510   F51  C~2r7Z      
2014 11  30.62476  11 33 22.491  +11 15 58.02  22.8G 14WN510   F51  C~2r7Z      
2014 12  09.61452  11 33 39.796  +11 16 22.38  23.1G 14WN510   F51  C~2r7Z      
2015 01  27.62275  11 33 03.616  +11 31 47.68  23.4G 14WN510   F51  C~2r7Z      
2015 01  29.63642  11 32 57.834  +11 32 47.93  22.4G 14WN510   F51  C~2r7Z      
2015 02  16.40726  11 31 55.924  +11 42 12.25  22.2w 14WN510   F51  C~1vXv      
2015 02  16.41869  11 31 55.861  +11 42 12.62  22.0w 14WN510   F51  C~1vXv      
2015 02  16.43013  11 31 55.833  +11 42 12.97  22.2w 14WN510   F51  C~1vXv      
2015 02  16.44158  11 31 55.789  +11 42 13.27  22.3w 14WN510   F51  C~1vXv      
2015 03  24.47994  11 29 18.997  +12 01 00.45  22.2w 14WN510   F51  C~1vXv      
2015 03  24.49143  11 29 18.954  +12 01 00.80  22.4w 14WN510   F51  C~1vXv      
2015 03  24.50291  11 29 18.927  +12 01 01.07  22.1w 14WN510   F51  C~1vXv      
2015 03  24.51436  11 29 18.846  +12 01 01.33  22.2w 14WN510   F51  C~1vXv      
2015 03  25.49401  11 29 14.589  +12 01 27.94  22.5w 14WN510   F51  C~1vXv      
2015 03  25.50550  11 29 14.538  +12 01 28.10  22.3w 14WN510   F51  C~1vXv      
2015 03  25.51696  11 29 14.481  +12 01 28.77  22.3w 14WN510   F51  C~1vXv      
2015 04  16.41497  11 27 47.180  +12 09 33.93  22.5w 14WN510   F51  C~1vXv      
2015 04  16.42663  11 27 47.133  +12 09 34.17  22.3w 14WN510   F51  C~1vXv      
2015 04  16.43826  11 27 47.090  +12 09 34.35  22.1w 14WN510   F51  C~1vXv      
2015 04  18.43817  11 27 40.181  +12 10 06.77  22.5G 14WN510   F51  C~2r7Z      
2016 01  13.51037  11 39 57.603  +10 59 51.46  22.5G 14WN510   F51  C~2r7Z      
2016 03  01.40367  11 37 24.090  +11 24 21.64  22.2G 14WN510   F51  C~2r7Z      
2016 03  11.38042  11 36 39.765  +11 29 43.75  22.5G 14WN510   F51  C~2r7Z      
2016 03  29.30827  11 35 20.166  +11 38 21.44  23.6G 14WN510   F51  C~2r7Z      
2016 03  29.32075  11 35 20.102  +11 38 21.64  22.2G 14WN510   F51  C~2r7Z      
2016 03  29.33329  11 35 20.051  +11 38 21.73  22.0G 14WN510   F51  C~2r7Z      
2016 03  29.34590  11 35 19.971  +11 38 22.12  22.3G 14WN510   F51  C~2r7Z      
2016 04  05.30936  11 34 50.777  +11 41 11.88  21.8G 14WN510   F51  C~2r7Z      
2016 04  22.38249  11 33 47.914  +11 46 28.93  22.4G 14WN510   F51  C~2r7Z      
2016 05  20.34671  11 32 45.549  +11 49 10.02  23.2G 14WN510   F51  C~2r7Z      
2017 01  30.47965  11 45 45.897  +10 41 35.50  22.1G 14WN510   F51  C~2r7Z      
2017 01  30.49153  11 45 45.860  +10 41 35.66  22.2G 14WN510   F51  C~2r7Z      
2017 01  30.50344  11 45 45.803  +10 41 36.55  21.5G 14WN510   F51  C~2r7Z      
2017 01  30.51542  11 45 45.795  +10 41 36.78  21.7G 14WN510   F51  C~2r7Z      
2017 02  16.56904  11 44 48.337  +10 50 45.09  22.0G 14WN510   F51  C~2r7Z      
2017 03  20.29755  11 42 31.286  +11 07 59.95  22.1G 14WN510   F51  C~2r7Z      
2017 03  20.30921  11 42 31.232  +11 08 00.32  22.2G 14WN510   F51  C~2r7Z      
2017 03  20.32086  11 42 31.177  +11 08 00.68  22.4G 14WN510   F51  C~2r7Z      
2017 03  20.33250  11 42 31.132  +11 08 01.13  22.4G 14WN510   F51  C~2r7Z      
2017 04  20.27979  11 40 23.787  +11 20 11.20  22.8G 14WN510   F51  C~2r7Z      
2017 04  20.29190  11 40 23.747  +11 20 11.62  22.6G 14WN510   F51  C~2r7Z      
2017 04  20.30409  11 40 23.689  +11 20 11.57  22.4G 14WN510   F51  C~2r7Z      
2017 05  09.35373  11 39 29.133  +11 23 33.81  23.2G 14WN510   F51  C~2r7Z      
2018 04  10.17446  11 47 36.288  +10 50 10.64  22.5R 14WN510   G37  C~2dYx      
2018 04  10.22689  11 47 36.110  +10 50 11.94        14WN510   G37  C~2dYx      
2021 02  07.48805  12 11 58.899  +08 51 47.04  22.1w 14WN510   F51  C~4ZEi      
2021 02  07.49852  12 11 58.857  +08 51 47.51  22.1w 14WN510   F51  C~4ZEi      
2021 02  07.50901  12 11 58.843  +08 51 47.52  22.4w 14WN510   F51  C~4ZEi      
2021 02  07.51951  12 11 58.791  +08 51 48.30  22.3w 14WN510   F51  C~4ZEi      
2024 04  09.311389 12 28 29.770  +07 51 15.79  21.8w 14WN510   F52  C~7xPi      
2024 04  09.322554 12 28 29.728  +07 51 15.88  21.7w 14WN510   F52  C~7xPi      
2024 04  09.333686 12 28 29.688  +07 51 16.29  21.9w 14WN510   F52  C~7xPi      
2025 01  08.633744 12 40 07.975  +06 32 33.66  22.1w 14WN510   F51  C~8cQ3      
2025 01  08.642432 12 40 08.003  +06 32 33.79  22.2w 14WN510   F51  C~8cQ3      
2025 01  08.659735 12 40 07.991  +06 32 34.11  22.0w 14WN510   F51  C~8cQ3      

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    -0.10
     2   0.0000      0.00     0.17       0.00    -0.11
     3   0.0000      0.00     0.24       0.00    -0.30
     4   0.0000      0.00     0.09       0.00     0.00
     5   0.0001      0.00     0.24       0.00    -0.14
     6   0.0001      0.00     0.22       0.00    -0.04
     7   0.0001      0.00     0.24       0.00     0.03
     8   0.0001      0.00     0.01       0.00     0.02
     9   0.0708      0.00    -0.32       0.00     0.09
    10   0.1117      0.00    -0.45       0.00     0.25
    11   0.9962      0.00    -0.14       0.00    -0.33
    12   0.9963      0.00    -0.20       0.00     0.09
    13   0.9963      0.00    -0.27       0.00    -0.11
    14   0.9964      0.00    -0.32       0.00    -0.12
    15   1.0430      0.00    -0.42       0.00    -0.02
    16   1.2971      0.00    -0.00       0.00    -0.18
    17   2.0889      0.00     0.06       0.00    -0.16
    18   2.7656      0.00    -0.18       0.00     0.25
    19   2.7764      0.00     0.33       0.00     0.04
    20   2.7764      0.00     0.04       0.00     0.05
    21   2.7764      0.00     0.47       0.00     0.16
    22   2.7873      0.00    -0.14       0.00    -0.05
    23   2.7873      0.00    -0.08       0.00    -0.04
    24   2.7874      0.00    -0.01       0.00    -0.33
    25   2.7874      0.00    -0.18       0.00     0.29
    26   2.8120      0.00    -0.06       0.00    -0.16
    27   2.9462      0.00    -0.15       0.00    -0.19
    28   2.9517      0.00     0.12       0.00     0.13
    29   3.0004      0.00     0.06       0.00     0.02
    30   3.0004      0.00    -0.20       0.00     0.02
    31   3.0004      0.00     0.07       0.00    -0.01
    32   3.0005      0.00     0.10       0.00    -0.09
    33   3.0991      0.00    -0.07       0.00     0.09
    34   3.0992      0.00     0.05       0.00     0.13
    35   3.0992      0.00     0.41       0.00     0.09
    36   3.0992      0.00    -0.04       0.00     0.04
    37   3.1019      0.00     0.19       0.00     0.20
    38   3.1019      0.00     0.19       0.00     0.05
    39   3.1020      0.00     0.10       0.00     0.42
    40   3.1619      0.00     0.19       0.00     0.21
    41   3.1620      0.00     0.11       0.00     0.26
    42   3.1620      0.00     0.09       0.00     0.24
    43   3.1675      0.00    -0.12       0.00    -0.10
    44   3.9069      0.00    -0.20       0.00     0.01
    45   4.0380      0.00     0.04       0.00    -0.04
    46   4.0653      0.00    -0.22       0.00     0.05
    47   4.1144      0.00     0.26       0.00     0.22
    48   4.1144      0.00     0.12       0.00     0.09
    49   4.1145      0.00     0.18       0.00    -0.14
    50   4.1145      0.00    -0.20       0.00    -0.08
    51   4.1336      0.00    -0.06       0.00     0.13
    52   4.1803      0.00     0.09       0.00     0.11
    53   4.2569      0.00    -0.01       0.00    -0.18
    54   4.9554      0.00     0.07       0.00     0.16
    55   4.9554      0.00     0.03       0.00    -0.04
    56   4.9555      0.00    -0.31       0.00     0.49
    57   4.9555      0.00     0.09       0.00     0.35
    58   5.0022      0.00    -0.26       0.00    -0.25
    59   5.0890      0.00    -0.02       0.00    -0.08
    60   5.0891      0.00    -0.03       0.00    -0.06
    61   5.0891      0.00    -0.05       0.00    -0.05
    62   5.0891      0.00     0.07       0.00     0.05
    63   5.1739      0.00     0.02       0.00    -0.18
    64   5.1739      0.00     0.07       0.00     0.04
    65   5.1739      0.00    -0.15       0.00    -0.21
    66   5.2261      0.00    -0.07       0.00    -0.16
    67   6.1455      0.00    -0.56       0.00    -0.25
    68   6.1457      0.00     0.03       0.00    -0.13
    69   8.9773      0.00     0.15       0.00    -0.17
    70   8.9773      0.00    -0.01       0.00    -0.03
    71   8.9774      0.00     0.25       0.00    -0.36
    72   8.9774      0.00    -0.06       0.00     0.08
    73  12.1445      0.00    -0.12       0.00     0.19
    74  12.1446      0.00     0.02       0.00    -0.02
    75  12.1446      0.00     0.19       0.00     0.09
    76  12.8956      0.00    -0.20       0.00    -0.03
    77  12.8956      0.00     0.18       0.00    -0.04
    78  12.8956      0.00    -0.09       0.00    -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.

14WN510    quality flag:3

Type:       SCATNEAR  SCATNEAR  SCATNEAR

axisobj        75.773    75.772    75.774
ecceobj         0.511     0.511     0.511
incobj         11.597    11.597    11.597
qmin           36.266    36.271    36.266
qmax          118.785   118.759   118.808
amean          76.063    76.292    76.348
amin           74.292    74.401    74.311
amax           77.937    77.955    77.927
emean           0.508     0.510     0.510
emin            0.489     0.489     0.496
emax            0.525     0.525     0.525
imean          10.931    10.894    10.848
imin           10.015     9.994     9.996
imax           11.890    11.862    11.705
excite_mean     0.542     0.544     0.544
fracstop        1.000     1.000     1.000
cjmean          3.084     3.084     3.084

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       172.7     175.8     175.4
kozaiamp        179.9     180.0     180.0