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 Jul 22 01:38:20 2018
# Orbit generated from Bernstein formalism
# Fitting   27 observations of   27
# Arc:   6.15y
# First observation: 2012/02/16
#  Last observation: 2018/04/10
Preliminary a, adot, b, bdot, g, gdot:
  -0.000698   0.027340  -0.000149   0.004467   0.023152   0.000000
# Chi-squared of fit:    21.54 DOF:   48 RMS:  0.16
# Min/Max residuals:    -0.51    0.34
# Exact a, adot, b, bdot, g, gdot:
  1.755682E-05  2.652229E-02  3.427029E-06  4.291454E-03  2.413673E-02 -7.954516E-03
# Covariance matrix:
  1.8257E-13 -9.1486E-14  5.1248E-15 -8.3043E-15 -3.5590E-14 -3.7406E-13
 -9.1486E-14  1.0226E-13 -8.4879E-15  1.3979E-14  7.0665E-14  6.2729E-13
  5.1248E-15 -8.4879E-15  1.5439E-13 -4.3311E-14  1.7829E-16 -7.1394E-14
 -8.3043E-15  1.3979E-14 -4.3311E-14  1.9714E-14  5.9456E-15  1.1005E-13
 -3.5590E-14  7.0665E-14  1.7829E-16  5.9456E-15  3.2346E-13  2.0226E-13
 -3.7406E-13  6.2729E-13 -7.1394E-14  1.1005E-13  2.0226E-13  5.0163E-12
#      lat0       lon0       xBary       yBary       zBary        JD0
    7.232434  164.198414    0.288684    0.119178   -0.939063  2455974.024756
# Heliocentric elements and errors
Epoch:              2455970.5000  =  2012/02/13
Mean Anomaly:          344.46736 +/-     0.005
Argument of Peri:       88.95544 +/-     0.011
Long of Asc Node:      126.59076 +/-     0.001
Inclination:            11.59222 +/-     0.000
Eccentricity:         0.51293951 +/-    0.0001
Semi-Major Axis:     75.98653529 +/-    0.0162
Time of Perihelion: 2466409.1965 +/-       1.4
Perihelion:          37.01003882 +/-    0.0113
Aphelion:           114.96303176 +/-    0.0259
Period (y)              662.3891 +/-      0.21
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -40.37716963 +/-    0.0009
Ecliptic Y           11.72845731 +/-    0.0003
Ecliptic Z            5.21604238 +/-    0.0001
Ecliptic XDOT         0.00009638 +/-    0.0000
Ecliptic YDOT        -0.00315095 +/-    0.0000
Ecliptic ZDOT         0.00036941 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   42.36838015 +/-    0.0009
Geocenter to KBO     41.43063669 +/-    0.0010
# Hcoef:  6.10

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      
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      
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      
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      

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    -0.04       0.00    -0.13
  2   0.0000     -0.03     0.04       0.02    -0.11
  3   0.0000     -0.80     0.17      -0.06    -0.26
  4   0.0000     -1.15    -0.08       0.17    -0.04
  5   0.0001     -1.87     0.11       0.17    -0.11
  6   0.0001     -2.04     0.05       0.26    -0.03
  7   0.0001     -2.95     0.04       0.40     0.05
  8   0.0001     -3.25    -0.16       0.31    -0.05
  9   2.7764  18528.30     0.13    1749.09     0.10
 10   2.7764  18528.50    -0.13    1749.16    -0.00
 11   2.7764  18529.29     0.20    1749.60     0.27
 12   3.0004  16848.42    -0.06    2724.16    -0.03
 13   3.0004  16847.42    -0.29    2724.12    -0.14
 14   3.0004  16846.90    -0.03    2724.27    -0.06
 15   3.0005  16846.18     0.03    2724.28    -0.12
 16   3.0991  14270.16    -0.16    2814.45    -0.02
 17   3.0992  14269.44    -0.07    2814.51     0.06
 18   3.0992  14268.97     0.27    2814.60     0.17
 19   3.0992  14267.77    -0.11    2814.35    -0.06
 20   3.1019  14199.56     0.04    2813.24     0.18
 21   3.1019  14198.81     0.10    2813.08     0.05
 22   3.1020  14197.77    -0.14    2813.35     0.34
 23   3.1619  12824.58     0.06    2736.23     0.20
 24   3.1620  12823.85    -0.03    2736.17     0.21
 25   3.1620  12823.20    -0.04    2736.08     0.19
 26   6.1455  30927.97    -0.18    5660.37    -0.51
 27   6.1457  30924.98     0.30    5660.44    -0.14

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        75.757    75.801    75.714
ecceobj         0.511     0.512     0.511
incobj         11.597    11.597    11.597
qmin           36.337    36.243    36.296
qmax          118.463   119.036   118.507
amean          75.528    76.051    76.042
amin           74.241    74.324    74.334
amax           77.893    78.029    77.851
emean           0.504     0.510     0.508
emin            0.490     0.495     0.491
emax            0.523     0.526     0.524
imean          10.941    10.470    11.033
imin            9.963     9.346    10.063
imax           11.753    11.595    12.159
excite_mean     0.538     0.542     0.543
fracstop        1.000     1.000     1.000
cjmean          3.085     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       184.1     183.6     180.4
kozaiamp        180.0     180.0     180.0