Orbit Fit and Astrometric record for 14QV495

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: 14QV495   
# Created Wed Dec 25 02:09:54 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     23 observations of     23
# Arc:   5.42y
# First observation: 2014/08/19
#  Last observation: 2020/01/18
# Chi-squared of fit:    68.71 DOF:     40 RMS:  0.31
# Min/Max residuals:    -0.84    1.59
# Exact a, adot, b, bdot, g, gdot:
  1.952521E-05  3.358786E-02  5.147991E-06  7.533779E-03  2.733539E-02  5.461743E-03
# Covariance matrix:
  2.3152E-13 -1.1026E-13  1.5164E-14 -3.1505E-14  1.2396E-13 -7.8419E-13
 -1.1026E-13  3.3574E-13 -3.6500E-14  9.1371E-14  7.7112E-14  2.4543E-12
  1.5164E-14 -3.6500E-14  1.0919E-13 -4.5238E-14 -1.2421E-15 -3.0321E-13
 -3.1505E-14  9.1371E-14 -4.5238E-14  5.8880E-14  1.1684E-14  7.4890E-13
  1.2396E-13  7.7112E-14 -1.2421E-15  1.1684E-14  2.0982E-13  3.9623E-13
 -7.8419E-13  2.4543E-12 -3.0321E-13  7.4890E-13  3.9623E-13  2.0019E-11
#      lat0       lon0       xBary       yBary       zBary        JD0
  -20.531123   12.368833    0.733547   -0.245810   -0.656727  2456888.834488
# Heliocentric elements and errors
Epoch:              2456888.5000  =  2014/08/19
Mean Anomaly:            5.73869 +/-     0.005
Argument of Peri:      277.13660 +/-     0.018
Long of Asc Node:       69.24025 +/-     0.001
Inclination:            23.38103 +/-     0.000
Eccentricity:         0.54275107 +/-    0.0001
Semi-Major Axis:     79.24863240 +/-    0.0208
Time of Perihelion: 2452780.8218 +/-       3.6
Perihelion:          36.23635245 +/-    0.0142
Aphelion:           122.26091234 +/-    0.0337
Period (y)              705.4981 +/-      0.28
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           34.30350374 +/-    0.0006
Ecliptic Y            6.77430081 +/-    0.0001
Ecliptic Z          -12.82993947 +/-    0.0002
Ecliptic XDOT         0.00003341 +/-    0.0000
Ecliptic YDOT         0.00344813 +/-    0.0000
Ecliptic ZDOT         0.00051490 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   37.24542028 +/-    0.0005
Geocenter to KBO     36.58252587 +/-    0.0006
# Hcoef:  6.86

The following table shows the complete astrometric record for 14QV495. 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 (14QV495) followed by the observatory code and reference code for the source of the astrometry.

2014 08  19.33371  01 17 54.975  -14 00 12.86  23.1g 14QV495   W84  C~4yTz      
2014 08  19.33507  01 17 54.977  -14 00 12.85  22.0z 14QV495   W84  C~4yTz      
2014 08  19.33618  01 17 54.971  -14 00 12.78  22.3Y 14QV495   W84  C~4yTz      
2014 09  16.25983  01 16 15.901  -14 17 33.06  21.7z 14QV495   W84  C~4yTz      
2014 09  25.23259  01 15 34.207  -14 22 35.29  23.2g 14QV495   W84  C~4yTz      
2014 09  25.233437 01 15 34.20   -14 22 35.1   23.1r 14QV495   W84  C~35bt      
2014 09  25.23533  01 15 34.192  -14 22 35.38  22.4i 14QV495   W84  C~4yTz      
2014 11  21.18686  01 11 02.047  -14 35 42.70  22.4i 14QV495   W84  C~4yTz      
2014 11  21.19377  01 11 02.018  -14 35 42.58  22.6r 14QV495   W84  C~4yTz      
2014 12  22.08427  01 09 48.246  -14 24 26.39  22.4i 14QV495   W84  C~4yTz      
2014 12  30.065336 01 09 44.27   -14 19 29.0   22.2z 14QV495   W84  C~35bt      
2014 12  30.06586  01 09 44.259  -14 19 29.21  22.2z 14QV495   W84  C~4yTz      
2015 09  13.27672  01 23 02.482  -13 05 29.30  22.5i 14QV495   W84  C~4yTz      
2015 09  13.27810  01 23 02.472  -13 05 29.38  22.3r 14QV495   W84  C~4yTz      
2015 09  13.27948  01 23 02.478  -13 05 29.38  23.3g 14QV495   W84  C~4yTz      
2015 09  23.26337  01 22 18.351  -13 11 12.34  22.8z 14QV495   W84  C~4yTz      
2015 10  07.188530 01 21 10.35   -13 18 09.6   22.6r 14QV495   W84  C~35bt      
2015 11  20.10905  01 17 40.484  -13 26 40.14  22.1z 14QV495   W84  C~4yTz      
2016 11  07.11352  01 24 59.170  -12 17 16.92  21.9z 14QV495   W84  C~4yTz      
2018 10  01.26729  01 40 34.244  -09 46 15.67  22.6z 14QV495   W84  C~4yTz      
2018 11  16.08750  01 36 51.733  -09 59 37.30  22.8i 14QV495   W84  C~4yTz      
2020 01  18.096920 01 40 50.016  -08 30 03.00  22.8G 14QV495   G37  C~3jSo      
2020 01  18.177520 01 40 50.249  -08 29 59.81        14QV495   G37  C~3jSo      

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     0.05       0.00    -0.16
     2   0.0000      0.00     0.13       0.00    -0.10
     3   0.0000      0.00     0.08       0.00     0.02
     4   0.0765      0.00    -0.10       0.00    -0.08
     5   0.1010      0.00     0.06       0.00    -0.06
     6   0.1010      0.00     0.01       0.00     0.16
     7   0.1010      0.00     0.03       0.00    -0.06
     8   0.2570      0.00    -0.01       0.00    -0.09
     9   0.2570      0.00    -0.06       0.00    -0.03
    10   0.3415      0.00    -0.02       0.00    -0.12
    11   0.3634      0.00     0.04       0.00     0.14
    12   0.3634      0.00    -0.13       0.00    -0.09
    13   1.0676      0.00     0.17       0.00     0.09
    14   1.0676      0.00     0.11       0.00     0.05
    15   1.0676      0.00     0.29       0.00     0.10
    16   1.0949      0.00     0.04       0.00     0.18
    17   1.1331      0.00    -0.32       0.00     0.11
    18   1.2533      0.00     0.02       0.00     0.05
    19   2.2198      0.00    -0.12       0.00     0.15
    20   4.1175      0.00    -0.40       0.00    -0.13
    21   4.2430      0.00    -0.49       0.00    -0.08
    22   5.4148      0.00    -0.84       0.00     0.06
    23   5.4150      0.00     1.59       0.00    -0.07

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.

14QV495    quality flag:3

Type:       SCATNEAR  SCATNEAR  SCATNEAR

axisobj        80.808    80.808    80.808
ecceobj         0.552     0.552     0.552
incobj         23.385    23.385    23.385
qmin           35.525    35.513    35.480
qmax          126.325   126.357   126.325
amean          79.576    79.629    79.478
amin           78.160    78.483    78.262
amax           81.280    81.293    81.280
emean           0.536     0.537     0.536
emin            0.519     0.522     0.520
emax            0.554     0.554     0.554
imean          23.008    22.958    22.958
imin           22.071    22.034    21.982
imax           23.941    23.862    23.875
excite_mean     0.663     0.663     0.663
fracstop        1.000     1.000     1.000
cjmean          2.905     2.905     2.905

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       167.6     168.2     169.6
kozaiamp        180.0     180.0     180.0