Orbit Fit and Astrometric record for 14QV510

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: 14QV510   
# Created Sun Dec 22 02:10:00 2024
# Orbit generated from Bernstein formalism
# Fitting     19 observations of     19
# Arc:   4.22y
# First observation: 2014/08/18
#  Last observation: 2018/11/06
Preliminary a, adot, b, bdot, g, gdot:
   0.000294   0.028329  -0.000035   0.001425   0.027339   0.000000
# Chi-squared of fit:     7.05 DOF:     32 RMS:  0.11
# Min/Max residuals:    -0.25    0.22
# Exact a, adot, b, bdot, g, gdot:
  1.702415E-05  2.819986E-02  1.463077E-06  1.468305E-03  2.658408E-02 -2.996817E-03
# Covariance matrix:
  2.4249E-13 -9.2514E-14 -6.8000E-15 -1.5082E-14  2.0071E-13 -5.9191E-13
 -9.2514E-14  5.6666E-13 -3.6147E-14  5.5888E-14  2.9976E-13  6.1045E-12
 -6.8000E-15 -3.6147E-14  1.6458E-13 -5.8070E-14 -4.6627E-14 -3.9681E-13
 -1.5082E-14  5.5888E-14 -5.8070E-14  4.4290E-14  2.0007E-16  6.6748E-13
  2.0071E-13  2.9976E-13 -4.6627E-14  2.0007E-16  7.9203E-13  2.9863E-12
 -5.9191E-13  6.1045E-12 -3.9681E-13  6.6748E-13  2.9863E-12  7.0682E-11
#      lat0       lon0       xBary       yBary       zBary        JD0
  -32.171655  -36.293775   -0.023306   -0.540206   -0.858997  2456887.735028
# Heliocentric elements and errors
Epoch:              2456880.5000  =  2014/08/11
Mean Anomaly:          321.80304 +/-     0.057
Argument of Peri:      325.52455 +/-     0.088
Long of Asc Node:       47.84428 +/-     0.001
Inclination:            31.50469 +/-     0.000
Eccentricity:         0.14966275 +/-    0.0003
Semi-Major Axis:     43.10642710 +/-    0.0069
Time of Perihelion: 2467848.7599 +/-      16.1
Perihelion:          36.65500089 +/-    0.0125
Aphelion:            49.55785331 +/-    0.0136
Period (y)              283.0227 +/-      0.07
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           26.49323421 +/-    0.0009
Ecliptic Y          -19.42721135 +/-    0.0006
Ecliptic Z          -20.02914172 +/-    0.0007
Ecliptic XDOT         0.00156854 +/-    0.0000
Ecliptic YDOT         0.00244351 +/-    0.0000
Ecliptic ZDOT         0.00029246 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   38.47693488 +/-    0.0008
Geocenter to KBO     37.61650293 +/-    0.0013
# Hcoef:  7.82

The following table shows the complete astrometric record for 14QV510. 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 (14QV510) followed by the observatory code and reference code for the source of the astrometry.

2014 08  18.23425  22 40 07.46   -43 27 28.7   23.6i 14QV510   W84  C~3cnQ      
2014 08  18.23561  22 40 07.449  -43 27 28.70  24.6g 14QV510   W84  C~4yU1      
2014 08  21.23138  22 39 47.928  -43 29 00.43  24.7g 14QV510   W84  C~4yU1      
2014 09  20.15369  22 36 31.290  -43 36 44.72  23.5r 14QV510   W84  C~4yU1      
2014 09  20.15806  22 36 31.274  -43 36 44.74  24.5g 14QV510   W84  C~4yU1      
2014 09  24.13285  22 36 06.970  -43 36 38.67  23.5r 14QV510   W84  C~4yU1      
2014 09  26.12280  22 35 55.111  -43 36 29.39  23.6i 14QV510   W84  C~4yU1      
2014 09  27.12311  22 35 49.259  -43 36 23.01  23.1i 14QV510   W84  C~4yU1      
2015 09  13.15059  22 45 00.672  -42 48 42.17  23.4i 14QV510   W84  C~4yU1      
2015 09  13.15197  22 45 00.645  -42 48 42.04  23.3r 14QV510   W84  C~4yU1      
2015 09  13.15335  22 45 00.622  -42 48 42.06  24.0g 14QV510   W84  C~4yU1      
2016 10  02.10427  22 50 33.977  -41 59 37.07  23.4r 14QV510   W84  C~4yU1      
2017 08  17.23369  23 02 47.917  -40 55 22.27  23.3r 14QV510   W84  C~4yU1      
2017 08  17.23506  23 02 47.884  -40 55 22.13  22.9i 14QV510   W84  C~4yU1      
2017 08  17.23643  23 02 47.893  -40 55 22.34  24.2g 14QV510   W84  C~4yU1      
2017 09  19.14372  22 59 18.243  -41 08 11.29  23.9r 14QV510   W84  C~4yU1      
2017 10  21.08104  22 56 25.036  -41 03 20.84  24.1i 14QV510   W84  C~4yU1      
2017 10  27.06098  22 56 01.783  -41 00 28.49  22.8z 14QV510   W84  C~4yU1      
2018 11  06.14056  23 02 43.438  -40 02 17.36  23.8r 14QV510   W84  C~4yU1      

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    -0.12
     2   0.0000     -0.11    -0.05       0.05    -0.07
     3   0.0082   -231.28    -0.10      11.50     0.08
     4   0.0901  -2357.54    -0.03     526.68     0.08
     5   0.0901  -2357.70     0.08     526.74     0.00
     6   0.1010  -2593.25     0.17     646.09    -0.07
     7   0.1065  -2705.52    -0.04     709.94    -0.02
     8   0.1092  -2760.17     0.08     743.04     0.04
     9   1.0703   3912.31     0.06     641.19    -0.16
    10   1.0703   3912.10    -0.05     641.45     0.05
    11   1.0703   3911.87    -0.19     641.54     0.12
    12   2.1242   8551.59     0.08    1548.37     0.09
    13   2.9979  17674.00     0.12     919.12    -0.13
    14   2.9979  17673.74    -0.03     919.43     0.17
    15   2.9980  17673.72     0.06     919.19    -0.06
    16   3.0880  15216.89     0.13    1429.01     0.22
    17   3.1755  13642.02     0.07    2640.17    -0.13
    18   3.1919  13494.53    -0.25    2918.84     0.05
    19   4.2188  19236.05    -0.07    3715.23    -0.13

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.

14QV510    quality flag:3

Type:       SCATEXTD  SCATEXTD  SCATEXTD

axisobj        43.357    43.376    43.339
ecceobj         0.155     0.155     0.154
incobj         31.529    31.529    31.529
qmin           35.729    35.636    35.674
qmax           51.298    51.402    51.321
amean          43.321    43.366    43.317
amin           42.969    43.007    42.953
amax           43.713    43.781    43.717
emean           0.156     0.157     0.156
emin            0.139     0.140     0.140
emax            0.174     0.175     0.174
imean          30.524    30.518    30.523
imin           30.141    30.108    30.133
imax           30.920    30.916    30.918
excite_mean     0.531     0.532     0.531
fracstop        1.000     1.000     1.000
cjmean          2.737     2.737     2.737

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       168.4     168.1     168.5
kozaiamp        180.0     180.0     180.0