Orbit Fit and Astrometric record for 15VG171

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: 15VG171   
# Created Fri Apr 26 01:17:43 2024
# Orbit generated from Bernstein formalism
# Fitting     27 observations of     27
# Arc:   2.27y
# First observation: 2015/09/07
#  Last observation: 2017/12/13
Preliminary a, adot, b, bdot, g, gdot:
  -0.000124   0.022024  -0.000002   0.002339   0.023313   0.000000
# Chi-squared of fit:    10.26 DOF:     48 RMS:  0.11
# Min/Max residuals:    -0.25    0.30
# Exact a, adot, b, bdot, g, gdot:
  1.485850E-05  2.186089E-02  1.193773E-06  2.322070E-03  2.325854E-02  4.969726E-04
# Covariance matrix:
  2.7435E-13  4.6565E-14 -3.0749E-15  1.9043E-14  2.3628E-13  4.0684E-12
  4.6565E-14  3.3920E-13 -8.5634E-15  4.3272E-14  2.6406E-13  9.1617E-12
 -3.0749E-15 -8.5634E-15  1.1452E-13 -7.8467E-14 -7.9984E-15 -3.3276E-13
  1.9043E-14  4.3272E-14 -7.8467E-14  1.0533E-13  4.4077E-14  1.6595E-12
  2.3628E-13  2.6406E-13 -7.9984E-15  4.4077E-14  3.9438E-13  9.3704E-12
  4.0684E-12  9.1617E-12 -3.3276E-13  1.6595E-12  9.3704E-12  3.5111E-10
#      lat0       lon0       xBary       yBary       zBary        JD0
   -0.912725   51.896813    0.932968   -0.006057   -0.389557  2457273.133899
# Heliocentric elements and errors
Epoch:              2457270.5000  =  2015/09/05
Mean Anomaly:          183.19608 +/-     2.446
Argument of Peri:      168.39549 +/-     2.446
Long of Asc Node:       59.14210 +/-     0.001
Inclination:             6.11427 +/-     0.001
Eccentricity:         0.01952051 +/-    0.0001
Semi-Major Axis:     42.56219745 +/-    0.0028
Time of Perihelion: 2507081.3404 +/-     689.0
Perihelion:          41.73136163 +/-    0.0044
Aphelion:            43.39303328 +/-    0.0044
Period (y)              277.6798 +/-      0.03
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           27.49844563 +/-    0.0007
Ecliptic Y           33.55910170 +/-    0.0009
Ecliptic Z           -0.68482447 +/-    0.0000
Ecliptic XDOT        -0.00198804 +/-    0.0000
Ecliptic YDOT         0.00163098 +/-    0.0000
Ecliptic ZDOT         0.00027243 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   43.39178267 +/-    0.0008
Geocenter to KBO     42.99496672 +/-    0.0012
# Hcoef:  8.89

The following table shows the complete astrometric record for 15VG171. 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 (15VG171) followed by the observatory code and reference code for the source of the astrometry.

2015 09  07.63311  03 18 54.234  +17 21 32.10  25.4w 15VG171   568  C~2nw8      
2015 09  12.49674  03 18 46.575  +17 21 03.54  25.8w 15VG171   568  C~2nw8      
2015 10  07.60373  03 17 36.748  +17 16 45.04  25.8w 15VG171   568  C~2nw8      
2015 10  09.58362  03 17 29.378  +17 16 17.91  25.7w 15VG171   568  C~2nw8      
2015 11  07.33788  03 15 22.202  +17 08 32.16  24.8r 15VG171   568  C~2nw9      
2015 11  07.38006  03 15 21.996  +17 08 31.39  25.1r 15VG171   568  C~2nw9      
2015 11  07.42224  03 15 21.785  +17 08 30.88  25.4r 15VG171   568  C~2nw9      
2015 11  10.50536  03 15 06.802  +17 07 36.29  25.9w 15VG171   568  C~2nw9      
2015 11  17.35218  03 14 33.470  +17 05 35.87  25.7w 15VG171   568  C~2nw9      
2015 11  17.39878  03 14 33.244  +17 05 35.11  25.3w 15VG171   568  C~2nw9      
2015 12  06.36096  03 13 04.294  +17 00 18.25  25.3w 15VG171   568  C~2nw9      
2015 12  06.49848  03 13 03.663  +17 00 16.05  25.7w 15VG171   568  C~2nw9      
2016 01  01.34872  03 11 27.889  +16 54 53.39  25.7w 15VG171   568  C~2nw9      
2016 01  08.25624  03 11 10.131  +16 53 59.43  25.7w 15VG171   568  C~2nw9      
2016 02  10.30807  03 10 44.531  +16 53 42.66  25.2w 15VG171   568  C~2nw9      
2016 09  07.62568  03 23 49.213  +17 48 15.02  25.8w 15VG171   568  C~2nw9      
2016 11  02.52573  03 20 40.980  +17 37 09.68        15VG171   568  C~2nw9      
2016 11  04.40084  03 20 32.012  +17 36 38.08        15VG171   568  C~2nw9      
2016 12  24.31334  03 16 47.196  +17 23 45.12        15VG171   568  C~2nw9      
2016 12  25.28177  03 16 43.854  +17 23 33.99  24.1w 15VG171   568  C~2nw9      
2016 12  28.42845  03 16 33.449  +17 23 00.75  24.9w 15VG171   568  C~2nw9      
2017 01  02.41556  03 16 18.493  +17 22 14.13  25.6w 15VG171   568  C~2nw9      
2017 01  26.32908  03 15 35.838  +17 20 24.75  25.4w 15VG171   568  C~2nw9      
2017 09  15.58856  03 28 34.211  +18 13 52.82  26.1w 15VG171   568  C~2nw9      
2017 09  22.57478  03 28 18.863  +18 13 01.28  26.1w 15VG171   568  C~2nw9      
2017 12  13.39064  03 22 28.822  +17 53 17.60  25.1w 15VG171   568  C~2nw9      
2017 12  13.42791  03 22 28.668  +17 53 17.02  25.2w 15VG171   568  C~2nw9      

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     0.00       0.00     0.08
     2   0.0133   -113.31     0.15       0.61     0.05
     3   0.0821  -1146.10    -0.01       8.92     0.05
     4   0.0875  -1255.09     0.16      10.04     0.09
     5   0.1662  -3136.00     0.01      34.62     0.03
     6   0.1663  -3139.05     0.02      34.65    -0.01
     7   0.1664  -3142.10     0.03      34.95     0.23
     8   0.1749  -3363.73    -0.25      38.48    -0.01
     9   0.1936  -3856.58    -0.01      47.60     0.05
    10   0.1937  -3859.91     0.07      47.71     0.08
    11   0.2457  -5174.57    -0.02      78.21    -0.15
    12   0.2460  -5183.89    -0.23      78.48    -0.15
    13   0.3168  -6595.53     0.10     132.16     0.01
    14   0.3357  -6855.83    -0.04     148.10    -0.10
    15   0.4262  -7214.80     0.06     230.11    -0.11
    16   1.0020   4487.53    -0.16     478.80    -0.05
    17   1.1551   1716.37    -0.07     515.31    -0.03
    18   1.1602   1584.33    -0.02     517.45     0.01
    19   1.2969  -1722.44     0.10     598.63     0.09
    20   1.2995  -1771.53    -0.08     600.32    -0.20
    21   1.3081  -1924.01    -0.08     606.95    -0.13
    22   1.3218  -2142.88     0.17     617.67    -0.00
    23   1.3873  -2761.06     0.11     671.41    -0.16
    24   2.0231   8811.82     0.04     961.71     0.30
    25   2.0423   8586.79     0.08     965.26    -0.08
    26   2.2663   3452.46    -0.09    1060.69     0.09
    27   2.2664   3450.19    -0.01    1060.69     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.

15VG171    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        42.957    42.966    42.948
ecceobj         0.011     0.012     0.011
incobj          6.093     6.093     6.093
qmin           41.174    41.264    41.146
qmax           44.279    44.243    44.311
amean          42.650    42.659    42.642
amin           42.329    42.338    42.311
amax           42.983    42.985    42.973
emean           0.014     0.014     0.015
emin            0.000     0.000     0.000
emax            0.031     0.030     0.032
imean           4.234     4.236     4.232
imin            3.321     3.329     3.317
imax            5.280     5.276     5.286
excite_mean     0.075     0.075     0.075
fracstop        1.000     1.000     1.000
cjmean          3.079     3.079     3.079

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       180.3     179.6     180.6
kozaiamp        180.0     180.0     180.0