Orbit Fit and Astrometric record for 15VN172

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: 15VN172   
# Created Fri May  3 01:17:48 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     27 observations of     27
# Arc:   6.24y
# First observation: 2015/09/06
#  Last observation: 2021/12/01
# Chi-squared of fit:     6.55 DOF:     48 RMS:  0.09
# Min/Max residuals:    -0.14    0.23
# Exact a, adot, b, bdot, g, gdot:
  1.423403E-05  1.908397E-02  7.679396E-07  6.740545E-04  2.131858E-02  1.056500E-03
# Covariance matrix:
  3.2802E-13 -6.3920E-14  1.1603E-15 -2.2487E-15  1.9208E-13 -5.0364E-13
 -6.3920E-14  1.8390E-13 -4.1588E-15  7.5093E-15  6.7645E-14  1.7373E-12
  1.1603E-15 -4.1588E-15  8.3923E-14 -2.2120E-14 -1.5666E-15 -4.3046E-14
 -2.2487E-15  7.5093E-15 -2.2120E-14  1.6252E-14  2.6914E-15  7.7771E-14
  1.9208E-13  6.7645E-14 -1.5666E-15  2.6914E-15  2.1412E-13  6.3750E-13
 -5.0364E-13  1.7373E-12 -4.3046E-14  7.7771E-14  6.3750E-13  1.7988E-11
#      lat0       lon0       xBary       yBary       zBary        JD0
    0.040967   50.888314    0.932990    0.000426   -0.390133  2457272.119709
# Heliocentric elements and errors
Epoch:              2457272.5000  =  2015/09/07
Mean Anomaly:          136.94844 +/-     0.217
Argument of Peri:      220.43997 +/-     0.213
Long of Asc Node:       48.61181 +/-     0.001
Inclination:             2.02587 +/-     0.000
Eccentricity:         0.05036306 +/-    0.0001
Semi-Major Axis:     45.57570978 +/-    0.0039
Time of Perihelion: 2414520.8193 +/-      67.9
Perihelion:          43.28037760 +/-    0.0066
Aphelion:            47.87104196 +/-    0.0068
Period (y)              307.6864 +/-      0.04
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           30.55674379 +/-    0.0007
Ecliptic Y           36.11024599 +/-    0.0008
Ecliptic Z            0.03358427 +/-    0.0000
Ecliptic XDOT        -0.00181799 +/-    0.0000
Ecliptic YDOT         0.00164491 +/-    0.0000
Ecliptic ZDOT         0.00008672 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   47.30394809 +/-    0.0007
Geocenter to KBO     46.90743058 +/-    0.0010
# Hcoef:  7.39

The following table shows the complete astrometric record for 15VN172. 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 (15VN172) followed by the observatory code and reference code for the source of the astrometry.

2015 09  06.61892  03 13 46.375  +18 01 01.01  24.3w 15VN172   568  C~2nwD      
2015 11  07.35377  03 10 25.222  +17 48 15.71  24.0r 15VN172   568  C~2nwD      
2015 11  07.39585  03 10 25.026  +17 48 14.99  24.1r 15VN172   568  C~2nwD      
2015 11  07.43803  03 10 24.835  +17 48 14.27  24.1r 15VN172   568  C~2nwD      
2015 11  10.52298  03 10 11.016  +17 47 20.21        15VN172   568  C~2nwD      
2015 11  17.36965  03 09 40.306  +17 45 20.55  24.3w 15VN172   568  C~2nwD      
2015 11  17.41626  03 09 40.093  +17 45 19.75  24.2w 15VN172   568  C~2nwD      
2015 12  06.37850  03 08 18.632  +17 40 00.61  24.5w 15VN172   568  C~2nwD      
2015 12  13.31287  03 07 51.736  +17 38 14.76  24.2w 15VN172   568  C~2nwD      
2015 12  13.37141  03 07 51.517  +17 38 13.89  24.3w 15VN172   568  C~2nwD      
2016 01  01.36607  03 06 51.328  +17 34 17.22  24.5w 15VN172   568  C~2nwD      
2016 01  07.31283  03 06 37.468  +17 33 22.93  24.6w 15VN172   568  C~2nwD      
2016 02  04.28927  03 06 11.210  +17 31 45.41  24.2w 15VN172   568  C~2nwD      
2016 09  06.61138  03 18 08.885  +18 20 16.82        15VN172   568  C~2nwD      
2016 09  26.60062  03 17 27.961  +18 17 50.66  24.0w 15VN172   568  C~2nwD      
2016 10  27.50259  03 15 35.805  +18 10 54.14  24.3w 15VN172   568  C~2nwD      
2016 11  02.60863  03 15 09.206  +18 09 13.95  24.3w 15VN172   568  C~2nwD      
2016 11  03.52763  03 15 05.160  +18 08 58.65  24.3w 15VN172   568  C~2nwD      
2016 12  29.38063  03 11 20.904  +17 54 41.06  24.4w 15VN172   568  C~2nwD      
2017 01  02.38784  03 11 10.267  +17 54 00.24  24.6w 15VN172   568  C~2nwD      
2017 01  26.27742  03 10 33.056  +17 51 39.22  24.3w 15VN172   568  C~2nwD      
2017 01  26.29981  03 10 33.042  +17 51 39.16  24.5w 15VN172   568  C~2nwD      
2017 12  13.37637  03 16 39.994  +18 17 44.09  24.2w 15VN172   568  C~2nwD      
2017 12  13.41395  03 16 39.840  +18 17 43.39  24.3w 15VN172   568  C~2nwD      
2021 12  01.260670 03 35 21.313  +19 34 59.12  24.2G 15VN172   G37  C~5J85      
2021 12  01.310190 03 35 21.108  +19 34 58.06        15VN172   G37  C~5J85      
2021 12  01.385990 03 35 20.759  +19 34 57.05        15VN172   G37  C~5J85      

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    -0.06
     2   0.1690      0.00    -0.03       0.00     0.21
     3   0.1691      0.00    -0.10       0.00     0.22
     4   0.1693      0.00    -0.09       0.00     0.23
     5   0.1777      0.00     0.01       0.00    -0.10
     6   0.1964      0.00     0.04       0.00    -0.03
     7   0.1966      0.00     0.03       0.00    -0.02
     8   0.2485      0.00    -0.01       0.00     0.01
     9   0.2675      0.00    -0.02       0.00    -0.07
    10   0.2676      0.00     0.03       0.00    -0.08
    11   0.3196      0.00     0.03       0.00    -0.05
    12   0.3359      0.00     0.05       0.00    -0.12
    13   0.4125      0.00     0.01       0.00     0.06
    14   1.0020      0.00     0.06       0.00    -0.05
    15   1.0568      0.00     0.05       0.00     0.01
    16   1.1414      0.00     0.06       0.00    -0.02
    17   1.1581      0.00    -0.12       0.00    -0.05
    18   1.1606      0.00     0.11       0.00    -0.02
    19   1.3135      0.00     0.02       0.00    -0.04
    20   1.3245      0.00    -0.11       0.00     0.01
    21   1.3899      0.00     0.10       0.00    -0.03
    22   1.3900      0.00     0.10       0.00    -0.04
    23   2.2690      0.00     0.03       0.00     0.09
    24   2.2691      0.00    -0.09       0.00    -0.07
    25   6.2358      0.00    -0.14       0.00     0.18
    26   6.2360      0.00     0.13       0.00    -0.14
    27   6.2362      0.00     0.00       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.

15VN172    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        46.020    46.020    46.020
ecceobj         0.047     0.047     0.047
incobj          2.017     2.017     2.017
qmin           42.789    42.780    42.784
qmax           48.795    48.796    48.793
amean          45.687    45.687    45.687
amin           45.324    45.323    45.326
amax           46.061    46.062    46.059
emean           0.047     0.047     0.047
emin            0.034     0.034     0.034
emax            0.060     0.060     0.060
imean           1.480     1.480     1.480
imin            1.066     1.066     1.066
imax            1.869     1.869     1.868
excite_mean     0.054     0.054     0.054
fracstop        1.000     1.000     1.000
cjmean          3.119     3.119     3.119

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       210.7     210.7     210.7
kozaiamp        179.9     180.0     180.0