Orbit Fit and Astrometric record for 15VM171

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: 15VM171   
# Created Tue Apr  1 01:10:41 2025
# Orbit generated from Bernstein formalism
# Fitting     25 observations of     25
# Arc:   2.27y
# First observation: 2015/09/07
#  Last observation: 2017/12/16
Preliminary a, adot, b, bdot, g, gdot:
  -0.000073   0.019141  -0.000002   0.000568   0.021531   0.000000
# Chi-squared of fit:     5.18 DOF:     44 RMS:  0.08
# Min/Max residuals:    -0.19    0.21
# Exact a, adot, b, bdot, g, gdot:
  1.294885E-05  1.900385E-02  3.437973E-07  5.626764E-04  2.148279E-02 -1.070987E-03
# Covariance matrix:
  2.2441E-13  2.3664E-14 -8.0833E-17  5.2609E-15  1.9119E-13  5.4865E-12
  2.3664E-14  3.5989E-13 -1.8368E-15  1.4889E-14  2.9283E-13  1.5347E-11
 -8.0833E-17 -1.8368E-15  1.2339E-13 -9.1439E-14 -1.4438E-15 -1.6038E-13
  5.2609E-15  1.4889E-14 -9.1439E-14  1.2834E-13  1.6541E-14  1.0817E-12
  1.9119E-13  2.9283E-13 -1.4438E-15  1.6541E-14  4.1747E-13  1.7117E-11
  5.4865E-12  1.5347E-11 -1.6038E-13  1.0817E-12  1.7117E-11  1.1120E-09
#      lat0       lon0       xBary       yBary       zBary        JD0
   -1.180696   52.130664    0.934550   -0.007801   -0.385714  2457273.133899
# Heliocentric elements and errors
Epoch:              2457270.5000  =  2015/09/05
Mean Anomaly:          233.83934 +/-     0.636
Argument of Peri:      100.05369 +/-     0.622
Long of Asc Node:       85.92783 +/-     0.017
Inclination:             2.04399 +/-     0.001
Eccentricity:         0.10340817 +/-    0.0012
Semi-Major Axis:     43.97873311 +/-    0.0102
Time of Perihelion: 2494602.7317 +/-     187.8
Perihelion:          39.43097297 +/-    0.0528
Aphelion:            48.52649325 +/-    0.0532
Period (y)              291.6569 +/-      0.10
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           29.53907780 +/-    0.0009
Ecliptic Y           36.46907533 +/-    0.0011
Ecliptic Z           -0.95914339 +/-    0.0000
Ecliptic XDOT        -0.00199663 +/-    0.0000
Ecliptic YDOT         0.00137375 +/-    0.0000
Ecliptic ZDOT         0.00007456 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   46.94113898 +/-    0.0010
Geocenter to KBO     46.54887807 +/-    0.0014
# Hcoef:  8.26

The following table shows the complete astrometric record for 15VM171. 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 (15VM171) followed by the observatory code and reference code for the source of the astrometry.

2015 09  07.63311  03 20 08.296  +17 09 35.43  24.9w 15VM171   568  C~2nw9      
2015 09  12.49674  03 20 01.180  +17 09 02.79  25.5w 15VM171   568  C~2nw9      
2015 10  07.54436  03 18 56.758  +17 04 35.43  25.0w 15VM171   568  C~2nw9      
2015 10  07.60373  03 18 56.552  +17 04 34.66  25.7w 15VM171   568  C~2nw9      
2015 10  09.58362  03 18 49.725  +17 04 07.22  25.2w 15VM171   568  C~2nw9      
2015 11  07.33788  03 16 51.870  +16 56 27.42  25.6r 15VM171   568  C~2nw9      
2015 11  07.38006  03 16 51.675  +16 56 26.74  25.0r 15VM171   568  C~2nw9      
2015 11  07.42224  03 16 51.488  +16 56 25.97  24.8r 15VM171   568  C~2nw9      
2015 11  10.50536  03 16 37.595  +16 55 32.80  25.1w 15VM171   568  C~2nw9      
2015 12  06.36096  03 14 43.589  +16 48 25.84  25.1w 15VM171   568  C~2nw9      
2015 12  06.49848  03 14 43.033  +16 48 23.99  24.9w 15VM171   568  C~2nw9      
2016 01  01.34872  03 13 13.223  +16 43 05.11  25.1w 15VM171   568  C~2nw9      
2016 02  05.28768  03 12 28.266  +16 41 10.81  24.8w 15VM171   568  C~2nw9      
2016 02  10.30807  03 12 30.511  +16 41 29.28  25.4w 15VM171   568  C~2nw9      
2016 09  07.62568  03 24 30.071  +17 27 54.20        15VM171   568  C~2nw9      
2016 09  26.58416  03 23 52.384  +17 25 15.98  25.8w 15VM171   568  C~2nw9      
2016 10  09.54522  03 23 12.023  +17 22 36.63  25.0w 15VM171   568  C~2nw9      
2016 10  09.61729  03 23 11.761  +17 22 35.70  25.3w 15VM171   568  C~2nw9      
2016 11  04.40084  03 21 26.925  +17 15 56.49  25.1w 15VM171   568  C~2nw9      
2016 12  24.31334  03 17 57.560  +17 03 19.73  25.0w 15VM171   568  C~2nw9      
2017 01  02.41556  03 17 30.587  +17 01 49.62  25.2w 15VM171   568  C~2nw9      
2017 01  26.32908  03 16 49.884  +16 59 54.23  25.6w 15VM171   568  C~2nw9      
2017 01  27.28684  03 16 49.264  +16 59 53.49  24.9w 15VM171   568  C~2nw9      
2017 12  16.34929  03 22 51.380  +17 23 41.49  25.1w 15VM171   568  C~2nw9      
2017 12  16.36856  03 22 51.305  +17 23 41.45  24.7w 15VM171   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     0.21       0.00     0.01
     2   0.0133   -106.95    -0.03      -5.48    -0.14
     3   0.0819  -1068.18    -0.05     -27.14     0.08
     4   0.0821  -1071.23    -0.04     -27.12     0.12
     5   0.0875  -1172.89     0.02     -28.47     0.01
     6   0.1662  -2925.01    -0.04     -35.83    -0.04
     7   0.1663  -2927.88    -0.07     -35.76     0.00
     8   0.1664  -2930.68    -0.00     -35.81    -0.06
     9   0.1749  -3137.05    -0.04     -35.37    -0.19
    10   0.2457  -4828.93    -0.18     -20.29     0.00
    11   0.2460  -4837.12     0.16     -19.99     0.16
    12   0.3168  -6166.43     0.00      11.81    -0.06
    13   0.4125  -6820.21     0.03      72.46     0.04
    14   0.4262  -6784.18     0.07      81.73    -0.03
    15   1.0020   3905.20    -0.06     115.31     0.06
    16   1.0539   3343.28    -0.03      97.21     0.04
    17   1.0894   2743.93     0.09      88.15    -0.04
    18   1.0896   2740.06     0.05      88.19     0.03
    19   1.1602   1186.53    -0.11      81.50    -0.04
    20   1.2969  -1907.94     0.01     118.43     0.10
    21   1.3218  -2304.95    -0.08     131.40     0.04
    22   1.3873  -2898.82     0.02     171.30     0.03
    23   1.3899  -2907.61     0.03     172.90    -0.08
    24   2.2744   2474.26    -0.00     225.37    -0.14
    25   2.2744   2473.21     0.05     225.61     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.

15VM171    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        44.348    44.372    44.326
ecceobj         0.094     0.097     0.091
incobj          2.042     2.042     2.042
qmin           38.781    38.671    38.928
qmax           49.649    49.748    49.447
amean          44.066    44.091    44.042
amin           43.714    43.733    43.686
amax           44.447    44.483    44.430
emean           0.098     0.102     0.095
emin            0.081     0.085     0.078
emax            0.117     0.119     0.113
imean           0.765     0.773     0.758
imin            0.474     0.462     0.486
imax            1.098     1.119     1.075
excite_mean     0.099     0.103     0.096
fracstop        1.000     1.000     1.000
cjmean          3.090     3.090     3.091

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       193.2     193.1     193.6
kozaiamp        179.9     180.0     179.9