Orbit Fit and Astrometric record for 15VV227

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: 15VV227   
# Created Thu Mar 27 01:10:53 2025
# Orbit generated from Bernstein formalism
# Fitting     26 observations of     26
# Arc:   0.97y
# First observation: 2015/01/21
#  Last observation: 2016/01/09
Preliminary a, adot, b, bdot, g, gdot:
  -0.000197   0.031858   0.000008  -0.002080   0.027454   0.000000
# Chi-squared of fit:    13.66 DOF:     46 RMS:  0.13
# Min/Max residuals:    -0.26    0.26
# Exact a, adot, b, bdot, g, gdot:
  1.784561E-05  3.217375E-02 -1.432248E-06 -2.073705E-03  2.797343E-02  3.061308E-04
# Covariance matrix:
  1.9412E-13  4.0738E-13 -3.6235E-15 -1.2066E-14  3.3183E-13  1.9916E-11
  4.0738E-13  5.3618E-11 -9.4243E-14  6.1139E-13  1.5522E-11  1.5338E-09
 -3.6235E-15 -9.4243E-14  1.2015E-13 -1.5293E-13 -3.3968E-14 -2.8607E-12
 -1.2066E-14  6.1139E-13 -1.5293E-13  3.8495E-13  1.3261E-13  1.6587E-11
  3.3183E-13  1.5522E-11 -3.3968E-14  1.3261E-13  4.9409E-12  4.5648E-10
  1.9916E-11  1.5338E-09 -2.8607E-12  1.6587E-11  4.5648E-10  4.4394E-08
#      lat0       lon0       xBary       yBary       zBary        JD0
  -15.136086  139.570897    0.317276   -0.242502   -0.897152  2457043.938318
# Heliocentric elements and errors
Epoch:              2457040.5000  =  2015/01/18
Mean Anomaly:            0.04055 +/-     1.158
Argument of Peri:      255.74018 +/-     1.944
Long of Asc Node:      243.73011 +/-     0.006
Inclination:            15.22958 +/-     0.000
Eccentricity:         0.23848332 +/-    0.0004
Semi-Major Axis:     48.12776499 +/-    0.0243
Time of Perihelion: 2457026.7635 +/-     392.3
Perihelion:          36.65009566 +/-    0.0283
Aphelion:            59.60543432 +/-    0.0370
Period (y)              333.8887 +/-      0.25
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -26.77283261 +/-    0.0021
Ecliptic Y           23.22315201 +/-    0.0018
Ecliptic Z           -9.33438399 +/-    0.0007
Ecliptic XDOT        -0.00202764 +/-    0.0000
Ecliptic YDOT        -0.00241799 +/-    0.0000
Ecliptic ZDOT        -0.00020365 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   36.65010340 +/-    0.0019
Geocenter to KBO     35.74821045 +/-    0.0028
# Hcoef:  8.96

The following table shows the complete astrometric record for 15VV227. 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 (15VV227) followed by the observatory code and reference code for the source of the astrometry.

2015 01  21.43754  09 09 10.37   +00 32 28.4   24.2i 15VV227   T09  C~8kvj      
2015 01  21.44452  09 09 10.31   +00 32 28.4   24.2i 15VV227   T09  C~8kvj      
2015 01  21.45697  09 09 10.26   +00 32 28.6   24.3i 15VV227   T09  C~8kvj      
2015 01  21.47327  09 09 10.19   +00 32 28.8   24.3i 15VV227   T09  C~8kvj      
2015 01  21.49519  09 09 10.06   +00 32 29.1   24.1i 15VV227   T09  C~8kvj      
2015 01  21.51165  09 09 09.98   +00 32 29.5   24.3i 15VV227   T09  C~8kvj      
2015 01  21.52917  09 09 09.89   +00 32 29.6   24.3i 15VV227   T09  C~8kvj      
2015 03  18.33529  09 04 40.59   +00 56 31.3   25.1r 15VV227   T09  C~8kvj      
2015 03  18.34385  09 04 40.55   +00 56 31.3   24.7r 15VV227   T09  C~8kvj      
2015 03  18.36546  09 04 40.47   +00 56 32.1   25.3r 15VV227   T09  C~8kvj      
2015 03  18.37860  09 04 40.44   +00 56 32.6   24.7r 15VV227   T09  C~8kvj      
2015 03  18.38081  09 04 40.41   +00 56 32.6   24.8r 15VV227   T09  C~8kvj      
2015 03  25.38568  09 04 17.59   +01 00 14.9   25.0g 15VV227   T09  C~8kvj      
2015 03  25.39368  09 04 17.57   +01 00 15.4   25.3g 15VV227   T09  C~8kvj      
2015 03  25.41289  09 04 17.51   +01 00 15.9   25.4g 15VV227   T09  C~8kvj      
2015 11  08.54855  09 19 00.85   +00 05 23.4   24.7r 15VV227   T09  C~8kvj      
2015 11  08.56993  09 19 00.87   +00 05 22.5   24.4r 15VV227   T09  C~8kvj      
2015 11  08.58902  09 19 00.88   +00 05 22.0   25.0r 15VV227   T09  C~8kvj      
2015 11  08.63991  09 19 00.97   +00 05 20.5   25.1r 15VV227   T09  C~8kvj      
2015 11  14.60004  09 19 06.17   +00 02 11.6   25.3g 15VV227   T09  C~8kvj      
2015 11  14.63222  09 19 06.18   +00 02 10.9   25.0g 15VV227   T09  C~8kvj      
2015 11  14.63646  09 19 06.17   +00 02 10.9   24.7g 15VV227   T09  C~8kvj      
2016 01  09.47070  09 17 02.55   -00 09 54.2   24.1y 15VV227   T09  C~8kvj      
2016 01  09.53920  09 17 02.25   -00 09 53.8   24.1y 15VV227   T09  C~8kvj      
2016 01  09.56090  09 17 02.13   -00 09 53.3   23.9y 15VV227   T09  C~8kvj      
2016 01  09.57457  09 17 02.06   -00 09 53.3   23.9y 15VV227   T09  C~8kvj      

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     0.07       0.00     0.05
     2   0.0000     -0.86    -0.24      -0.27    -0.15
     3   0.0001     -1.63    -0.04      -0.31    -0.06
     4   0.0001     -2.69     0.18      -0.44    -0.02
     5   0.0002     -4.64    -0.04      -0.74    -0.10
     6   0.0002     -5.91    -0.01      -0.72     0.08
     7   0.0003     -7.23     0.05      -1.04    -0.05
     8   0.1530  -4293.91     0.03     150.42     0.18
     9   0.1531  -4294.48    -0.01     150.24    -0.12
    10   0.1531  -4295.87    -0.07     150.64    -0.02
    11   0.1532  -4296.45     0.16     150.98     0.13
    12   0.1532  -4296.88    -0.13     150.84    -0.03
    13   0.1723  -4690.53     0.02     259.21    -0.08
    14   0.1724  -4690.97     0.01     259.59     0.18
    15   0.1724  -4691.98     0.02     259.80     0.07
    16   0.7970   8938.80    -0.05    1135.28     0.05
    17   0.7971   8939.36    -0.05    1134.51    -0.15
    18   0.7971   8939.65    -0.26    1134.08    -0.08
    19   0.7973   8941.40     0.17    1133.06     0.25
    20   0.8136   9073.21     0.26     976.54    -0.23
    21   0.8137   9073.56     0.11     975.91     0.00
    22   0.8137   9073.42    -0.10     975.87     0.07
    23   0.9666   7523.38     0.05    -278.01    -0.15
    24   0.9667   7518.97     0.26    -279.00    -0.08
    25   0.9668   7517.10    -0.15    -279.06     0.18
    26   0.9668   7516.09    -0.23    -279.38     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.

15VV227    quality flag:3

Type:           2:1E      2:1E      2:1E

axisobj        47.847    48.070    47.670
ecceobj         0.233     0.238     0.230
incobj         15.208    15.209    15.207
qmin           35.099    35.400    35.255
qmax           61.230    61.279    61.490
amean          47.795    47.797    47.796
amin           47.167    47.079    47.112
amax           48.520    48.603    48.603
emean           0.235     0.238     0.238
emin            0.205     0.213     0.208
emax            0.264     0.262     0.265
imean          15.717    16.267    16.252
imin           14.779    15.588    15.539
imax           16.665    17.061    17.181
excite_mean     0.359     0.367     0.368
fracstop        1.000     1.000     1.000
cjmean          2.987     2.979     2.978

libcent 0       179.4     179.1     181.3
libamp  0       151.0     165.7     164.1
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       191.5     188.1     192.5
kozaiamp        180.0     180.0     180.0