Orbit Fit and Astrometric record for 15KQ175

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: 15KQ175   
# Created Wed May  8 01:17:11 2024
# Orbit generated from Bernstein formalism
# Fitting     25 observations of     26
# Arc:   2.03y
# First observation: 2015/03/19
#  Last observation: 2017/03/28
Preliminary a, adot, b, bdot, g, gdot:
  -0.000184   0.027449   0.000014  -0.005017   0.026193   0.000000
# Chi-squared of fit:     6.19 DOF:     44 RMS:  0.09
# Min/Max residuals:    -0.19    0.19
# Exact a, adot, b, bdot, g, gdot:
  1.611060E-05  2.724014E-02 -2.622660E-06 -4.992247E-03  2.616367E-02 -2.982365E-04
# Covariance matrix:
  2.6723E-13 -1.4514E-13 -5.7652E-15 -3.1494E-15  1.6685E-13  8.0924E-13
 -1.4514E-13  6.0045E-13  1.3805E-14 -9.0001E-14  1.5279E-13  1.2495E-11
 -5.7652E-15  1.3805E-14  1.3362E-13 -1.2697E-13 -1.2671E-15  3.8123E-13
 -3.1494E-15 -9.0001E-14 -1.2697E-13  2.2664E-13 -4.5268E-14 -2.9365E-12
  1.6685E-13  1.5279E-13 -1.2671E-15 -4.5268E-14  2.8908E-13  6.7737E-12
  8.0924E-13  1.2495E-11  3.8123E-13 -2.9365E-12  6.7737E-12  4.1181E-10
#      lat0       lon0       xBary       yBary       zBary        JD0
    8.234129 -122.475362    0.850757    0.073306   -0.505772  2457101.145738
# Heliocentric elements and errors
Epoch:              2457100.5000  =  2015/03/19
Mean Anomaly:          345.15121 +/-     0.342
Argument of Peri:      159.53817 +/-     0.428
Long of Asc Node:       94.32077 +/-     0.003
Inclination:            13.03335 +/-     0.001
Eccentricity:         0.10408029 +/-    0.0002
Semi-Major Axis:     43.03072084 +/-    0.0041
Time of Perihelion: 2461353.1048 +/-      98.1
Perihelion:          38.55207101 +/-    0.0103
Aphelion:            47.50937066 +/-    0.0107
Period (y)              282.2774 +/-      0.04
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -21.30540836 +/-    0.0004
Ecliptic Y          -31.88588851 +/-    0.0006
Ecliptic Z            5.47387513 +/-    0.0001
Ecliptic XDOT         0.00237775 +/-    0.0000
Ecliptic YDOT        -0.00157338 +/-    0.0000
Ecliptic ZDOT        -0.00052140 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   38.73749631 +/-    0.0006
Geocenter to KBO     38.22093636 +/-    0.0008
# Hcoef:  8.84

The following table shows the complete astrometric record for 15KQ175. 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 (15KQ175) followed by the observatory code and reference code for the source of the astrometry.

2015 03  19.64496  15 48 36.019  -11 34 43.36  24.5r 15KQ175   568  C~2nvh      
2015 03  22.56564  15 48 29.923  -11 33 57.41  24.7r 15KQ175   568  C~2nvh      
2015 04  13.57652  15 47 20.627  -11 27 36.56  24.8r 15KQ175   568  C~2nvh      
2015 04  13.61766  15 47 20.460  -11 27 35.72  24.8r 15KQ175   568  C~2nvh      
2015 04  18.58658  15 46 59.957  -11 26 04.91  25.0r 15KQ175   568  C~2nvh      
2015 05  21.34720  15 44 19.983  -11 16 58.42  24.5r 15KQ175   568  C~2nvh      
2015 05  21.38827  15 44 19.775  -11 16 57.93  24.6r 15KQ175   568  C~2nvh      
2015 05  21.42959  15 44 19.543  -11 16 57.43  24.6r 15KQ175   568  C~2nvh      
2015 05  22.50587  15 44 13.972  -11 16 42.64  24.6r 15KQ175   568  C~2nvh      
2015 05  25.49667  15 43 58.562  -11 16 02.94  24.4r 15KQ175   568  C~2nvi      
2015 06  20.38581  15 41 54.277  -11 12 10.08  24.7r 15KQ175   568  C~2nvi      
2015 06  20.42660  15 41 54.097  -11 12 09.87  24.7r 15KQ175   568  C~2nvi      
2015 06  23.44700  15 41 41.456  -11 11 57.89  24.6r 15KQ175   568  C~2nvi      
2015 07  12.30961  15 40 36.300  -11 12 03.72  24.2r 15KQ175   568  C~2nvi      
2015 07  18.39769  15 40 21.155  -11 12 36.45  24.7r 15KQ175   568  C~2nvi      
2016 02  06.64531  15 54 22.201  -12 17 42.81  24.7w 15KQ175   568  C~2nvi      
2016 02  12.63086  15 54 35.205  -12 17 24.70  24.9w 15KQ175   568  C~2nvi      
2016 03  15.64428  15 54 40.515  -12 12 27.95  25.6w 15KQ175   568  C~2nvi      
2016 04  03.55878  15 53 55.440  -12 07 37.73  24.9w 15KQ175   568  C~2nvi      
2016 04  08.60833  15 53 38.245  -12 06 12.32  25.3w 15KQ175   568  C~2nvi      
2016 04  09.55226  15 53 34.832  -12 05 56.26  25.0w 15KQ175   568  C~2nvi      
2016 04  29.50547  15 52 09.523  -12 00 12.90  24.9w 15KQ175   568  C~2nvi      
2016 05  04.47810  15 51 45.317  -11 58 50.59  24.9w 15KQ175   568  C~2nvi      
2016 05  30.45392  15 49 32.038  -11 52 44.59  24.7w 15KQ175   568  C~2nvi      
2016 07  04.31437  15 46 57.641  -11 49 30.84  24.9w 15KQ175   568  C~2nvi      
2017 03  28.61223  16 00 16.497  -12 46 00.72  25.2w 15KQ175   568  C~2nvi      

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    -0.08
     2   0.0080    -97.45    -0.01      25.31     0.19
     3   0.0683  -1174.60    -0.06     174.31    -0.05
     4   0.0684  -1177.18    -0.08     174.59     0.04
     5   0.0820  -1491.20 (  -0.16)    197.11 (   0.44)
     6   0.1717  -3906.85    -0.01     211.41     0.17
     7   0.1718  -3909.94     0.12     211.21     0.12
     8   0.1719  -3913.38    -0.07     210.94    -0.00
     9   0.1748  -3996.60    -0.08     207.20    -0.10
    10   0.1830  -4226.54    -0.00     195.63    -0.19
    11   0.2539  -6062.16     0.09      15.22    -0.04
    12   0.2540  -6064.79     0.05      14.83    -0.02
    13   0.2623  -6248.93     0.00     -15.12    -0.07
    14   0.3139  -7182.91     0.00    -235.95     0.05
    15   0.3306  -7392.96    -0.05    -318.00    -0.05
    16   0.8871   5518.31     0.14   -1424.36    -0.13
    17   0.9035   5700.81    -0.15   -1366.10    -0.11
    18   0.9911   5713.73    -0.02   -1059.45    -0.05
    19   1.0429   5005.64    -0.04    -916.59    -0.04
    20   1.0567   4740.89     0.02    -886.97     0.16
    21   1.0593   4688.53     0.17    -881.97     0.12
    22   1.1139   3392.07    -0.07    -814.69     0.14
    23   1.1275   3027.42     0.03    -810.69    -0.07
    24   1.1987   1038.33    -0.03    -876.29     0.04
    25   1.2941  -1215.93    -0.00   -1182.07     0.05
    26   2.0259  10956.40    -0.02   -1995.03    -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.

15KQ175    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        42.676    42.689    42.664
ecceobj         0.099     0.099     0.099
incobj         13.033    13.033    13.033
qmin           37.932    37.993    37.934
qmax           48.338    48.285    48.385
amean          43.009    43.022    42.999
amin           42.666    42.682    42.652
amax           43.381    43.391    43.365
emean           0.099     0.099     0.099
emin            0.084     0.085     0.084
emax            0.115     0.114     0.116
imean          11.096    11.098    11.092
imin           10.326    10.322    10.327
imax           11.859    11.844    11.856
excite_mean     0.216     0.217     0.216
fracstop        1.000     1.000     1.000
cjmean          3.034     3.034     3.034

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       180.0     180.1     180.0
kozaiamp        180.0     180.0     180.0