Orbit Fit and Astrometric record for 15FK564

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: 15FK564   
# Created Sun Oct 19 01:10:51 2025
# Orbit generated from Bernstein formalism
# Fitting     34 observations of     34
# Arc:  62.84d
# First observation: 2015/01/16
#  Last observation: 2015/03/20
Preliminary a, adot, b, bdot, g, gdot:
  -0.000000   0.016281   0.000001   0.006824   0.020447   0.000000
# Chi-squared of fit:    18.30 DOF:     62 RMS:  0.13
# Min/Max residuals:    -0.25    0.41
# Exact a, adot, b, bdot, g, gdot:
  1.208957E-05  1.582758E-02  6.143938E-06  6.808612E-03  2.034536E-02  1.563176E-03
# Covariance matrix:
  1.8162E-13  1.1102E-10  5.8106E-14  2.6947E-12  2.2426E-11  1.3156E-09
  1.1102E-10  1.6386E-07  8.2219E-11  3.0760E-09  3.0522E-08  1.1322E-06
  5.8106E-14  8.2219E-11  9.9318E-14  1.1911E-12  1.5393E-11  5.9328E-10
  2.6947E-12  3.0760E-09  1.1911E-12  7.5105E-11  5.9408E-10  2.8128E-08
  2.2426E-11  3.0522E-08  1.5393E-11  5.9408E-10  5.7441E-09  2.2998E-07
  1.3156E-09  1.1322E-06  5.9328E-10  2.8128E-08  2.2998E-07  1.4041E-05
#      lat0       lon0       xBary       yBary       zBary        JD0
   -9.059655  151.506080    0.574045   -0.125259   -0.786589  2457039.040018
# Heliocentric elements and errors
Epoch:              2457030.5000  =  2015/01/08
Mean Anomaly:          130.21972 +/-    87.728
Argument of Peri:      198.86552 +/-    83.908
Long of Asc Node:      170.82447 +/-     0.505
Inclination:            24.65360 +/-     0.530
Eccentricity:         0.11387169 +/-    0.1113
Semi-Major Axis:     46.23015242 +/-    2.4398
Time of Perihelion: 2415500.6218 +/-   27784.4
Perihelion:          40.96584663 +/-    5.5791
Aphelion:            51.49445820 +/-    5.8170
Period (y)              314.3375 +/-     24.88
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -43.08794685 +/-    0.1589
Ecliptic Y           24.04061276 +/-    0.0863
Ecliptic Z           -7.73921651 +/-    0.0288
Ecliptic XDOT        -0.00132934 +/-    0.0005
Ecliptic YDOT        -0.00170931 +/-    0.0002
Ecliptic ZDOT         0.00087177 +/-    0.0001
# Distances at JD0 (AU)
Heliocenter to KBO   49.94414578 +/-    0.1433
Geocenter to KBO     49.15125260 +/-    0.1831
# Hcoef:  8.79

The following table shows the complete astrometric record for 15FK564. 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 (15FK564) followed by the observatory code and reference code for the source of the astrometry.

2015 01  16.53924  10 01 14.03   +02 27 37.5   25.3z 15FK564   T09  C~90HY      
2015 01  16.54315  10 01 14.02   +02 27 37.9   25.2z 15FK564   T09  C~90HY      
2015 01  16.55599  10 01 13.97   +02 27 37.7   25.3z 15FK564   T09  C~90HY      
2015 01  16.56849  10 01 13.94   +02 27 38.0   25.3z 15FK564   T09  C~90HY      
2015 01  16.57632  10 01 13.90   +02 27 38.2   25.1z 15FK564   T09  C~90HY      
2015 01  16.61461  10 01 13.78   +02 27 38.9   25.3z 15FK564   T09  C~90HY      
2015 01  16.61862  10 01 13.76   +02 27 38.9   25.4z 15FK564   T09  C~90HY      
2015 01  16.62952  10 01 13.74   +02 27 38.9   24.9z 15FK564   T09  C~90HY      
2015 01  16.63677  10 01 13.71   +02 27 39.1   25.0z 15FK564   T09  C~90HY      
2015 01  17.36841  10 01 11.35   +02 27 50.1   26.2i 15FK564   T09  C~90HY      
2015 01  17.40524  10 01 11.23   +02 27 51.2   26.6i 15FK564   T09  C~90HY      
2015 01  17.40983  10 01 11.20   +02 27 50.8   25.8i 15FK564   T09  C~90HY      
2015 01  17.41437  10 01 11.19   +02 27 51.0   25.4i 15FK564   T09  C~90HY      
2015 01  17.42357  10 01 11.18   +02 27 51.0   26.1i 15FK564   T09  C~90HY      
2015 01  17.42812  10 01 11.16   +02 27 51.2   25.8i 15FK564   T09  C~90HY      
2015 01  17.43268  10 01 11.16   +02 27 51.2   25.3i 15FK564   T09  C~90HY      
2015 01  20.42343  10 01 01.18   +02 28 39.0   26.6g 15FK564   T09  C~90HY      
2015 01  20.43306  10 01 01.16   +02 28 39.0   26.3g 15FK564   T09  C~90HY      
2015 01  20.43784  10 01 01.15   +02 28 39.0   26.4g 15FK564   T09  C~90HY      
2015 01  21.55881  10 00 57.30   +02 28 57.8   25.8i 15FK564   T09  C~90HY      
2015 01  21.56653  10 00 57.29   +02 28 58.2   25.5i 15FK564   T09  C~90HY      
2015 01  21.57534  10 00 57.23   +02 28 58.2   25.2i 15FK564   T09  C~90HY      
2015 01  21.58764  10 00 57.19   +02 28 58.2   25.3i 15FK564   T09  C~90HY      
2015 01  21.59540  10 00 57.17   +02 28 58.4   25.7i 15FK564   T09  C~90HY      
2015 01  21.60268  10 00 57.14   +02 28 58.5   25.6i 15FK564   T09  C~90HY      
2015 01  21.61742  10 00 57.10   +02 28 58.9   25.6i 15FK564   T09  C~90HY      
2015 01  21.62126  10 00 57.10   +02 28 58.9   25.3i 15FK564   T09  C~90HY      
2015 03  18.39076  09 57 27.87   +02 51 43.5   26.2r 15FK564   T09  C~90HY      
2015 03  18.42974  09 57 27.75   +02 51 44.7   25.6r 15FK564   T09  C~90HY      
2015 03  18.44789  09 57 27.68   +02 51 45.0   25.6r 15FK564   T09  C~90HY      
2015 03  20.33757  09 57 21.47   +02 52 37.5   25.5i 15FK564   T09  C~90HY      
2015 03  20.35412  09 57 21.43   +02 52 37.8   25.6i 15FK564   T09  C~90HY      
2015 03  20.36873  09 57 21.38   +02 52 38.3   25.9i 15FK564   T09  C~90HY      
2015 03  20.38334  09 57 21.33   +02 52 38.7   25.6i 15FK564   T09  C~90HY      

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     0.04       0.00    -0.18
     2   0.0000     -0.28    -0.04       0.32     0.16
     3   0.0000     -0.91    -0.01      -0.13    -0.25
     4   0.0001     -1.44     0.11      -0.00    -0.08
     5   0.0001     -2.07    -0.12      -0.03    -0.08
     6   0.0002     -4.00    -0.08       0.00     0.07
     7   0.0002     -4.28    -0.15      -0.10    -0.02
     8   0.0002     -4.56     0.13      -0.21    -0.09
     9   0.0003     -5.05     0.01      -0.18    -0.04
    10   0.0023    -42.03     0.01      -2.25    -0.11
    11   0.0024    -44.10    -0.15      -1.85     0.41
    12   0.0024    -44.38    -0.19      -2.38    -0.11
    13   0.0024    -44.59    -0.17      -2.25     0.04
    14   0.0024    -44.73     0.17      -2.30     0.01
    15   0.0024    -45.09     0.05      -2.22     0.11
    16   0.0024    -45.09     0.29      -2.22     0.12
    17   0.0106   -201.92    -0.14      -9.77     0.14
    18   0.0107   -202.20     0.10      -9.87     0.06
    19   0.0107   -202.34     0.22      -9.92     0.02
    20   0.0137   -262.97    -0.02     -12.50    -0.07
    21   0.0138   -263.25     0.13     -12.18     0.27
    22   0.0138   -264.09    -0.23     -12.49    -0.02
    23   0.0138   -264.65    -0.11     -12.70    -0.20
    24   0.0138   -265.00    -0.03     -12.62    -0.10
    25   0.0139   -265.46    -0.09     -12.68    -0.15
    26   0.0139   -266.16     0.02     -12.52     0.05
    27   0.0139   -266.16     0.23     -12.52     0.06
    28   0.1666  -3680.81    -0.11     170.20     0.00
    29   0.1667  -3682.91     0.02     170.70     0.18
    30   0.1668  -3684.00    -0.03     170.61    -0.06
    31   0.1719  -3789.55    -0.14     187.33    -0.01
    32   0.1720  -3790.21     0.12     187.40    -0.08
    33   0.1720  -3791.09     0.07     187.60    -0.00
    34   0.1721  -3791.93     0.05     187.72    -0.02

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.

15FK564    quality flag:0

Type:      ERR2LARGE ERR2LARGE ERR2LARGE

axisobj         0.000     0.000     0.000
ecceobj        -1.000    -1.000    -1.000
incobj         -1.000    -1.000    -1.000
qmin            0.000     0.000     0.000
qmax            0.000     0.000     0.000
amean           0.000     0.000     0.000
amin            0.000     0.000     0.000
amax            0.000     0.000     0.000
emean           0.000     0.000     0.000
emin            0.000     0.000     0.000
emax            0.000     0.000     0.000
imean           0.000     0.000     0.000
imin            0.000     0.000     0.000
imax            0.000     0.000     0.000
excite_mean     0.000     0.000     0.000
fracstop        0.000     0.000     0.000
cjmean          0.000     0.000     0.000

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         0.0       0.0       0.0
kozaiamp          0.0       0.0       0.0