Orbit Fit and Astrometric record for 17BK232

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: 17BK232   
# Created Fri Nov 22 02:10:48 2024
# Orbit generated from Bernstein formalism
# Fitting     22 observations of     22
# Arc:   0.90y
# First observation: 2016/04/02
#  Last observation: 2017/02/23
Preliminary a, adot, b, bdot, g, gdot:
  -0.000038   0.022658   0.000006  -0.007226   0.023564   0.000000
# Chi-squared of fit:    10.28 DOF:     38 RMS:  0.12
# Min/Max residuals:    -0.29    0.28
# Exact a, adot, b, bdot, g, gdot:
  1.433331E-05  2.261869E-02 -4.618369E-06 -7.272317E-03  2.391057E-02 -2.083323E-03
# Covariance matrix:
  2.6188E-13  1.3515E-12  3.4271E-14 -4.2705E-13  8.3202E-13  6.3593E-11
  1.3515E-12  2.0023E-10  3.4990E-12 -4.5922E-11  6.8001E-11  6.8297E-09
  3.4271E-14  3.4990E-12  2.0700E-13 -1.0047E-12  1.2121E-12  1.2037E-10
 -4.2705E-13 -4.5922E-11 -1.0047E-12  1.1100E-11 -1.5842E-11 -1.5775E-09
  8.3202E-13  6.8001E-11  1.2121E-12 -1.5842E-11  2.4042E-11  2.3564E-09
  6.3593E-11  6.8297E-09  1.2037E-10 -1.5775E-09  2.3564E-09  2.3462E-07
#      lat0       lon0       xBary       yBary       zBary        JD0
    1.725733 -175.479906   -0.142990    0.029812   -0.984842  2457480.890761
# Heliocentric elements and errors
Epoch:              2457480.5000  =  2016/04/02
Mean Anomaly:          320.09402 +/-     4.902
Argument of Peri:      224.16531 +/-     7.044
Long of Asc Node:        9.95478 +/-     0.001
Inclination:            17.85997 +/-     0.003
Eccentricity:         0.11840526 +/-    0.0164
Semi-Major Axis:     46.74765232 +/-    0.1716
Time of Perihelion: 2470421.6710 +/-    1587.9
Perihelion:          41.21248446 +/-    0.7801
Aphelion:            52.28282017 +/-    0.7889
Period (y)              319.6303 +/-      1.76
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -42.64820663 +/-    0.0085
Ecliptic Y           -3.51732179 +/-    0.0007
Ecliptic Z            1.25932132 +/-    0.0002
Ecliptic XDOT         0.00041692 +/-    0.0001
Ecliptic YDOT        -0.00257204 +/-    0.0000
Ecliptic ZDOT        -0.00083951 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   42.81152849 +/-    0.0085
Geocenter to KBO     41.82250688 +/-    0.0086
# Hcoef:  8.28

The following table shows the complete astrometric record for 17BK232. 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 (17BK232) followed by the observatory code and reference code for the source of the astrometry.

2016 04  02.389972 12 19 19.93   -00 12 44.0         17BK232   T09  C~83Eq      
2016 04  02.515196 12 19 19.36   -00 12 41.0         17BK232   T09  C~83Eq      
2016 04  04.34598  12 19 11.17   -00 11 56.6   25.0g 17BK232   T09  C~89UT      
2016 04  04.36164  12 19 11.09   -00 11 56.4   25.2g 17BK232   T09  C~89UT      
2016 04  04.38727  12 19 10.99   -00 11 55.8   25.1g 17BK232   T09  C~89UT      
2016 04  04.41295  12 19 10.88   -00 11 55.1   25.2g 17BK232   T09  C~89UT      
2016 06  04.25196  12 16 00.04   +00 02 33.4   24.8z 17BK232   T09  C~8COq      
2016 06  04.27037  12 16 00.02   +00 02 33.2   24.0z 17BK232   T09  C~8COq      
2016 06  04.28656  12 16 00.02   +00 02 33.6   24.1z 17BK232   T09  C~8COq      
2016 06  04.30544  12 15 59.96   +00 02 33.4   24.1z 17BK232   T09  C~8COq      
2016 06  04.32707  12 15 59.95   +00 02 33.4   24.6z 17BK232   T09  C~8COq      
2016 06  04.33517  12 15 59.96   +00 02 33.4   24.3z 17BK232   T09  C~8COq      
2016 06  05.339160 12 15 58.85   +00 02 33.7         17BK232   T09  C~83Eq      
2017 01  23.61293  12 27 36.09   -01 29 28.6   24.6i 17BK232   T09  C~7xTo      
2017 01  23.61560  12 27 36.08   -01 29 28.6   24.4i 17BK232   T09  C~7xTo      
2017 01  23.61828  12 27 36.08   -01 29 28.6   24.4i 17BK232   T09  C~7xTo      
2017 01  23.62095  12 27 36.06   -01 29 28.6   24.7i 17BK232   T09  C~7xTp      
2017 01  28.59194  12 27 27.13   -01 28 43.6   24.3z 17BK232   T09  C~7xTp      
2017 01  28.60879  12 27 27.09   -01 28 43.3   24.2z 17BK232   T09  C~7xTp      
2017 01  28.61418  12 27 27.08   -01 28 43.1   24.9z 17BK232   T09  C~7xTp      
2017 02  23.521659 12 26 11.34   -01 21 50.2         17BK232   T09  C~83Eq      
2017 02  23.595374 12 26 11.05   -01 21 48.7         17BK232   T09  C~83Eq      

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     0.13       0.00    -0.04
     2   0.0003     -9.04     0.16      -0.64    -0.06
     3   0.0054   -139.42    -0.16      -8.59     0.12
     4   0.0054   -140.60    -0.21      -8.88    -0.10
     5   0.0055   -142.22     0.02      -8.93    -0.01
     6   0.0055   -144.01     0.07      -8.94     0.10
     7   0.1721  -3116.55    -0.10    -346.86    -0.02
     8   0.1722  -3116.75     0.02    -347.16    -0.20
     9   0.1722  -3116.91     0.13    -346.80     0.28
    10   0.1723  -3117.65    -0.29    -347.34    -0.13
    11   0.1723  -3117.79    -0.06    -347.40    -0.05
    12   0.1723  -3117.65     0.21    -347.34     0.06
    13   0.1751  -3133.06     0.09    -353.66     0.00
    14   0.8110   8662.21     0.05   -1278.76     0.15
    15   0.8110   8662.07    -0.02   -1278.82     0.10
    16   0.8110   8662.07     0.05   -1278.82     0.11
    17   0.8110   8661.79    -0.15   -1278.94    -0.01
    18   0.8246   8520.77     0.10   -1290.65    -0.10
    19   0.8247   8520.10    -0.02   -1290.61    -0.02
    20   0.8247   8519.88    -0.06   -1290.49     0.12
    21   0.8956   7311.68     0.08   -1361.15    -0.11
    22   0.8958   7307.09    -0.05   -1361.50    -0.19

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.

17BK232    quality flag:2

Type:       SCATEXTD  SCATNEAR  SCATEXTD

axisobj        46.289    47.177    46.048
ecceobj         0.117     0.190     0.079
incobj         17.953    17.966    17.946
qmin           40.220    37.710    41.646
qmax           53.133    57.713    51.135
amean          46.532    47.447    46.275
amin           46.137    47.015    45.914
amax           46.954    47.998    46.661
emean           0.119     0.182     0.085
emin            0.107     0.163     0.073
emax            0.132     0.202     0.096
imean          18.030    18.149    17.981
imin           17.710    17.629    17.719
imax           18.351    18.736    18.261
excite_mean     0.332     0.361     0.320
fracstop        1.000     1.000     1.000
cjmean          2.994     2.980     3.000

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       187.1     182.3     184.1
kozaiamp        179.8     180.0     180.0