Orbit Fit and Astrometric record for 17BN233

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: 17BN233   
# Created Wed Jul 17 01:11:28 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     20 observations of     20
# Arc:   5.96y
# First observation: 2015/02/17
#  Last observation: 2021/02/01
# Chi-squared of fit:     6.91 DOF:     34 RMS:  0.10
# Min/Max residuals:    -0.18    0.26
# Exact a, adot, b, bdot, g, gdot:
  1.733883E-05  2.810867E-02 -1.785397E-06 -1.066123E-03  2.616515E-02 -3.714426E-03
# Covariance matrix:
  9.8899E-13 -6.9581E-13 -2.4486E-14  2.1143E-14 -1.5469E-13 -3.0239E-12
 -6.9581E-13  5.5850E-13  2.2675E-14 -1.8251E-14  4.6021E-14  2.5905E-12
 -2.4486E-14  2.2675E-14  3.0354E-13 -1.1988E-13 -8.7534E-15  1.1643E-13
  2.1143E-14 -1.8251E-14 -1.1988E-13  6.2325E-14 -1.4314E-15 -9.5117E-14
 -1.5469E-13  4.6021E-14 -8.7534E-15 -1.4314E-15  6.0287E-13  3.3876E-13
 -3.0239E-12  2.5905E-12  1.1643E-13 -9.5117E-14  3.3876E-13  1.3523E-11
#      lat0       lon0       xBary       yBary       zBary        JD0
  -11.798290  145.080245   -0.046324   -0.201026   -0.963344  2457070.559507
# Heliocentric elements and errors
Epoch:              2457070.5000  =  2015/02/17
Mean Anomaly:          330.78746 +/-     0.024
Argument of Peri:      304.36129 +/-     0.041
Long of Asc Node:      245.63209 +/-     0.002
Inclination:            11.69321 +/-     0.000
Eccentricity:         0.21456827 +/-    0.0001
Semi-Major Axis:     47.34907764 +/-    0.0074
Time of Perihelion: 2466727.2851 +/-      27.0
Perihelion:          37.18946818 +/-    0.0078
Aphelion:            57.50868710 +/-    0.0104
Period (y)              325.8183 +/-      0.08
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -31.51241922 +/-    0.0009
Ecliptic Y           21.94071451 +/-    0.0006
Ecliptic Z           -7.81458963 +/-    0.0002
Ecliptic XDOT        -0.00135663 +/-    0.0000
Ecliptic YDOT        -0.00264807 +/-    0.0000
Ecliptic ZDOT        -0.00002964 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   39.18548175 +/-    0.0008
Geocenter to KBO     38.21888271 +/-    0.0011
# Hcoef:  7.42

The following table shows the complete astrometric record for 17BN233. 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 (17BN233) followed by the observatory code and reference code for the source of the astrometry.

2015 02  17.058729 09 33 43.26   +02 01 21.4         17BN233   W84  C~81Bn      
2016 01  14.292950 09 42 26.53   +01 15 31.1         17BN233   W84  C~81Bn      
2016 03  02.159153 09 38 39.52   +01 32 26.3         17BN233   W84  C~81Bn      
2016 03  02.160939 09 38 39.49   +01 32 26.3         17BN233   W84  C~81Bn      
2016 12  25.468651 09 49 35.73   +00 38 52.2         17BN233   T09  C~81Bn      
2016 12  25.497963 09 49 35.65   +00 38 52.2         17BN233   T09  C~81Bn      
2017 01  26.46395  09 47 33.77   +00 42 54.0   22.9z 17BN233   T09  C~7zpa      
2017 01  26.47200  09 47 33.74   +00 42 54.1   23.1z 17BN233   T09  C~7zpa      
2017 01  26.47736  09 47 33.70   +00 42 54.1   23.0z 17BN233   T09  C~7zpa      
2017 01  26.48805  09 47 33.66   +00 42 54.3   23.0z 17BN233   T09  C~7zpa      
2017 01  26.49611  09 47 33.61   +00 42 54.3   22.9z 17BN233   T09  C~7zpa      
2017 01  26.50415  09 47 33.57   +00 42 54.6   23.1z 17BN233   T09  C~7zpa      
2017 01  28.43605  09 47 24.54   +00 43 28.1   23.5g 17BN233   T09  C~7zpa      
2017 01  28.47391  09 47 24.36   +00 43 28.7   24.2g 17BN233   T09  C~7zpa      
2017 01  28.47880  09 47 24.33   +00 43 28.9   24.5g 17BN233   T09  C~7zpa      
2017 03  06.36925  09 44 25.87   +00 58 50.9   23.1i 17BN233   T09  C~7zpa      
2017 03  06.38040  09 44 25.83   +00 58 51.2   23.0i 17BN233   T09  C~7zpa      
2017 03  06.38871  09 44 25.78   +00 58 51.4   22.9i 17BN233   T09  C~7zpa      
2017 03  06.41085  09 44 25.69   +00 58 52.1   23.0i 17BN233   T09  C~7zpa      
2021 02  01.253988 10 11 46.04   -01 39 56.1         17BN233   W84  C~81Bn      

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     0.01       0.00     0.25
     2   0.9069      0.00    -0.12       0.00    -0.02
     3   1.0379      0.00     0.26       0.00    -0.06
     4   1.0379      0.00    -0.07       0.00    -0.11
     5   1.8546      0.00     0.14       0.00    -0.12
     6   1.8547      0.00     0.17       0.00    -0.05
     7   1.9422      0.00    -0.04       0.00     0.09
     8   1.9423      0.00     0.08       0.00     0.05
     9   1.9423      0.00    -0.13       0.00    -0.04
    10   1.9423      0.00     0.03       0.00    -0.02
    11   1.9423      0.00    -0.15       0.00    -0.15
    12   1.9424      0.00    -0.18       0.00     0.01
    13   1.9476      0.00    -0.01       0.00     0.09
    14   1.9477      0.00     0.01       0.00     0.02
    15   1.9478      0.00    -0.08       0.00     0.13
    16   2.0488      0.00    -0.10       0.00     0.02
    17   2.0488      0.00     0.07       0.00    -0.02
    18   2.0488      0.00    -0.10       0.00    -0.06
    19   2.0489      0.00     0.08       0.00    -0.02
    20   5.9581      0.00     0.04       0.00     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.

17BN233    quality flag:3

Type:       SCATNEAR  SCATNEAR  SCATNEAR

axisobj        46.980    46.980    46.981
ecceobj         0.207     0.207     0.207
incobj         11.678    11.678    11.678
qmin           36.538    36.543    36.593
qmax           58.093    57.999    58.088
amean          47.029    47.028    47.030
amin           46.610    46.594    46.606
amax           47.555    47.561    47.551
emean           0.205     0.205     0.205
emin            0.191     0.191     0.190
emax            0.222     0.220     0.222
imean          13.204    13.204    13.204
imin           12.491    12.493    12.497
imax           13.813    13.815    13.813
excite_mean     0.307     0.307     0.307
fracstop        1.000     1.000     1.000
cjmean          3.022     3.022     3.022

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       176.1     176.1     176.1
kozaiamp        180.0     180.0     180.0