Orbit Fit and Astrometric record for 17BM231

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: 17BM231   
# Created Fri Nov 22 02:10:48 2024
# Orbit generated from Bernstein formalism
# Fitting     25 observations of     25
# Arc:   3.73y
# First observation: 2015/03/22
#  Last observation: 2018/12/12
Preliminary a, adot, b, bdot, g, gdot:
   0.000353   0.037601   0.000031   0.004425   0.031828   0.000000
# Chi-squared of fit:    12.32 DOF:     44 RMS:  0.12
# Min/Max residuals:    -0.27    0.27
# Exact a, adot, b, bdot, g, gdot:
  1.866963E-05  3.760080E-02  2.242009E-06  4.444422E-03  3.209634E-02  1.296071E-04
# Covariance matrix:
  4.5180E-13 -3.5751E-13  1.6584E-14 -2.2919E-14 -5.3792E-14 -1.3887E-12
 -3.5751E-13  4.3954E-13 -2.5833E-14  3.2974E-14 -5.5229E-14  1.9373E-12
  1.6584E-14 -2.5833E-14  2.9895E-13 -1.4095E-13  5.3969E-16 -1.4746E-13
 -2.2919E-14  3.2974E-14 -1.4095E-13  8.3738E-14  6.5482E-15  2.0538E-13
 -5.3792E-14 -5.5229E-14  5.3969E-16  6.5482E-15  3.6995E-13  5.5871E-13
 -1.3887E-12  1.9373E-12 -1.4746E-13  2.0538E-13  5.5871E-13  1.2478E-11
#      lat0       lon0       xBary       yBary       zBary        JD0
  -13.618664  142.431917   -0.622482   -0.182116   -0.752266  2457103.879016
# Heliocentric elements and errors
Epoch:              2457100.5000  =  2015/03/19
Mean Anomaly:            8.74443 +/-     0.033
Argument of Peri:      285.76445 +/-     0.044
Long of Asc Node:      205.50390 +/-     0.001
Inclination:            14.98497 +/-     0.000
Eccentricity:         0.13176391 +/-    0.0001
Semi-Major Axis:     36.67565292 +/-    0.0039
Time of Perihelion: 2455129.9191 +/-       7.5
Perihelion:          31.84312535 +/-    0.0046
Aphelion:            41.50818050 +/-    0.0054
Period (y)              222.1135 +/-      0.04
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -24.99752329 +/-    0.0005
Ecliptic Y           18.44043702 +/-    0.0003
Ecliptic Z           -7.33591866 +/-    0.0001
Ecliptic XDOT        -0.00203821 +/-    0.0000
Ecliptic YDOT        -0.00248709 +/-    0.0000
Ecliptic ZDOT         0.00036594 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   31.91773160 +/-    0.0004
Geocenter to KBO     31.15620111 +/-    0.0006
# Hcoef:  9.35

The following table shows the complete astrometric record for 17BM231. 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 (17BM231) followed by the observatory code and reference code for the source of the astrometry.

2015 03  22.378238 09 21 35.57   +01 07 39.2         17BM231   T09  C~81Bn      
2015 03  22.379982 09 21 35.56   +01 07 39.3         17BM231   T09  C~81Bn      
2015 03  22.456321 09 21 35.26   +01 07 42.3         17BM231   T09  C~81Bn      
2016 04  04.246919 09 29 18.48   +00 50 12.8         17BM231   T09  C~81Bn      
2016 04  04.253297 09 29 18.46   +00 50 13.1         17BM231   T09  C~81Bn      
2016 12  25.46448  09 46 00.29   -00 22 43.6   24.7r 17BM231   T09  C~7xTm      
2016 12  25.48124  09 46 00.24   -00 22 43.9   24.4r 17BM231   T09  C~7xTm      
2016 12  25.49171  09 46 00.20   -00 22 43.7   24.7r 17BM231   T09  C~7xTm      
2016 12  25.50217  09 46 00.18   -00 22 43.9   24.5r 17BM231   T09  C~7xTm      
2017 01  21.37737  09 44 01.96   -00 18 44.1   24.0z 17BM231   T09  C~7xTm      
2017 01  21.56723  09 44 00.92   -00 18 40.2   23.7z 17BM231   T09  C~7xTm      
2017 01  21.63253  09 44 00.56   -00 18 39.0   23.9z 17BM231   T09  C~7xTm      
2017 01  21.64058  09 44 00.54   -00 18 38.8   23.9z 17BM231   T09  C~7xTm      
2017 01  28.43816  09 43 23.14   -00 16 12.0   26.0g 17BM231   T09  C~7xTm      
2017 01  28.45502  09 43 23.03   -00 16 11.7   25.6g 17BM231   T09  C~7xTm      
2017 01  28.47182  09 43 22.94   -00 16 11.0   25.2g 17BM231   T09  C~7xTm      
2017 01  28.47671  09 43 22.93   -00 16 11.0   26.0g 17BM231   T09  C~7xTm      
2017 03  04.39116  09 40 01.57   +00 02 59.8   23.8i 17BM231   T09  C~7xTm      
2017 03  04.41889  09 40 01.40   +00 03 00.6   24.0i 17BM231   T09  C~7xTm      
2017 03  04.42156  09 40 01.39   +00 03 00.8   24.2i 17BM231   T09  C~7xTm      
2017 03  04.42430  09 40 01.39   +00 03 00.9   24.1i 17BM231   T09  C~7xTm      
2017 03  04.42698  09 40 01.36   +00 03 01.1   24.0i 17BM231   T09  C~7xTm      
2017 03  04.43238  09 40 01.33   +00 03 01.3   24.1i 17BM231   T09  C~7xTm      
2018 12  12.299673 10 03 13.301  -01 12 51.62  23.3r 17BM231   W84  C~8HJz      
2018 12  12.300471 10 03 13.301  -01 12 51.77  23.9g 17BM231   W84  C~8HK0      

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    -0.03       0.00    -0.01
     2   0.0000     -0.17    -0.08       0.05     0.00
     3   0.0002     -5.39     0.07       1.48     0.01
     4   1.0373   6920.67     0.08    1198.91    -0.11
     5   1.0373   6920.29     0.04    1199.10    -0.06
     6   1.7634  22648.68    -0.05    1802.42     0.10
     7   1.7635  22648.06     0.12    1801.90    -0.13
     8   1.7635  22647.42    -0.02    1801.90     0.06
     9   1.7635  22647.19     0.25    1801.61    -0.05
    10   1.8371  20869.25     0.12    1466.14    -0.02
    11   1.8376  20853.05    -0.07    1464.90     0.19
    12   1.8378  20847.49    -0.13    1464.33     0.11
    13   1.8378  20847.14     0.20    1464.42     0.27
    14   1.8564  20262.73    -0.12    1426.02     0.02
    15   1.8565  20261.05    -0.27    1425.78    -0.14
    16   1.8565  20259.54    -0.27    1426.02     0.18
    17   1.8565  20259.39     0.03    1425.97     0.15
    18   1.9521  17003.65     0.09    1562.57     0.10
    19   1.9522  17000.96    -0.06    1562.52    -0.26
    20   1.9522  17000.75    -0.02    1562.67    -0.15
    21   1.9522  17000.72     0.20    1562.76    -0.09
    22   1.9522  17000.23    -0.05    1562.81    -0.07
    23   1.9522  16999.73    -0.05    1562.86    -0.08
    24   3.7260  38655.98    -0.02    3879.40     0.05
    25   3.7260  38656.02     0.04    3879.26    -0.08

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.

17BM231    quality flag:3

Type:           4:3E      4:3E      4:3E

axisobj        36.534    36.547    36.521
ecceobj         0.128     0.128     0.127
incobj         14.990    14.990    14.990
qmin           29.949    29.973    29.994
qmax           43.195    43.374    43.334
amean          36.476    36.476    36.476
amin           36.139    36.138    36.132
amax           36.854    36.854    36.845
emean           0.143     0.143     0.142
emin            0.101     0.102     0.101
emax            0.176     0.179     0.177
imean          15.417    15.410    15.435
imin           14.077    14.034    14.102
imax           16.812    16.785    16.849
excite_mean     0.302     0.302     0.302
fracstop        1.000     1.000     1.000
cjmean          2.925     2.925     2.925

libcent 0       178.9     179.9     179.4
libamp  0        63.0      61.8      65.1
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       181.6     181.7     181.7
kozaiamp        180.0     180.0     180.0