Orbit Fit and Astrometric record for 17BR236

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: 17BR236   
# Created Thu Oct 31 01:10:31 2024
# Orbit generated from Bernstein formalism
# Fitting     20 observations of     20
# Arc:   1.87y
# First observation: 2015/03/22
#  Last observation: 2017/02/01
Preliminary a, adot, b, bdot, g, gdot:
  -0.000089   0.024321   0.000008  -0.002418   0.024652   0.000000
# Chi-squared of fit:     9.11 DOF:     34 RMS:  0.12
# Min/Max residuals:    -0.27    0.31
# Exact a, adot, b, bdot, g, gdot:
  1.533188E-05  2.415721E-02 -1.378646E-06 -2.402384E-03  2.471843E-02  7.584437E-04
# Covariance matrix:
  7.3203E-13 -1.0829E-12 -9.0470E-15  6.8933E-14 -5.3093E-13 -1.4122E-11
 -1.0829E-12  7.8044E-12  5.1216E-14 -8.0303E-13  1.0100E-11  1.8331E-10
 -9.0470E-15  5.1216E-14  6.1942E-13 -3.5007E-13  2.4187E-14  8.7682E-13
  6.8933E-14 -8.0303E-13 -3.5007E-13  3.0588E-13 -1.1679E-12 -2.0215E-11
 -5.3093E-13  1.0100E-11  2.4187E-14 -1.1679E-12  1.8324E-11  2.8406E-10
 -1.4122E-11  1.8331E-10  8.7682E-13 -2.0215E-11  2.8406E-10  4.7576E-09
#      lat0       lon0       xBary       yBary       zBary        JD0
  -14.373214  143.014889   -0.614689   -0.193548   -0.755815  2457103.887201
# Heliocentric elements and errors
Epoch:              2457100.5000  =  2015/03/19
Mean Anomaly:           71.29180 +/-     0.909
Argument of Peri:      172.73229 +/-     1.264
Long of Asc Node:      255.33291 +/-     0.006
Inclination:            15.10287 +/-     0.000
Eccentricity:         0.04712112 +/-    0.0027
Semi-Major Axis:     41.76498270 +/-    0.0154
Time of Perihelion: 2437577.1679 +/-     248.8
Perihelion:          39.79696990 +/-    0.1132
Aphelion:            43.73299549 +/-    0.1134
Period (y)              269.9148 +/-      0.15
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -32.30065619 +/-    0.0054
Ecliptic Y           23.55488141 +/-    0.0041
Ecliptic Z          -10.04262907 +/-    0.0017
Ecliptic XDOT        -0.00162534 +/-    0.0000
Ecliptic YDOT        -0.00213390 +/-    0.0000
Ecliptic ZDOT        -0.00027853 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   41.21916092 +/-    0.0049
Geocenter to KBO     40.45563956 +/-    0.0070
# Hcoef:  7.72

The following table shows the complete astrometric record for 17BR236. 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 (17BR236) followed by the observatory code and reference code for the source of the astrometry.

2015 03  22.386423 09 22 47.03   +00 13 57.9         17BR236   T09  C~81Bo      
2015 03  22.435986 09 22 46.86   +00 13 59.4         17BR236   T09  C~81Bo      
2016 04  02.333733 09 27 17.13   -00 14 35.9         17BR236   T09  C~81Bo      
2016 04  02.360442 09 27 17.06   -00 14 35.2         17BR236   T09  C~81Bo      
2016 12  25.500066 09 39 01.35   -01 19 51.5         17BR236   T09  C~81Bo      
2017 01  21.36520  09 37 20.86   -01 18 12.3   23.5z 17BR236   T09  C~81Bo      
2017 01  21.37468  09 37 20.83   -01 18 12.3   23.5z 17BR236   T09  C~81Bo      
2017 01  21.38272  09 37 20.79   -01 18 12.1   23.2z 17BR236   T09  C~81Bo      
2017 01  21.39079  09 37 20.76   -01 18 11.9   23.6z 17BR236   T09  C~81Bo      
2017 01  21.39882  09 37 20.74   -01 18 11.9   22.9z 17BR236   T09  C~81Bo      
2017 01  21.40149  09 37 20.71   -01 18 11.6   23.1z 17BR236   T09  C~81Bo      
2017 01  21.40688  09 37 20.69   -01 18 11.8   23.2z 17BR236   T09  C~81Bo      
2017 01  21.62985  09 37 19.70   -01 18 08.9   23.9z 17BR236   T09  C~81Bo      
2017 01  28.38299  09 36 49.07   -01 16 36.1   25.8g 17BR236   T09  C~81Bo      
2017 01  28.39348  09 36 49.03   -01 16 36.0   25.5g 17BR236   T09  C~81Bp      
2017 01  28.41043  09 36 48.92   -01 16 35.6   25.5g 17BR236   T09  C~81Bp      
2017 01  28.45084  09 36 48.75   -01 16 35.0   25.0g 17BR236   T09  C~81Bp      
2017 02  01.50891  09 36 29.74   -01 15 27.3   23.3i 17BR236   T09  C~81Bp      
2017 02  01.58031  09 36 29.40   -01 15 26.0   22.6i 17BR236   T09  C~81Bp      
2017 02  01.58299  09 36 29.40   -01 15 26.0   22.9i 17BR236   T09  C~81Bp      

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    -0.03
     2   0.0001     -2.89    -0.02       0.61     0.01
     3   1.0320   4386.75    -0.01    -337.65     0.06
     4   1.0321   4385.53     0.01    -337.32    -0.00
     5   1.7635  15675.06     0.11    -698.40    -0.02
     6   1.8370  14206.81    -0.27   -1083.02    -0.15
     7   1.8371  14206.38    -0.06   -1083.16    -0.19
     8   1.8371  14205.75    -0.15   -1083.16    -0.11
     9   1.8371  14205.26    -0.09   -1083.11     0.02
    10   1.8371  14204.97     0.17   -1083.21     0.00
    11   1.8371  14204.45    -0.18   -1083.07     0.17
    12   1.8372  14204.22    -0.03   -1083.35    -0.06
    13   1.8378  14189.15     0.09   -1085.31     0.25
    14   1.8563  13721.98     0.16   -1143.05     0.01
    15   1.8563  13721.38     0.31   -1143.15    -0.01
    16   1.8563  13719.68    -0.16   -1143.29    -0.02
    17   1.8564  13717.06     0.15   -1143.53     0.04
    18   1.8675  13423.96    -0.10   -1169.77    -0.02
    19   1.8677  13418.69    -0.08   -1170.15     0.02
    20   1.8678  13418.69     0.12   -1170.15     0.04

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.

17BR236    quality flag:3

Type:       SCATEXTD  SCATEXTD  SCATEXTD

axisobj        41.568    41.608    41.529
ecceobj         0.050     0.046     0.053
incobj         15.083    15.083    15.084
qmin           38.735    38.878    38.519
qmax           44.570    44.503    44.663
amean          41.560    41.616    41.520
amin           41.249    41.288    41.206
amax           41.894    41.960    41.851
emean           0.051     0.049     0.055
emin            0.039     0.035     0.042
emax            0.065     0.062     0.068
imean          16.794    16.791    16.796
imin           16.186    16.170    16.182
imax           17.404    17.394    17.421
excite_mean     0.293     0.293     0.294
fracstop        1.000     1.000     1.000
cjmean          2.971     2.972     2.970

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       183.9     180.7     184.6
kozaiamp        180.0     180.0     180.0