Orbit Fit and Astrometric record for 17CH56

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: 17CH56    
# Created Wed Mar 26 01:11:06 2025
# Orbit generated from Bernstein formalism
# Fitting     21 observations of     21
# Arc:   1.87y
# First observation: 2015/03/22
#  Last observation: 2017/02/01
Preliminary a, adot, b, bdot, g, gdot:
   0.000043   0.021933   0.000001   0.003038   0.022761   0.000000
# Chi-squared of fit:     6.58 DOF:     36 RMS:  0.10
# Min/Max residuals:    -0.26    0.21
# Exact a, adot, b, bdot, g, gdot:
  1.384451E-05  2.151237E-02  2.109457E-06  3.051885E-03  2.376194E-02  2.156859E-03
# Covariance matrix:
  1.8328E-13 -2.0229E-13  3.4558E-16 -1.3285E-14 -9.2071E-14 -2.4328E-12
 -2.0229E-13  4.3705E-12 -6.0805E-15  4.3406E-13  1.1369E-12  7.5988E-11
  3.4558E-16 -6.0805E-15  1.7656E-13 -1.0169E-13 -4.6422E-15 -1.3741E-13
 -1.3285E-14  4.3406E-13 -1.0169E-13  1.4213E-13  1.6039E-13  8.1519E-12
 -9.2071E-14  1.1369E-12 -4.6422E-15  1.6039E-13  1.2803E-12  2.9689E-11
 -2.4328E-12  7.5988E-11 -1.3741E-13  8.1519E-12  2.9689E-11  1.4427E-09
#      lat0       lon0       xBary       yBary       zBary        JD0
  -13.931483  141.762905   -0.631453   -0.184462   -0.744173  2457103.877264
# Heliocentric elements and errors
Epoch:              2457100.5000  =  2015/03/19
Mean Anomaly:          118.51255 +/-     0.474
Argument of Peri:      169.25244 +/-     0.445
Long of Asc Node:      201.14382 +/-     0.003
Inclination:            15.93343 +/-     0.000
Eccentricity:         0.13791597 +/-    0.0012
Semi-Major Axis:     39.69590672 +/-    0.0146
Time of Perihelion: 2427027.3552 +/-     119.2
Perihelion:          34.22120730 +/-    0.0483
Aphelion:            45.17060613 +/-    0.0495
Period (y)              250.1075 +/-      0.14
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -33.07942859 +/-    0.0015
Ecliptic Y           25.25890623 +/-    0.0012
Ecliptic Z          -10.13213094 +/-    0.0005
Ecliptic XDOT        -0.00179342 +/-    0.0000
Ecliptic YDOT        -0.00175099 +/-    0.0000
Ecliptic ZDOT         0.00028155 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   42.83597807 +/-    0.0014
Geocenter to KBO     42.08411233 +/-    0.0020
# Hcoef:  8.37

The following table shows the complete astrometric record for 17CH56. 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 (17CH56) followed by the observatory code and reference code for the source of the astrometry.

2015 03  22.376486 09 18 43.91   +01 02 04.3         17CH56    T09  C~86ur      
2015 03  22.38922  09 18 43.86   +01 02 04.8   24.7i 17CH56    T09  C~8ifR      
2015 03  22.39754  09 18 43.84   +01 02 05.0   24.8i 17CH56    T09  C~8ifR      
2015 03  22.40303  09 18 43.83   +01 02 05.2   24.9i 17CH56    T09  C~8ifR      
2015 03  22.41404  09 18 43.78   +01 02 05.5   25.4i 17CH56    T09  C~8ifR      
2015 03  22.42499  09 18 43.75   +01 02 05.8   24.6i 17CH56    T09  C~8ifR      
2015 03  22.43327  09 18 43.71   +01 02 06.2   24.8i 17CH56    T09  C~8ifR      
2015 03  22.453542 09 18 43.66   +01 02 06.6         17CH56    T09  C~86ur      
2016 01  12.369773 09 28 31.61   +00 20 59.8         17CH56    T09  C~86ur      
2016 11  28.55912  09 35 10.51   +00 09 40.1   24.8r 17CH56    T09  C~81Br      
2016 11  28.58230  09 35 10.51   +00 09 39.7   24.5r 17CH56    T09  C~81Br      
2016 11  28.58442  09 35 10.50   +00 09 39.7   24.9r 17CH56    T09  C~81Br      
2016 11  28.62032  09 35 10.49   +00 09 39.1   25.2r 17CH56    T09  C~81Br      
2016 12  23.43184  09 34 27.93   +00 06 20.5   24.0z 17CH56    T09  C~81Br      
2016 12  23.43719  09 34 27.91   +00 06 20.3   24.7z 17CH56    T09  C~81Br      
2016 12  23.44791  09 34 27.87   +00 06 20.5   24.3z 17CH56    T09  C~81Br      
2017 02  01.48410  09 31 54.59   +00 13 19.2   24.2i 17CH56    T09  C~81Br      
2017 02  01.50616  09 31 54.48   +00 13 19.7   23.8i 17CH56    T09  C~81Br      
2017 02  01.52538  09 31 54.39   +00 13 19.9   24.0i 17CH56    T09  C~81Br      
2017 02  01.53367  09 31 54.35   +00 13 20.2   24.0i 17CH56    T09  C~81Br      
2017 02  01.54729  09 31 54.30   +00 13 20.6   24.1i 17CH56    T09  C~81Br      

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     0.10       0.00    -0.02
     2   0.0000     -0.87    -0.07       0.24     0.05
     3   0.0001     -1.22     0.04       0.34     0.02
     4   0.0001     -1.42     0.14       0.48     0.09
     5   0.0001     -2.23    -0.06       0.53    -0.01
     6   0.0001     -2.75     0.02       0.68    -0.02
     7   0.0002     -3.44    -0.22       0.87     0.05
     8   0.0002     -4.28     0.05       1.01    -0.09
     9   0.8104   9149.38    -0.00     416.46    -0.10
    10   1.6898  15065.78    -0.16    1647.42     0.01
    11   1.6898  15065.90     0.09    1647.04     0.04
    12   1.6898  15065.76    -0.04    1646.99     0.03
    13   1.6899  15065.80     0.21    1646.37     0.04
    14   1.7579  14518.80     0.04    1256.68    -0.05
    15   1.7579  14518.58     0.03    1256.40    -0.26
    16   1.7579  14517.94    -0.18    1256.40    -0.11
    17   1.8675  12193.45     0.07     933.05     0.10
    18   1.8676  12191.72    -0.06     933.01     0.10
    19   1.8676  12190.37    -0.01     932.78    -0.09
    20   1.8676  12189.70    -0.07     932.88     0.02
    21   1.8677  12188.86     0.08     933.02     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.

17CH56    quality flag:3

Type:           3:2E      3:2E      3:2E

axisobj        39.573    39.618    39.529
ecceobj         0.144     0.147     0.142
incobj         15.957    15.957    15.958
qmin           32.831    29.883    32.886
qmax           46.735    49.863    46.522
amean          39.457    39.457    39.457
amin           38.955    38.852    38.960
amax           40.004    40.129    39.989
emean           0.139     0.164     0.142
emin            0.111     0.065     0.118
emax            0.170     0.245     0.165
imean          16.526    15.557    16.325
imin           15.685    13.231    15.564
imax           17.363    18.382    17.114
excite_mean     0.317     0.317     0.315
fracstop        1.000     1.000     1.000
cjmean          2.937     2.936     2.938

libcent 0       179.6     184.0     179.2
libamp  0       128.9     169.4     122.4
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       173.4     241.5     178.7
kozaiamp        180.0     180.0     180.0