Orbit Fit and Astrometric record for 17HQ108

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: 17HQ108   
# Created Wed May  8 01:18:09 2024
# Orbit generated from Bernstein formalism
# Fitting     21 observations of     21
# Arc:  82.83d
# First observation: 2017/02/02
#  Last observation: 2017/04/26
Preliminary a, adot, b, bdot, g, gdot:
  -0.000018   0.051433   0.000042  -0.002724   0.032405   0.000000
# Chi-squared of fit:     8.16 DOF:     36 RMS:  0.11
# Min/Max residuals:    -0.21    0.22
# Exact a, adot, b, bdot, g, gdot:
  2.108185E-05  4.059043E-02 -4.428645E-08 -1.975147E-03  3.069310E-02 -7.245832E-03
# Covariance matrix:
  3.5820E-13 -1.2241E-12 -2.6915E-16 -1.1355E-14  6.1485E-13  1.0520E-10
 -1.2241E-12  5.4729E-09  2.1113E-11 -3.8106E-10  7.2668E-10 -5.4655E-08
 -2.6915E-16  2.1113E-11  3.3462E-13 -2.7881E-12  2.8046E-12 -2.1184E-10
 -1.1355E-14 -3.8106E-10 -2.7881E-12  3.6067E-11 -5.0713E-11  3.8071E-09
  6.1485E-13  7.2668E-10  2.8046E-12 -5.0713E-11  1.0011E-10 -6.6615E-09
  1.0520E-10 -5.4655E-08 -2.1184E-10  3.8071E-09 -6.6615E-09  6.5383E-07
#      lat0       lon0       xBary       yBary       zBary        JD0
   -9.368082  153.891264    0.346814   -0.150140   -0.911098  2457787.007031
# Heliocentric elements and errors
Epoch:              2457780.5000  =  2017/01/27
Mean Anomaly:          352.73923 +/-     0.598
Argument of Peri:      282.98318 +/-     2.479
Long of Asc Node:      260.75468 +/-     0.029
Inclination:             9.54199 +/-     0.002
Eccentricity:         0.56190736 +/-    0.0178
Semi-Major Axis:     72.72048105 +/-    2.2608
Time of Perihelion: 2462348.8938 +/-     310.2
Perihelion:          31.85830724 +/-    1.6277
Aphelion:           113.58265485 +/-    3.7600
Period (y)              620.1451 +/-     28.92
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -29.54605114 +/-    0.0094
Ecliptic Y           14.85973751 +/-    0.0046
Ecliptic Z           -5.30336859 +/-    0.0017
Ecliptic XDOT        -0.00099206 +/-    0.0001
Ecliptic YDOT        -0.00355120 +/-    0.0000
Ecliptic ZDOT        -0.00006869 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   33.49487506 +/-    0.0086
Geocenter to KBO     32.58061323 +/-    0.0106
# Hcoef:  8.27

The following table shows the complete astrometric record for 17HQ108. 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 (17HQ108) followed by the observatory code and reference code for the source of the astrometry.

2017 02  02.50623  10 09 36.68   +01 20 21.5   23.5r 17HQ108   T09  C~7xUY      
2017 02  02.51587  10 09 36.63   +01 20 22.1   23.4r 17HQ108   T09  C~7xUY      
2017 02  02.52702  10 09 36.59   +01 20 22.1   23.4r 17HQ108   T09  C~7xUY      
2017 02  02.59348  10 09 36.23   +01 20 23.6   23.1i 17HQ108   T09  C~7xUY      
2017 03  04.32155  10 06 55.62   +01 34 11.0   23.0z 17HQ108   T09  C~7xUY      
2017 03  04.34714  10 06 55.47   +01 34 11.9   23.0z 17HQ108   T09  C~7xUY      
2017 03  04.50300  10 06 54.62   +01 34 16.8   23.2i 17HQ108   T09  C~7xUY      
2017 03  22.39453  10 05 26.90   +01 44 03.4   23.1z 17HQ108   T09  C~7xUY      
2017 03  22.42021  10 05 26.79   +01 44 04.1   23.0z 17HQ108   T09  C~7xUY      
2017 03  22.44588  10 05 26.66   +01 44 05.1   22.9z 17HQ108   T09  C~7xUY      
2017 03  22.47157  10 05 26.55   +01 44 05.9   22.9z 17HQ108   T09  C~7xUY      
2017 03  22.49332  10 05 26.46   +01 44 06.4   23.0z 17HQ108   T09  C~7xUY      
2017 04  26.23645  10 03 42.82   +02 00 44.2   23.7i 17HQ108   T09  C~7xUY      
2017 04  26.24028  10 03 42.82   +02 00 44.4   23.7i 17HQ108   T09  C~7xUY      
2017 04  26.24413  10 03 42.81   +02 00 44.7   23.6i 17HQ108   T09  C~7xUY      
2017 04  26.26326  10 03 42.79   +02 00 44.9   23.8i 17HQ108   T09  C~7xUY      
2017 04  26.29400  10 03 42.75   +02 00 45.4   23.6i 17HQ108   T09  C~7xUY      
2017 04  26.29783  10 03 42.74   +02 00 45.6   23.5i 17HQ108   T09  C~7xUY      
2017 04  26.32635  10 03 42.71   +02 00 46.1   24.4g 17HQ108   T09  C~7xUY      
2017 04  26.33018  10 03 42.70   +02 00 46.4   24.3g 17HQ108   T09  C~7xUY      
2017 04  26.33400  10 03 42.70   +02 00 46.4   24.3g 17HQ108   T09  C~7xUZ      

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    -0.04       0.00    -0.20
     2   0.0000     -0.91    -0.16       0.29     0.17
     3   0.0001     -1.47     0.19       0.08     0.05
     4   0.0002     -7.05     0.05      -0.45     0.05
     5   0.0816  -2552.22     0.10     -87.77     0.04
     6   0.0817  -2554.64    -0.09     -87.74     0.04
     7   0.0821  -2568.30    -0.20     -87.71    -0.11
     8   0.1311  -4006.66     0.01      -9.18     0.05
     9   0.1312  -4008.46     0.14      -9.11    -0.05
    10   0.1313  -4010.63    -0.11      -8.87     0.02
    11   0.1313  -4012.46    -0.02      -8.71     0.02
    12   0.1314  -4013.90     0.17      -8.73    -0.14
    13   0.2265  -5822.42    -0.11     369.32    -0.09
    14   0.2265  -5822.49    -0.07     369.50     0.05
    15   0.2265  -5822.74    -0.21     369.73     0.22
    16   0.2266  -5823.09    -0.03     369.81     0.05
    17   0.2267  -5823.83     0.08     370.06    -0.11
    18   0.2267  -5824.04    -0.02     370.20    -0.03
    19   0.2267  -5824.64     0.17     370.50    -0.11
    20   0.2268  -5824.89     0.03     370.73     0.07
    21   0.2268  -5824.89     0.13     370.73     0.02

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.

17HQ108    quality flag:1

Type:     11:3EEEEEE  CENTAURS  SCATNEAR

axisobj        71.596    76.598    68.290
ecceobj         0.554     0.593     0.524
incobj          9.525     9.522     9.528
qmin           31.097    29.932    31.890
qmax          114.701   159.219   107.653
amean          71.595    80.293    68.083
amin           70.460    66.200    65.720
amax           73.260    95.450    70.303
emean           0.555     0.608     0.510
emin            0.546     0.530     0.478
emax            0.566     0.668     0.535
imean          10.754    11.563    13.067
imin           10.351     9.365    10.954
imax           11.102    14.594    14.918
excite_mean     0.586     0.640     0.559
fracstop        1.000     1.000     1.000
cjmean          2.939     2.910     2.961

libcent 0       181.1    -180.0    -180.0
libamp  0        95.6    -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       148.9     186.1     174.2
kozaiamp        180.0     180.0     180.0