Orbit Fit and Astrometric record for 15GD58

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: 15GD58    
# Created Wed May  8 01:17:05 2024
# Orbit generated from Bernstein formalism
# Fitting     34 observations of     34
# Arc:   2.34y
# First observation: 2015/02/17
#  Last observation: 2017/06/22
Preliminary a, adot, b, bdot, g, gdot:
  -0.000101   0.024102   0.000005  -0.000602   0.024204   0.000000
# Chi-squared of fit:     4.65 DOF:     62 RMS:  0.07
# Min/Max residuals:    -0.16    0.14
# Exact a, adot, b, bdot, g, gdot:
  1.545595E-05  2.401605E-02 -2.257310E-07 -5.989761E-04  2.425230E-02 -1.220641E-03
# Covariance matrix:
  1.6874E-13  5.3601E-15 -8.4455E-16 -1.9960E-15  1.3685E-13  2.6914E-12
  5.3601E-15  2.9910E-13  6.8167E-17 -7.8053E-15  1.9192E-13  8.2236E-12
 -8.4455E-16  6.8167E-17  8.8715E-14 -7.1730E-14 -9.7377E-16  1.5624E-14
 -1.9960E-15 -7.8053E-15 -7.1730E-14  1.1250E-13 -6.5517E-15 -3.6100E-13
  1.3685E-13  1.9192E-13 -9.7377E-16 -6.5517E-15  2.6608E-13  7.6066E-12
  2.6914E-12  8.2236E-12  1.5624E-14 -3.6100E-13  7.6066E-12  3.7183E-10
#      lat0       lon0       xBary       yBary       zBary        JD0
    2.996339 -157.207836    0.802004    0.030058   -0.571567  2457071.081158
# Heliocentric elements and errors
Epoch:              2457070.5000  =  2015/02/17
Mean Anomaly:          307.28195 +/-     0.219
Argument of Peri:      175.54875 +/-     0.303
Long of Asc Node:       86.67732 +/-     0.013
Inclination:             3.25975 +/-     0.000
Eccentricity:         0.08113418 +/-    0.0007
Semi-Major Axis:     43.77011383 +/-    0.0057
Time of Perihelion: 2472559.4436 +/-      64.2
Perihelion:          40.21886150 +/-    0.0319
Aphelion:            47.32136617 +/-    0.0320
Period (y)              289.5841 +/-      0.06
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -38.80271747 +/-    0.0008
Ecliptic Y          -15.43380752 +/-    0.0003
Ecliptic Z            2.15534106 +/-    0.0000
Ecliptic XDOT         0.00117024 +/-    0.0000
Ecliptic YDOT        -0.00245311 +/-    0.0000
Ecliptic ZDOT        -0.00007464 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   41.81505462 +/-    0.0008
Geocenter to KBO     41.23320626 +/-    0.0009
# Hcoef:  7.70

The following table shows the complete astrometric record for 15GD58. 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 (15GD58) followed by the observatory code and reference code for the source of the astrometry.

2015 02  17.58038  13 28 48.218  -06 04 49.72  23.9r 15GD58    568  C~2nvY      
2015 02  17.62132  13 28 48.123  -06 04 49.00  23.8r 15GD58    568  C~2nvY      
2015 02  20.61441  13 28 41.250  -06 03 57.64  23.8r 15GD58    568  C~2nvY      
2015 03  18.55881  13 27 16.308  -05 54 23.90  23.7r 15GD58    568  C~2nvY      
2015 03  18.59998  13 27 16.143  -05 54 22.88  23.7r 15GD58    568  C~2nvY      
2015 03  20.56294  13 27 08.223  -05 53 32.54  23.7r 15GD58    568  C~2nvY      
2015 04  11.49722  13 25 32.234  -05 43 45.37  24.0r 15GD58    568  C~2nvY      
2015 04  13.36151  13 25 23.765  -05 42 55.20  23.8r 15GD58    568  C~2nvY      
2015 04  13.40245  13 25 23.579  -05 42 54.10  24.0r 15GD58    568  C~2nvY      
2015 04  13.48799  13 25 23.176  -05 42 52.04  23.8r 15GD58    568  C~2nvY      
2015 04  13.50003  13 25 23.120  -05 42 51.53  23.7r 15GD58    568  C~2nvY      
2015 04  13.50498  13 25 23.099  -05 42 51.41  23.8r 15GD58    568  C~2nvY      
2015 04  19.40228  13 24 56.305  -05 40 15.40  23.5r 15GD58    568  C~2nvY      
2015 04  19.51922  13 24 55.759  -05 40 12.33  23.9r 15GD58    568  C~2nvY      
2015 05  18.27664  13 22 56.228  -05 29 16.14  24.0r 15GD58    568  C~2nvY      
2015 05  18.32493  13 22 56.048  -05 29 15.18  23.9r 15GD58    568  C~2nvY      
2015 06  20.27498  13 21 33.075  -05 23 09.35  23.8r 15GD58    568  C~2nvY      
2015 06  20.31583  13 21 33.013  -05 23 09.29  24.0r 15GD58    568  C~2nvY      
2015 07  14.27191  13 21 26.618  -05 24 27.80  24.1r 15GD58    568  C~2nvY      
2015 07  20.26475  13 21 32.809  -05 25 34.75  23.9r 15GD58    568  C~2nvY      
2016 02  04.56329  13 34 15.261  -06 40 01.35  24.1w 15GD58    568  C~2nvY      
2016 02  10.55122  13 34 08.086  -06 38 55.14  24.1w 15GD58    568  C~2nvY      
2016 02  10.60087  13 34 08.003  -06 38 54.58  23.9w 15GD58    568  C~2nvY      
2016 03  11.53218  13 32 49.280  -06 29 37.74  24.0w 15GD58    568  C~2nvY      
2016 04  03.43317  13 31 14.964  -06 19 50.64  24.1w 15GD58    568  C~2nvY      
2016 04  09.41297  13 30 47.964  -06 17 10.12  24.0w 15GD58    568  C~2nvY      
2016 05  02.30717  13 29 05.150  -06 07 25.17  24.1w 15GD58    568  C~2nvZ      
2016 05  06.31695  13 28 48.172  -06 05 52.92  24.3w 15GD58    568  C~2nvZ      
2016 05  28.27195  13 27 27.887  -05 59 02.49  24.1w 15GD58    568  C~2nvZ      
2016 06  04.35340  13 27 07.926  -05 57 31.37  24.1w 15GD58    568  C~2nvZ      
2016 06  27.27271  13 26 29.146  -05 55 23.21  24.5w 15GD58    568  C~2nvZ      
2016 07  06.30847  13 26 25.793  -05 55 47.43  24.4w 15GD58    568  C~2nvZ      
2017 02  24.63168  13 38 46.781  -07 07 24.22        15GD58    568  C~2nvZ      
2017 06  22.27110  13 31 40.381  -06 27 52.46  24.1w 15GD58    568  C~2nvZ      

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    -0.03
     2   0.0001     -1.58    -0.01       0.15    -0.01
     3   0.0083   -115.81     0.03      10.08    -0.02
     4   0.0793  -1505.32    -0.05      75.53     0.01
     5   0.0795  -1507.98    -0.00      75.56    -0.00
     6   0.0848  -1636.40    -0.03      78.68    -0.06
     7   0.1449  -3184.64     0.00      94.47    -0.02
     8   0.1500  -3320.67     0.01      94.29     0.12
     9   0.1501  -3323.66     0.06      94.28     0.14
    10   0.1503  -3330.01     0.06      93.97    -0.11
    11   0.1504  -3330.98    -0.02      94.13     0.06
    12   0.1504  -3331.31     0.01      94.13     0.06
    13   0.1665  -3760.71    -0.03      90.95    -0.07
    14   0.1668  -3769.42    -0.14      90.78    -0.10
    15   0.2456  -5671.00     0.06      38.51    -0.02
    16   0.2457  -5673.86    -0.00      38.41     0.04
    17   0.3359  -6961.30     0.07     -82.23     0.09
    18   0.3360  -6962.19     0.01     -82.52    -0.01
    19   0.4016  -7021.73    -0.08    -190.97     0.07
    20   0.4180  -6910.89    -0.02    -218.77    -0.08
    21   0.9637   5311.36     0.00    -171.75     0.00
    22   0.9801   5187.55     0.04    -149.30     0.12
    23   0.9802   5186.20    -0.02    -149.23     0.03
    24   1.0622   3890.00    -0.15     -61.33    -0.16
    25   1.1249   2366.38     0.03     -31.75    -0.03
    26   1.1412   1932.96     0.08     -30.55    -0.02
    27   1.2039    292.07     0.13     -51.38    -0.06
    28   1.2149     22.67    -0.08     -59.00     0.00
    29   1.2750  -1241.86    -0.03    -119.55    -0.05
    30   1.2944  -1552.26    -0.04    -144.89    -0.05
    31   1.3571  -2137.28    -0.02    -239.68     0.14
    32   1.3819  -2174.81     0.09    -280.68    -0.02
    33   2.0207   9681.32     0.03    -224.41     0.07
    34   2.3428   2895.94    -0.04    -340.57    -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.

15GD58    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        43.358    43.370    43.346
ecceobj         0.078     0.080     0.077
incobj          3.260     3.260     3.260
qmin           39.590    39.425    39.668
qmax           47.892    48.133    47.801
amean          43.635    43.646    43.624
amin           43.289    43.294    43.269
amax           44.008    44.021    43.994
emean           0.071     0.072     0.069
emin            0.045     0.045     0.046
emax            0.089     0.094     0.087
imean           1.415     1.475     1.384
imin            0.477     0.448     0.445
imax            2.253     2.396     2.117
excite_mean     0.076     0.077     0.074
fracstop        1.000     1.000     1.000
cjmean          3.090     3.090     3.090

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       182.1     180.9     181.3
kozaiamp        179.9     180.0     179.9