Orbit Fit and Astrometric record for 15AB309

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: 15AB309   
# Created Fri Nov 22 02:10:14 2024
# Orbit generated from Bernstein formalism
# Fitting     21 observations of     21
# Arc:   1.05y
# First observation: 2015/01/14
#  Last observation: 2016/02/02
Preliminary a, adot, b, bdot, g, gdot:
   0.000089   0.037569   0.000011   0.016935   0.034315   0.000000
# Chi-squared of fit:     9.64 DOF:     36 RMS:  0.12
# Min/Max residuals:    -0.28    0.31
# Exact a, adot, b, bdot, g, gdot:
  1.878549E-05  3.754663E-02  8.522035E-06  1.681470E-02  3.303943E-02 -3.875317E-03
# Covariance matrix:
  2.3890E-13  4.3745E-12 -2.5123E-14  2.0204E-12  2.8673E-12  1.2244E-10
  4.3745E-12  2.1520E-10 -1.2051E-12  9.5520E-11  1.3153E-10  5.7853E-09
 -2.5123E-14 -1.2051E-12  1.4569E-13 -6.8304E-13 -7.3274E-13 -3.2410E-11
  2.0204E-12  9.5520E-11 -6.8304E-13  4.2797E-11  5.8679E-11  2.5731E-09
  2.8673E-12  1.3153E-10 -7.3274E-13  5.8679E-11  8.2557E-11  3.5555E-09
  1.2244E-10  5.7853E-09 -3.2410E-11  2.5731E-09  3.5555E-09  1.5585E-07
#      lat0       lon0       xBary       yBary       zBary        JD0
    3.261914   62.343391   -0.764308    0.035229   -0.615156  2457036.830958
# Heliocentric elements and errors
Epoch:              2457030.5000  =  2015/01/08
Mean Anomaly:          346.44194 +/-     1.504
Argument of Peri:       30.15137 +/-     2.583
Long of Asc Node:       56.62836 +/-     0.002
Inclination:            24.18977 +/-     0.006
Eccentricity:         0.23632439 +/-    0.0050
Semi-Major Axis:     39.87049534 +/-    0.1286
Time of Perihelion: 2460493.6470 +/-     383.8
Perihelion:          30.44812489 +/-    0.2215
Aphelion:            49.29286580 +/-    0.2544
Period (y)              251.7594 +/-      1.22
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           13.63187151 +/-    0.0039
Ecliptic Y           27.66687256 +/-    0.0074
Ecliptic Z            1.72242280 +/-    0.0005
Ecliptic XDOT        -0.00294537 +/-    0.0000
Ecliptic YDOT         0.00108467 +/-    0.0000
Ecliptic ZDOT         0.00137294 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   30.89094524 +/-    0.0068
Geocenter to KBO     30.26686444 +/-    0.0083
# Hcoef:  7.12

The following table shows the complete astrometric record for 15AB309. 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 (15AB309) followed by the observatory code and reference code for the source of the astrometry.

2015 01  14.33018  03 58 15.07   +23 49 34.3   22.4w 15AB309   F51  C~77s0      
2015 01  14.343    03 58 15.02   +23 49 34.3   22.5w 15AB309   F51  C~77s0      
2015 01  14.35578  03 58 14.98   +23 49 34.2   22.6w 15AB309   F51  C~77s0      
2015 01  22.3358   03 57 47.90   +23 48 49.6   22.5w 15AB309   F51  C~77s0      
2015 01  22.34976  03 57 47.86   +23 48 49.4   22.3w 15AB309   F51  C~77s0      
2015 01  22.36372  03 57 47.81   +23 48 49.3   22.3w 15AB309   F51  C~77s0      
2015 01  22.3776   03 57 47.78   +23 48 49.4   22.6w 15AB309   F51  C~77s0      
2015 01  24.3182   03 57 42.45   +23 48 41.1   22.5w 15AB309   F51  C~77s0      
2015 01  24.33273  03 57 42.42   +23 48 41.2   22.2w 15AB309   F51  C~77s0      
2015 01  24.34723  03 57 42.39   +23 48 41.4   22.3w 15AB309   F51  C~77s0      
2015 01  24.36175  03 57 42.31   +23 48 41.1   22.4w 15AB309   F51  C~77s0      
2015 12  06.45389  04 10 38.38   +25 18 09.9   22.2w 15AB309   F51  C~77s0      
2015 12  06.46745  04 10 38.31   +25 18 09.5   22.2w 15AB309   F51  C~77s0      
2015 12  06.481    04 10 38.19   +25 18 09.4   21.9w 15AB309   F51  C~77s0      
2015 12  06.49464  04 10 38.08   +25 18 09.4   22.0w 15AB309   F51  C~77s0      
2016 01  03.36585  04 07 37.87   +25 13 21.9   22.1w 15AB309   F51  C~77s0      
2016 01  03.3767   04 07 37.81   +25 13 21.8   22.1w 15AB309   F51  C~77s0      
2016 01  03.3875   04 07 37.74   +25 13 21.6   22.4w 15AB309   F51  C~77s0      
2016 01  03.39831  04 07 37.69   +25 13 21.7   22.0w 15AB309   F51  C~77s0      
2016 02  02.32629  04 05 48.02   +25 09 53.4   22.3w 15AB309   F51  C~77s0      
2016 02  02.35089  04 05 47.98   +25 09 53.2   21.8w 15AB309   F51  C~77s0      

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    -0.17       0.00    -0.10
     2   0.0000     -0.67    -0.13       0.14    -0.01
     3   0.0001     -1.23     0.02       0.15    -0.06
     4   0.0219   -374.17     0.06      31.62     0.10
     5   0.0220   -374.75     0.05      31.54    -0.04
     6   0.0220   -375.44    -0.07      31.58    -0.05
     7   0.0220   -375.82     0.12      31.76     0.09
     8   0.0273   -449.13    -0.03      38.46    -0.17
     9   0.0274   -449.52     0.13      38.64    -0.04
    10   0.0274   -449.88     0.31      38.92     0.19
    11   0.0275   -451.01    -0.28      38.85     0.07
    12   0.8929  10979.60    -0.07    3284.91     0.21
    13   0.8929  10978.59     0.28    3284.68    -0.12
    14   0.8930  10976.97     0.00    3284.88    -0.03
    15   0.8930  10975.50    -0.11    3285.15     0.13
    16   0.9693   8513.69    -0.01    3447.84    -0.06
    17   0.9693   8512.87    -0.01    3447.90    -0.05
    18   0.9694   8511.89    -0.16    3447.87    -0.11
    19   0.9694   8511.24     0.01    3448.10     0.07
    20   1.0513   7007.65     0.02    3521.14     0.04
    21   1.0514   7007.08     0.06    3521.04    -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.

15AB309    quality flag:2

Type:       CENTAURS  CENTAURR  CENTAURS

axisobj        40.114    40.221    40.063
ecceobj         0.238     0.245     0.236
incobj         24.135    24.114    24.149
qmin           29.232    28.850    30.202
qmax           60.795    51.781    49.506
amean          41.303    39.778    39.451
amin           37.841    38.734    38.882
amax           45.802    40.897    40.105
emean           0.248     0.242     0.173
emin            0.165     0.202     0.098
emax            0.331     0.274     0.237
imean          23.552    22.047    24.173
imin           21.773    20.167    22.311
imax           25.209    23.413    25.840
excite_mean     0.472     0.447     0.446
fracstop        1.000     0.251     1.000
cjmean          2.809     2.821     2.818

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       168.4     179.5     138.8
kozaiamp        180.0     179.8     180.0