Orbit Fit and Astrometric record for 24YK27

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: 24YK27    
# Created Sat Feb 22 02:11:38 2025
# Orbit generated from Bernstein formalism
# Fitting     24 observations of     24
# Arc:  32.02d
# First observation: 2024/12/05
#  Last observation: 2025/01/06
Preliminary a, adot, b, bdot, g, gdot:
   0.000049   0.619757  -0.000059  -0.174666   0.210715   0.000000
# Chi-squared of fit:    25.14 DOF:     42 RMS:  0.18
# Min/Max residuals:    -0.61    0.72
# Exact a, adot, b, bdot, g, gdot:
  4.416262E-05  5.459658E-01 -1.287133E-05 -1.616100E-01  1.944105E-01  4.821180E-02
# Covariance matrix:
  3.6117E-13  1.2594E-13 -3.5155E-15 -1.6503E-12  2.0228E-12  1.5126E-10
  1.2594E-13  9.0284E-08 -8.1013E-11 -1.4152E-08  1.7162E-08  2.2230E-07
 -3.5155E-15 -8.1013E-11  3.6356E-13  8.6478E-12 -1.5408E-11 -1.9915E-10
 -1.6503E-12 -1.4152E-08  8.6478E-12  2.3050E-09 -2.7097E-09 -3.6871E-08
  2.0228E-12  1.7162E-08 -1.5408E-11 -2.7097E-09  3.2864E-09  4.4756E-08
  1.5126E-10  2.2230E-07 -1.9915E-10 -3.6871E-08  4.4756E-08  8.3092E-07
#      lat0       lon0       xBary       yBary       zBary        JD0
   19.482990  112.868521    0.617488    0.253335   -0.716457  2460650.015880
# Heliocentric elements and errors
Epoch:              2460650.5000  =  2024/12/06
Mean Anomaly:          359.43561 +/-     0.202
Argument of Peri:      130.30794 +/-     0.404
Long of Asc Node:      335.18553 +/-     0.018
Inclination:            22.02992 +/-     0.007
Eccentricity:         0.29323514 +/-    0.0005
Semi-Major Axis:      8.34869633 +/-    0.0046
Time of Perihelion: 2460664.3136 +/-       5.0
Perihelion:           5.90056521 +/-    0.0056
Aphelion:            10.79682744 +/-    0.0075
Period (y)               24.1233 +/-      0.02
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           -1.60516233 +/-    0.0006
Ecliptic Y            5.41297624 +/-    0.0013
Ecliptic Z            1.71546438 +/-    0.0005
Ecliptic XDOT        -0.00763519 +/-    0.0000
Ecliptic YDOT        -0.00169480 +/-    0.0000
Ecliptic ZDOT        -0.00191904 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO    5.90081994 +/-    0.0012
Geocenter to KBO      5.14375468 +/-    0.0015
# Hcoef: 14.78

The following table shows the complete astrometric record for 24YK27. 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 (24YK27) followed by the observatory code and reference code for the source of the astrometry.

2024 12  05.515079 07 55 30.551  +40 39 25.48  22.0G 24YK27    F51  C~8cUC      
2024 12  05.526486 07 55 30.319  +40 39 26.71  22.0G 24YK27    F51  C~8cUC      
2024 12  05.537891 07 55 30.087  +40 39 27.83  22.6G 24YK27    F51  C~8cUC      
2024 12  05.549405 07 55 29.854  +40 39 29.03  22.6G 24YK27    F51  C~8cUC      
2024 12  20.534281 07 49 16.340  +41 01 20.93  21.2G 24YK27    F52  C~8cUC      
2024 12  20.546565 07 49 15.958  +41 01 20.96  21.9G 24YK27    F52  C~8cUC      
2024 12  20.558729 07 49 15.529  +41 01 22.05  21.3G 24YK27    F52  C~8cUC      
2024 12  26.412168 07 46 11.480  +41 07 03.13  22.4w 24YK27    F52  C~8cUC      
2024 12  26.423771 07 46 11.092  +41 07 03.76  22.2w 24YK27    F52  C~8cUC      
2024 12  26.441836 07 46 10.483  +41 07 04.79  22.2w 24YK27    F52  C~8cUC      
2024 12  26.620099 07 46 04.474  +41 07 12.75  22.0G 24YK27    F52  C~8cUC      
2024 12  26.620733 07 46 04.438  +41 07 12.83  22.2G 24YK27    F52  C~8cUC      
2024 12  30.442282 07 43 55.471  +41 09 44.07  22.5G 24YK27    F52  C~8cUC      
2024 12  30.453993 07 43 55.069  +41 09 43.98  22.1G 24YK27    F52  C~8cUC      
2024 12  30.465756 07 43 54.631  +41 09 44.65  22.5G 24YK27    F52  C~8cUC      
2025 01  03.465628 07 41 34.145  +41 11 16.20  22.5G 24YK27    F51  C~8cUC      
2025 01  03.477655 07 41 33.682  +41 11 16.31  22.4G 24YK27    F51  C~8cUC      
2025 01  03.489653 07 41 33.258  +41 11 16.34  22.7G 24YK27    F51  C~8cUC      
2025 01  03.501568 07 41 32.820  +41 11 16.45  23.1G 24YK27    F51  C~8cUC      
2025 01  05.378501 07 40 25.621  +41 11 34.27  22.2G 24YK27    T14  C~8cUC      
2025 01  05.379714 07 40 25.569  +41 11 34.28  22.8G 24YK27    T14  C~8cUC      
2025 01  05.380924 07 40 25.519  +41 11 34.27  22.2G 24YK27    T14  C~8cUC      
2025 01  06.530879 07 39 43.819  +41 11 37.20  22.5G 24YK27    T12  C~8cUC      
2025 01  06.535009 07 39 43.668  +41 11 37.16  22.7G 24YK27    T12  C~8cUC      

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     0.05       0.00    -0.06
     2   0.0000     -2.84     0.03       0.67    -0.01
     3   0.0001     -5.65     0.03       1.22    -0.07
     4   0.0001     -8.49     0.03       1.86    -0.05
     5   0.0411  -4422.22    -0.05     461.88     0.72
     6   0.0412  -4426.48     0.05     461.10    -0.07
     7   0.0412  -4431.45    -0.61     461.27     0.10
     8   0.0572  -6541.61    -0.05     417.97    -0.13
     9   0.0572  -6546.04    -0.02     417.81    -0.08
    10   0.0573  -6553.00    -0.03     417.60     0.04
    11   0.0578  -6621.31     0.21     413.39    -0.13
    12   0.0578  -6621.73     0.04     413.40    -0.11
    13   0.0682  -8084.50     0.09     308.39     0.14
    14   0.0683  -8088.97     0.31     307.53    -0.30
    15   0.0683  -8093.96     0.03     307.34    -0.06
    16   0.0793  -9675.91     0.26     131.13     0.08
    17   0.0793  -9681.09     0.01     130.38    -0.01
    18   0.0793  -9685.83     0.20     129.62    -0.11
    19   0.0794  -9690.73     0.18     128.92    -0.16
    20   0.0845 -10443.82    -0.06      22.77     0.06
    21   0.0845 -10444.40    -0.14      22.68     0.05
    22   0.0845 -10444.96    -0.20      22.58     0.02
    23   0.0877 -10911.27    -0.18     -50.12     0.09
    24   0.0877 -10912.95    -0.15     -50.43     0.07

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.

24YK27    quality flag:1

Type:       CENTAURR  CENTAURR  CENTAURR

axisobj         8.467     9.560     7.542
ecceobj         0.303     0.345     0.271
incobj         22.033    22.330    21.701
qmin            5.835     5.887     5.497
qmax           11.092    14.329     9.587
amean           8.465    10.236     7.371
amin            8.463     9.418     7.235
amax            8.467    11.234     7.556
emean           0.307     0.306     0.224
emin            0.303     0.231     0.199
emax            0.311     0.383     0.271
imean          23.365    23.861    22.191
imin           23.120    21.067    21.131
imax           23.610    26.108    22.806
excite_mean     0.501     0.510     0.440
fracstop        0.000     0.003     0.000
cjmean          4.474     3.966     4.982

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       135.6     224.0     175.6
kozaiamp          4.6      83.2     120.6