Orbit Fit and Astrometric record for 24PL17

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: 24PL17    
# Created Fri Aug 15 01:12:15 2025
# Orbit generated from Bernstein formalism
# Fitting     19 observations of     19
# Arc:   1.80y
# First observation: 2023/10/05
#  Last observation: 2025/07/25
Preliminary a, adot, b, bdot, g, gdot:
   0.007592  -0.194147  -0.004279   0.058572   0.117572   0.000000
# Chi-squared of fit:     7.97 DOF:     32 RMS:  0.11
# Min/Max residuals:    -0.35    0.28
# Exact a, adot, b, bdot, g, gdot:
 -2.715260E-05 -1.461533E-01  7.718599E-06  4.590288E-02  8.577429E-02 -1.403991E-01
# Covariance matrix:
  3.3036E-13 -5.2043E-13 -5.8985E-14  1.4960E-13  1.0910E-13  1.0987E-12
 -5.2043E-13  2.6064E-12  1.5209E-13 -3.4878E-13 -2.2166E-12 -4.3131E-12
 -5.8985E-14  1.5209E-13  2.7143E-13 -2.8153E-13  1.1775E-14 -6.4689E-13
  1.4960E-13 -3.4878E-13 -2.8153E-13  4.4581E-13 -8.4462E-14  1.6260E-12
  1.0910E-13 -2.2166E-12  1.1775E-14 -8.4462E-14  2.8379E-12  1.9678E-12
  1.0987E-12 -4.3131E-12 -6.4689E-13  1.6260E-12  1.9678E-12  1.2640E-11
#      lat0       lon0       xBary       yBary       zBary        JD0
  -35.915922    3.564245   -0.137995   -0.576139   -0.795092  2460222.928375
# Heliocentric elements and errors
Epoch:              2460220.5000  =  2023/10/03
Mean Anomaly:          357.72468 +/-     0.003
Argument of Peri:       26.21600 +/-     0.003
Long of Asc Node:      307.20258 +/-     0.000
Inclination:           142.03010 +/-     0.000
Eccentricity:         0.92220160 +/-    0.0001
Semi-Major Axis:     84.46845182 +/-    0.0635
Time of Perihelion: 2462012.6727 +/-       0.0
Perihelion:           6.57151065 +/-    0.0069
Aphelion:           162.36539299 +/-    0.1222
Period (y)              776.3365 +/-      0.88
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           10.40355700 +/-    0.0002
Ecliptic Y            0.78769695 +/-    0.0000
Ecliptic Z           -6.83878589 +/-    0.0001
Ecliptic XDOT        -0.00247862 +/-    0.0000
Ecliptic YDOT        -0.00482045 +/-    0.0000
Ecliptic ZDOT         0.00381545 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   12.47491312 +/-    0.0002
Geocenter to KBO     11.65850501 +/-    0.0002
# Hcoef: 10.78

The following table shows the complete astrometric record for 24PL17. 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 (24PL17) followed by the observatory code and reference code for the source of the astrometry.

2023 10  05.427574 01 16 18.311  -31 12 33.33  21.8w 24PL17    F51  C~8Hfg      
2023 10  05.438528 01 16 18.020  -31 12 35.17  21.9w 24PL17    F51  C~8Hfg      
2023 10  05.449485 01 16 17.665  -31 12 36.39  21.6w 24PL17    F51  C~8Hfg      
2023 10  05.460442 01 16 17.370  -31 12 37.62  21.6w 24PL17    F51  C~8Hfg      
2024 08  15.501591 00 54 20.061  -29 55 40.18  21.4w 24PL17    F51  C~8Hfg      
2024 08  15.511285 00 54 19.840  -29 55 42.43  21.3w 24PL17    F51  C~8Hfg      
2024 08  15.520962 00 54 19.615  -29 55 44.46  21.2w 24PL17    F51  C~8Hfg      
2024 08  15.530639 00 54 19.387  -29 55 46.98  21.4w 24PL17    F51  C~8Hfg      
2024 09  01.504431 00 46 54.418  -30 59 09.81  21.1G 24PL17    F51  C~8Hfg      
2024 09  07.480050 00 43 54.260  -31 19 42.33  21.2w 24PL17    F51  C~8Hfg      
2024 09  07.491588 00 43 53.884  -31 19 44.48  21.4w 24PL17    F51  C~8Hfg      
2024 09  07.503198 00 43 53.525  -31 19 46.75  21.4w 24PL17    F51  C~8Hfg      
2024 09  07.568280 00 43 51.508  -31 19 59.66  21.7G 24PL17    F51  C~8Hfg      
2024 09  07.568925 00 43 51.471  -31 19 59.86  21.8G 24PL17    F51  C~8Hfg      
2024 09  08.468747 00 43 23.470  -31 22 58.20  21.7G 24PL17    T12  C~8Hfg      
2024 09  08.469827 00 43 23.433  -31 22 58.46  21.9G 24PL17    T12  C~8Hfg      
2025 07  25.583303 00 06 40.585  -29 03 58.02  20.8w 24PL17    F51  C~91bO      
2025 07  25.589832 00 06 40.435  -29 03 59.58  20.9w 24PL17    F51  C~91bO      
2025 07  25.596346 00 06 40.255  -29 04 00.98  20.8w 24PL17    F51  C~91bO      

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     0.15
     2   0.0000     -4.16     0.12       0.10    -0.35
     3   0.0001     -8.76    -0.24       1.14     0.07
     4   0.0001    -12.68     0.08       1.80     0.12
     5   0.8626 -13260.37    -0.06   11694.27    -0.00
     6   0.8627 -13263.94    -0.00   11693.44    -0.03
     7   0.8627 -13267.47     0.10   11692.83     0.17
     8   0.8627 -13271.24    -0.05   11691.79    -0.07
     9   0.9092 -20133.68    -0.03   10608.97    -0.05
    10   0.9255 -22777.59    -0.05   10413.12    -0.10
    11   0.9256 -22782.94    -0.15   10413.08     0.11
    12   0.9256 -22788.13    -0.06   10412.84     0.12
    13   0.9258 -22817.36     0.28   10411.35    -0.00
    14   0.9258 -22817.88     0.05   10411.35     0.02
    15   0.9282 -23223.31     0.01   10391.14    -0.06
    16   0.9282 -23223.85    -0.04   10391.09    -0.09
    17   1.8047 -47849.41    -0.06   29094.91    -0.00
    18   1.8047 -47851.91     0.12   29094.07    -0.10
    19   1.8047 -47854.75    -0.06   29093.52     0.10

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.

24PL17    quality flag:3

Type:       CENTAURR  CENTAURR  CENTAURR

axisobj        83.225    83.289    83.161
ecceobj         0.922     0.922     0.922
incobj        142.039   142.039   142.039
qmin            6.336     6.400     6.295
qmax          185.267   180.357   223.964
amean          85.199    84.325    97.538
amin           74.164    75.506    83.161
amax           96.837    94.103   115.512
emean           0.913     0.915     0.923
emin            0.903     0.906     0.903
emax            0.925     0.925     0.941
imean         139.371   140.881   139.452
imin          134.365   137.215   135.634
imax          144.020   144.021   144.035
excite_mean     1.121     1.111     1.129
fracstop        0.089     0.059     0.114
cjmean         -0.687    -0.696    -0.734

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        32.4      32.5      28.9
kozaiamp          5.1       4.6       4.2