Orbit Fit and Astrometric record for 23PZ4

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: 23PZ4     
# Created Wed Apr 16 01:11:35 2025
# Orbit generated from Bernstein formalism
# Fitting      8 observations of      8
# Arc:   1.14y
# First observation: 2023/08/13
#  Last observation: 2024/10/04
Preliminary a, adot, b, bdot, g, gdot:
  -0.000015   0.024353  -0.000002  -0.000396   0.024816   0.000000
# Chi-squared of fit:     0.73 DOF:     10 RMS:  0.05
# Min/Max residuals:    -0.07    0.11
# Exact a, adot, b, bdot, g, gdot:
  1.584454E-05  2.474624E-02  1.668950E-08 -4.155443E-04  2.516714E-02  6.488592E-03
# Covariance matrix:
  7.2097E-13  3.3506E-12  8.3080E-14 -3.9511E-13  2.4702E-12  2.2752E-10
  3.3506E-12  3.4609E-10  5.2465E-12 -4.6217E-11  1.3850E-10  2.4136E-08
  8.3080E-14  5.2465E-12  3.7029E-13 -9.9452E-13  2.1755E-12  3.6488E-10
 -3.9511E-13 -4.6217E-11 -9.9452E-13  7.0918E-12 -1.8304E-11 -3.2379E-09
  2.4702E-12  1.3850E-10  2.1755E-12 -1.8304E-11  5.8141E-11  9.6133E-09
  2.2752E-10  2.4136E-08  3.6488E-10 -3.2379E-09  9.6133E-09  1.6895E-06
#      lat0       lon0       xBary       yBary       zBary        JD0
    7.103308  -52.033902   -0.204001    0.121795   -0.979550  2460169.853061
# Heliocentric elements and errors
Epoch:              2460160.5000  =  2023/08/04
Mean Anomaly:           60.81102 +/-     4.233
Argument of Peri:        6.85445 +/-     0.145
Long of Asc Node:      210.59297 +/-     0.035
Inclination:             6.99289 +/-     0.001
Eccentricity:         0.26352720 +/-    0.0523
Semi-Major Axis:     43.60353903 +/-    1.2813
Time of Perihelion: 2442395.6797 +/-     957.1
Perihelion:          32.11282046 +/-    2.4661
Aphelion:            55.09425760 +/-    2.7951
Period (y)              287.9326 +/-     12.69
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           25.03390032 +/-    0.0073
Ecliptic Y          -31.73561569 +/-    0.0094
Ecliptic Z            4.91355623 +/-    0.0015
Ecliptic XDOT         0.00255331 +/-    0.0001
Ecliptic YDOT         0.00110767 +/-    0.0001
Ecliptic ZDOT         0.00004244 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   40.71840497 +/-    0.0086
Geocenter to KBO     39.73434789 +/-    0.0120
# Hcoef:  7.04

The following table shows the complete astrometric record for 23PZ4. 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 (23PZ4) followed by the observatory code and reference code for the source of the astrometry.

2023 08  13.35226  20 34 04.483  -11 24 16.53  23.1r 23PZ4     T09  C~8nlW      
2023 08  13.49372  20 34 03.814  -11 24 19.30  23.2r 23PZ4     T09  C~8nlW      
2023 09  14.02116  20 31 56.611  -11 35 11.62  23.0r 23PZ4     269  C~8nlW      
2023 09  15.02127  20 31 53.515  -11 35 31.21  23.1r 23PZ4     269  C~8nlW      
2023 10  06.06582  20 31 07.176  -11 41 40.14  23.1r 23PZ4     269  C~8nlW      
2023 10  07.04784  20 31 05.966  -11 41 54.68  23.1r 23PZ4     269  C~8nlW      
2024 10  03.22934  20 36 42.033  -11 21 33.38        23PZ4     G37  C~8nlW      
2024 10  04.19282  20 36 40.537  -11 21 48.75        23PZ4     G37  C~8nlW      

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    -0.06       0.00    -0.06
     2   0.0004    -10.22     0.08      -0.23     0.04
     3   0.0867  -1983.54     0.01    -166.96    -0.07
     4   0.0894  -2032.47    -0.04    -174.67    -0.02
     5   0.1471  -2783.48    -0.05    -363.67    -0.00
     6   0.1497  -2804.30     0.07    -373.37     0.11
     7   1.1413   2283.77     0.03    -422.98    -0.04
     8   1.1440   2258.60    -0.03    -432.31     0.03

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.

23PZ4    quality flag:1

Type:         7:4EEE  CENTAURR CLASSICAL

axisobj        43.325    48.470    40.238
ecceobj         0.262     0.381     0.155
incobj          7.008     7.007     7.008
qmin           31.520    29.919    33.451
qmax           56.892    67.880    47.770
amean          43.726    48.750    40.424
amin           43.172    48.416    40.023
amax           44.404    49.042    40.819
emean           0.266     0.384     0.157
emin            0.252     0.381     0.140
emax            0.281     0.387     0.171
imean           8.537     7.509    10.469
imin            7.474     7.502     7.454
imax            9.441     7.521    14.999
excite_mean     0.305     0.406     0.241
fracstop        1.000     0.000     1.000
cjmean          2.986     2.950     2.997

libcent 0       178.0    -180.0    -180.0
libamp  0       129.2    -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       168.0      15.2     167.3
kozaiamp        180.0       0.7     179.9