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: 23FS54
# Created Wed Dec 25 02:11:19 2024
# Orbit generated from Bernstein formalism
# Fitting 9 observations of 9
# Arc: 0.97y
# First observation: 2023/03/21
# Last observation: 2024/03/08
Preliminary a, adot, b, bdot, g, gdot:
-0.000004 0.010746 0.000001 0.000559 0.015586 0.000000
# Chi-squared of fit: 8.70 DOF: 12 RMS: 0.17
# Min/Max residuals: -0.29 0.35
# Exact a, adot, b, bdot, g, gdot:
1.072602E-05 1.072755E-02 1.169812E-06 5.596603E-04 1.571744E-02 2.144261E-03
# Covariance matrix:
7.4679E-13 4.2048E-12 1.9275E-14 2.1317E-13 3.1357E-12 4.1307E-10
4.2048E-12 6.9735E-10 3.4946E-13 3.1114E-11 2.7686E-10 5.5390E-08
1.9275E-14 3.4946E-13 3.5173E-13 -3.7907E-13 1.9957E-13 2.9984E-11
2.1317E-13 3.1114E-11 -3.7907E-13 2.2273E-12 1.2395E-11 2.4753E-09
3.1357E-12 2.7686E-10 1.9957E-13 1.2395E-11 1.1473E-10 2.2187E-08
4.1307E-10 5.5390E-08 2.9984E-11 2.4753E-09 2.2187E-08 4.4111E-06
# lat0 lon0 xBary yBary zBary JD0
2.607688 156.931889 -0.395715 0.041807 -0.922823 2460024.799871
# Heliocentric elements and errors
Epoch: 2460020.5000 = 2023/03/17
Mean Anomaly: 124.98249 +/- 28.221
Argument of Peri: 253.72273 +/- 24.476
Long of Asc Node: 116.58666 +/- 0.104
Inclination: 3.93915 +/- 0.008
Eccentricity: 0.29098154 +/- 0.0804
Semi-Major Axis: 53.29523491 +/- 2.7191
Time of Perihelion: 2410682.9385 +/- 10481.2
Perihelion: 37.78730559 +/- 4.6993
Aphelion: 68.80316422 +/- 5.5397
Period (y) 389.0817 +/- 29.78
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -59.47188193 +/- 0.0398
Ecliptic Y 24.90136281 +/- 0.0170
Ecliptic Z 2.89476611 +/- 0.0020
Ecliptic XDOT -0.00107331 +/- 0.0003
Ecliptic YDOT -0.00156606 +/- 0.0001
Ecliptic ZDOT 0.00011436 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 64.53961792 +/- 0.0373
Geocenter to KBO 63.62357828 +/- 0.0434
# Hcoef: 5.28
The following table shows the complete astrometric record for 23FS54. 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 (23FS54) followed by the observatory code and reference code for the source of the astrometry.
2023 03 21.29907 10 38 34.292 +11 23 14.35 23.3r 23FS54 568 C~7xZn 2023 03 21.49670 10 38 33.706 +11 23 17.57 23.3r 23FS54 568 C~7xZn 2023 04 22.11167 10 37 18.602 +11 30 00.22 23.3r 23FS54 304 C~7xZn 2023 05 15.07121 10 36 52.992 +11 31 43.36 23.4r 23FS54 304 C~7xZn 2023 05 15.97289 10 36 52.560 +11 31 43.73 23.2r 23FS54 304 C~7xZn 2024 03 06.22490 10 41 39.497 +11 07 02.97 23FS54 G37 C~7xZn 2024 03 06.24854 10 41 39.461 +11 07 03.86 23FS54 G37 C~7xZn 2024 03 07.24436 10 41 36.305 +11 07 22.29 23.3r 23FS54 304 C~7xZn 2024 03 08.18364 10 41 33.389 +11 07 39.65 23.4r 23FS54 304 C~7xZn
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 0.01 0.00 -0.13
2 0.0005 -9.20 0.00 -0.23 -0.17
3 0.0871 -1183.88 -0.06 -38.25 0.35
4 0.1500 -1571.67 0.18 -82.60 0.07
5 0.1524 -1577.70 -0.13 -84.62 -0.10
6 0.9608 2890.35 -0.09 119.84 -0.29
7 0.9608 2889.53 0.27 120.47 0.34
8 0.9636 2839.54 -0.16 120.09 -0.06
9 0.9661 2793.24 -0.02 120.06 -0.01
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.
23FS54 quality flag:0 Type: ERR2LARGE ERR2LARGE ERR2LARGE axisobj 0.000 0.000 0.000 ecceobj -1.000 -1.000 -1.000 incobj -1.000 -1.000 -1.000 qmin 0.000 0.000 0.000 qmax 0.000 0.000 0.000 amean 0.000 0.000 0.000 amin 0.000 0.000 0.000 amax 0.000 0.000 0.000 emean 0.000 0.000 0.000 emin 0.000 0.000 0.000 emax 0.000 0.000 0.000 imean 0.000 0.000 0.000 imin 0.000 0.000 0.000 imax 0.000 0.000 0.000 excite_mean 0.000 0.000 0.000 fracstop 0.000 0.000 0.000 cjmean 0.000 0.000 0.000 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 0.0 0.0 0.0 kozaiamp 0.0 0.0 0.0