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: 00PL30 # Created Thu Apr 25 01:10:10 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 21 observations of 21 # Arc: 23.09y # First observation: 2000/08/05 # Last observation: 2023/09/06 # Chi-squared of fit: 189.66 DOF: 36 RMS: 0.53 # Min/Max residuals: -1.57 0.82 # Exact a, adot, b, bdot, g, gdot: 1.040803E-05 1.629064E-02 -1.001031E-08 1.656768E-03 2.054813E-02 -2.548616E-03 # Covariance matrix: 1.3952E-13 -3.0458E-14 1.9052E-15 -2.8710E-15 1.2441E-13 -6.9963E-14 -3.0458E-14 3.1827E-14 -2.3062E-15 3.3101E-15 -2.4545E-14 8.0211E-14 1.9052E-15 -2.3062E-15 1.0412E-13 -5.3838E-15 2.0362E-15 -5.9458E-15 -2.8710E-15 3.3101E-15 -5.3838E-15 1.0163E-15 -3.8725E-15 8.5777E-15 1.2441E-13 -2.4545E-14 2.0362E-15 -3.8725E-15 7.4705E-13 -9.6568E-14 -6.9963E-14 8.0211E-14 -5.9458E-15 8.5777E-15 -9.6568E-14 2.0798E-13 # lat0 lon0 xBary yBary zBary JD0 -0.778244 -41.290754 0.102450 -0.013897 -1.008249 2451761.943623 # Heliocentric elements and errors Epoch: 2451762.5000 = 2000/08/06 Mean Anomaly: 229.95846 +/- 0.033 Argument of Peri: 139.90292 +/- 0.016 Long of Asc Node: 326.04711 +/- 0.000 Inclination: 5.86177 +/- 0.000 Eccentricity: 0.23955994 +/- 0.0001 Semi-Major Axis: 42.06594380 +/- 0.0054 Time of Perihelion: 2487760.1359 +/- 15.4 Perihelion: 31.98862897 +/- 0.0055 Aphelion: 52.14325863 +/- 0.0076 Period (y) 272.8376 +/- 0.05 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 37.25913807 +/- 0.0015 Ecliptic Y -32.84869861 +/- 0.0014 Ecliptic Z -0.66098782 +/- 0.0000 Ecliptic XDOT 0.00117229 +/- 0.0000 Ecliptic YDOT 0.00185851 +/- 0.0000 Ecliptic ZDOT 0.00022549 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 49.67622266 +/- 0.0015 Geocenter to KBO 48.66635538 +/- 0.0020 # Hcoef: 7.32
The following table shows the complete astrometric record for 00PL30. 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 (00PL30) followed by the observatory code and reference code for the source of the astrometry.
2000 08 05.44288 21 25 33.61 -15 57 26.7 00PL30 568 Cb8005 2000 08 05.48448 21 25 33.45 -15 57 27.4 00PL30 568 Cb8005 2000 08 05.52555 21 25 33.27 -15 57 28.3 23.4R 00PL30 568 Cb8005 2000 08 06.43095 21 25 29.53 -15 57 45.2 00PL30 568 Cb8005 2000 08 06.47320 21 25 29.35 -15 57 46.0 23.7R 00PL30 568 Cb8005 2000 08 06.51483 21 25 29.17 -15 57 46.8 00PL30 568 Cb8005 2000 09 24.27180 21 22 26.20 -16 10 59.6 24.5R 00PL30 568 Cd2824 2000 09 24.32190 21 22 26.06 -16 11 00.1 24.4R 00PL30 568 Cd2824 2000 09 24.38171 21 22 25.88 -16 11 01.0 24.3R 00PL30 568 Cd2824 2001 08 12.54968 21 28 39.09 -15 36 38.7 00PL30 568 Cd2824 2001 08 12.58664 21 28 38.91 -15 36 39.5 00PL30 568 Cd2824 2001 08 13.40598 21 28 35.55 -15 36 54.4 00PL30 568 Cd2824 2001 08 13.44202 21 28 35.39 -15 36 54.6 00PL30 568 Cd2824 2003 07 08.45504 21 38 03.21 -14 39 05.6 24.0R 00PL30 568 Ci2628 2003 07 09.50134 21 37 59.84 -14 39 21.5 00PL30 568 Ci2628 2019 09 04.220010 22 33 03.593 -07 53 03.35 23.3G 00PL30 G37 C~3cUl 2019 09 04.292170 22 33 03.293 -07 53 05.06 00PL30 G37 C~3cUl 2019 09 04.339690 22 33 03.100 -07 53 06.22 00PL30 G37 C~3cUl 2023 09 06.271050 22 48 22.356 -05 53 12.86 23.4G 00PL30 G37 C~7ALU 2023 09 06.307600 22 48 22.205 -05 53 13.35 00PL30 G37 C~7ALU 2023 09 06.344290 22 48 22.049 -05 53 14.34 00PL30 G37 C~7ALU
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 0.35 0.00 0.39
2 0.0001 0.00 0.57 0.00 0.46
3 0.0002 0.00 0.46 0.00 0.32
4 0.0027 0.00 0.44 0.00 0.27
5 0.0028 0.00 0.41 0.00 0.25
6 0.0029 0.00 0.34 0.00 0.22
7 0.1364 0.00 0.28 0.00 0.08
8 0.1366 0.00 0.36 0.00 0.16
9 0.1367 0.00 0.27 0.00 -0.06
10 1.0188 0.00 -1.20 0.00 -0.67
11 1.0189 0.00 -1.57 0.00 -0.78
12 1.0211 0.00 -1.07 0.00 -0.22
13 1.0212 0.00 -1.18 0.00 0.26
14 2.9213 0.00 0.69 0.00 -0.56
15 2.9242 0.00 0.82 0.00 -0.34
16 19.0795 0.00 0.07 0.00 0.13
17 19.0797 0.00 0.15 0.00 0.13
18 19.0798 0.00 0.27 0.00 0.09
19 23.0851 0.00 -0.19 0.00 -0.29
20 23.0852 0.00 -0.12 0.00 0.12
21 23.0853 0.00 -0.10 0.00 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.
00PL30 quality flag:3 Type: 5:3EE 5:3EE 5:3EE axisobj 42.133 42.133 42.133 ecceobj 0.238 0.238 0.238 incobj 5.853 5.853 5.853 qmin 31.519 31.568 31.502 qmax 54.023 54.017 54.026 amean 42.328 42.328 42.328 amin 41.740 41.704 41.739 amax 42.995 43.044 43.018 emean 0.240 0.239 0.241 emin 0.221 0.225 0.226 emax 0.257 0.256 0.258 imean 7.093 6.110 7.002 imin 5.628 4.034 5.649 imax 8.195 8.201 8.190 excite_mean 0.270 0.263 0.271 fracstop 1.000 1.000 1.000 cjmean 2.994 3.000 2.994 libcent 0 179.9 180.8 178.9 libamp 0 141.6 151.3 144.9 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 188.4 188.3 187.4 kozaiamp 180.0 179.9 179.9