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: 14PE88 # Created Fri Apr 26 01:16:02 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 36 observations of 36 # Arc: 7.03y # First observation: 2014/07/27 # Last observation: 2021/08/07 # Chi-squared of fit: 36.33 DOF: 66 RMS: 0.18 # Min/Max residuals: -0.49 0.60 # Exact a, adot, b, bdot, g, gdot: 1.707395E-05 2.945176E-02 -9.377874E-07 -1.421102E-03 2.757150E-02 3.730788E-04 # Covariance matrix: 1.9998E-13 -9.7148E-14 -1.6015E-14 4.5585E-15 1.2309E-13 -3.3378E-13 -9.7148E-14 1.1265E-13 8.1892E-15 -5.1025E-15 -4.4441E-14 5.2495E-13 -1.6015E-14 8.1892E-15 1.0908E-13 -2.0331E-14 -2.7506E-14 2.7695E-14 4.5585E-15 -5.1025E-15 -2.0331E-14 6.3448E-15 4.1646E-15 -2.4066E-14 1.2309E-13 -4.4441E-14 -2.7506E-14 4.1646E-15 2.3587E-13 -1.0485E-13 -3.3378E-13 5.2495E-13 2.7695E-14 -2.4066E-14 -1.0485E-13 2.6457E-12 # lat0 lon0 xBary yBary zBary JD0 -22.997918 -53.739347 0.036381 -0.397453 -0.936606 2456865.971013 # Heliocentric elements and errors Epoch: 2456866.5000 = 2014/07/28 Mean Anomaly: 8.07526 +/- 0.036 Argument of Peri: 253.86269 +/- 0.042 Long of Asc Node: 43.50331 +/- 0.000 Inclination: 22.55209 +/- 0.000 Eccentricity: 0.07417690 +/- 0.0001 Semi-Major Axis: 40.14944442 +/- 0.0036 Time of Perihelion: 2454782.1455 +/- 9.3 Perihelion: 37.17128322 +/- 0.0044 Aphelion: 43.12760561 +/- 0.0048 Period (y) 254.4061 +/- 0.03 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 20.31764187 +/- 0.0003 Ecliptic Y -27.76073513 +/- 0.0005 Ecliptic Z -14.17032608 +/- 0.0002 Ecliptic XDOT 0.00234072 +/- 0.0000 Ecliptic YDOT 0.00174263 +/- 0.0000 Ecliptic ZDOT -0.00014425 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 37.20567989 +/- 0.0004 Geocenter to KBO 36.26935344 +/- 0.0006 # Hcoef: 7.06
The following table shows the complete astrometric record for 14PE88. 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 (14PE88) followed by the observatory code and reference code for the source of the astrometry.
2014 07 27.470235 21 04 02.378 -40 49 17.99 22.3G 14PE88 F51 C~5BTn 2014 07 27.478838 21 04 02.341 -40 49 18.05 23.7G 14PE88 F51 C~5BTn 2014 07 27.487428 21 04 02.236 -40 49 18.44 22.7G 14PE88 F51 C~5BTn 2014 08 08.162946 21 02 44.021 -40 53 44.97 14PE88 W84 C~3wpJ 2014 09 04.100342 20 59 52.662 -40 57 38.63 22.3i 14PE88 W84 C~3wpJ 2014 09 24.017240 20 58 15.840 -40 54 21.98 23.4g 14PE88 W84 C~3wpJ 2014 09 25.028351 20 58 11.948 -40 54 03.74 23.2g 14PE88 W84 C~3wpJ 2014 09 26.038687 20 58 08.173 -40 53 44.89 14PE88 W84 C~3wpJ 2014 09 26.060851 20 58 08.093 -40 53 44.49 22.4i 14PE88 W84 C~3wpJ 2014 09 27.039705 20 58 04.551 -40 53 25.30 22.2z 14PE88 W84 C~3wpJ 2014 10 13.071580 20 57 22.870 -40 46 36.45 22.5r 14PE88 W84 C~3wpK 2014 10 19.044127 20 57 15.729 -40 43 21.60 21.6r 14PE88 W84 C~3wpK 2016 06 03.576442 21 24 58.648 -39 16 22.65 23.1G 14PE88 F51 C~5BTn 2016 08 09.420256 21 19 30.864 -39 56 52.57 22.4G 14PE88 F51 C~5BTn 2016 08 09.440868 21 19 30.729 -39 56 52.70 22.4G 14PE88 F51 C~5BTn 2016 08 09.451200 21 19 30.648 -39 56 53.31 22.5G 14PE88 F51 C~5BTn 2017 06 23.552898 21 32 09.974 -38 57 05.21 23.3G 14PE88 F51 C~5BTn 2017 08 14.391019 21 27 18.072 -39 26 27.44 22.4G 14PE88 F51 C~5BTn 2018 07 10.488688 21 38 59.534 -38 33 28.52 22.3G 14PE88 F51 C~5BTn 2018 08 17.360168 21 35 11.141 -38 53 15.53 22.2G 14PE88 F51 C~5BTn 2018 08 17.370108 21 35 11.089 -38 53 15.54 22.3G 14PE88 F51 C~5BTn 2019 07 03.522222 21 47 29.779 -37 51 29.81 23.1G 14PE88 F51 C~5BTn 2019 07 03.541547 21 47 29.731 -37 51 30.75 22.7G 14PE88 F51 C~5BTn 2020 06 21.564285 21 55 55.825 -37 04 33.14 23.2G 14PE88 F51 C~5BTn 2020 06 21.575106 21 55 55.803 -37 04 34.33 22.8G 14PE88 F51 C~5BTn 2020 06 21.585904 21 55 55.760 -37 04 34.57 22.5G 14PE88 F51 C~5BTn 2020 06 24.540723 21 55 46.868 -37 06 41.38 22.6G 14PE88 F51 C~5BTn 2020 06 24.561392 21 55 46.823 -37 06 41.89 22.8G 14PE88 F51 C~5BTn 2020 06 30.520808 21 55 26.060 -37 10 56.53 22.3G 14PE88 F51 C~5BTn 2020 06 30.531108 21 55 26.045 -37 10 56.78 23.0G 14PE88 F51 C~5BTn 2020 08 14.372153 21 51 24.707 -37 38 01.36 22.6G 14PE88 F51 C~5BTn 2020 08 14.391521 21 51 24.579 -37 38 02.00 22.3G 14PE88 F51 C~5BTn 2020 08 14.401150 21 51 24.529 -37 38 02.08 22.9G 14PE88 F51 C~5BTn 2021 08 07.425747 21 59 55.260 -36 54 31.70 22.3G 14PE88 F51 C~5BTn 2021 08 07.436117 21 59 55.201 -36 54 32.00 22.7G 14PE88 F51 C~5BTn 2021 08 07.456890 21 59 55.086 -36 54 33.05 22.9G 14PE88 F51 C~5BTn
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 0.01
2 0.0000 0.00 0.26 0.00 0.18
3 0.0000 0.00 -0.45 0.00 0.02
4 0.0320 0.00 0.30 0.00 -0.11
5 0.1058 0.00 0.06 0.00 0.02
6 0.1603 0.00 0.02 0.00 0.04
7 0.1631 0.00 -0.02 0.00 0.06
8 0.1658 0.00 -0.04 0.00 -0.06
9 0.1659 0.00 0.02 0.00 -0.08
10 0.1686 0.00 -0.01 0.00 -0.02
11 0.2125 0.00 0.03 0.00 -0.08
12 0.2288 0.00 0.03 0.00 0.08
13 1.8538 0.00 0.10 0.00 0.10
14 2.0368 0.00 -0.00 0.00 -0.10
15 2.0369 0.00 0.05 0.00 0.22
16 2.0369 0.00 -0.12 0.00 -0.17
17 2.9078 0.00 -0.26 0.00 -0.24
18 3.0497 0.00 -0.11 0.00 -0.08
19 3.9535 0.00 0.12 0.00 -0.04
20 4.0572 0.00 0.05 0.00 0.08
21 4.0572 0.00 0.25 0.00 0.27
22 4.9337 0.00 -0.21 0.00 -0.08
23 4.9338 0.00 0.33 0.00 -0.21
24 5.9031 0.00 -0.14 0.00 0.60
25 5.9031 0.00 0.01 0.00 -0.13
26 5.9031 0.00 -0.15 0.00 0.09
27 5.9112 0.00 0.02 0.00 -0.49
28 5.9113 0.00 0.37 0.00 -0.12
29 5.9276 0.00 -0.22 0.00 -0.01
30 5.9276 0.00 0.16 0.00 0.18
31 6.0504 0.00 -0.17 0.00 0.07
32 6.0504 0.00 -0.22 0.00 -0.08
33 6.0505 0.00 -0.04 0.00 0.09
34 7.0307 0.00 -0.12 0.00 0.08
35 7.0307 0.00 -0.04 0.00 0.11
36 7.0308 0.00 0.17 0.00 -0.29
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.
14PE88 quality flag:3 Type: SCATEXTD SCATEXTD SCATEXTD axisobj 40.255 40.255 40.255 ecceobj 0.077 0.077 0.077 incobj 22.584 22.584 22.584 qmin 36.757 36.791 36.791 qmax 44.184 44.216 44.240 amean 40.357 40.356 40.356 amin 40.035 40.035 40.035 amax 40.684 40.684 40.686 emean 0.073 0.073 0.073 emin 0.061 0.060 0.061 emax 0.087 0.087 0.088 imean 21.474 21.474 21.474 imin 20.826 20.826 20.826 imax 22.053 22.037 22.029 excite_mean 0.373 0.373 0.373 fracstop 1.000 1.000 1.000 cjmean 2.894 2.894 2.894 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 181.4 181.2 181.3 kozaiamp 180.0 180.0 180.0