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: 14FL70 # Created Sat Apr 20 01:15:49 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 19 observations of 19 # Arc: 7.94y # First observation: 2014/03/25 # Last observation: 2022/03/02 # Chi-squared of fit: 47.41 DOF: 32 RMS: 0.28 # Min/Max residuals: -0.54 0.70 # Exact a, adot, b, bdot, g, gdot: 8.838690E-06 1.187552E-02 -1.237136E-06 -3.621624E-04 1.683979E-02 -5.384837E-03 # Covariance matrix: 1.8332E-13 -1.0257E-13 -4.7490E-15 2.5285E-15 4.1261E-14 -7.3655E-13 -1.0257E-13 1.4102E-13 7.5422E-15 -4.2597E-15 -6.1662E-14 1.2696E-12 -4.7490E-15 7.5422E-15 1.4015E-13 -2.7045E-14 -1.7662E-14 5.6877E-14 2.5285E-15 -4.2597E-15 -2.7045E-14 1.1492E-14 3.5426E-15 -3.9874E-14 4.1261E-14 -6.1662E-14 -1.7662E-14 3.5426E-15 2.4633E-13 -3.4219E-13 -7.3655E-13 1.2696E-12 5.6877E-14 -3.9874E-14 -3.4219E-13 1.2744E-11 # lat0 lon0 xBary yBary zBary JD0 -8.883294 156.651945 -0.460955 -0.136186 -0.872190 2456741.538078 # Heliocentric elements and errors Epoch: 2456742.5000 = 2014/03/26 Mean Anomaly: 281.59892 +/- 0.037 Argument of Peri: 24.04749 +/- 0.015 Long of Asc Node: 257.42684 +/- 0.003 Inclination: 8.89519 +/- 0.000 Eccentricity: 0.41031998 +/- 0.0002 Semi-Major Axis: 55.72237474 +/- 0.0094 Time of Perihelion: 2489829.8825 +/- 33.9 Perihelion: 32.85837111 +/- 0.0129 Aphelion: 78.58637837 +/- 0.0176 Period (y) 415.9610 +/- 0.11 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X -54.86138638 +/- 0.0016 Ecliptic Y 23.18038594 +/- 0.0007 Ecliptic Z -9.17018884 +/- 0.0003 Ecliptic XDOT 0.00003171 +/- 0.0000 Ecliptic YDOT -0.00212223 +/- 0.0000 Ecliptic ZDOT 0.00007715 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 60.25968564 +/- 0.0015 Geocenter to KBO 59.38350552 +/- 0.0018 # Hcoef: 6.01
The following table shows the complete astrometric record for 14FL70. 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 (14FL70) followed by the observatory code and reference code for the source of the astrometry.
2014 03 25.03730 10 20 28.813 +00 48 23.20 24.5r 14FL70 807 C~1MjU 2014 03 26.04437 10 20 25.991 +00 48 44.36 14FL70 807 C~1MjU 2014 03 26.09634 10 20 25.840 +00 48 45.51 14FL70 807 C~1MjU 2014 05 01.00746 10 19 14.599 +00 59 42.43 14FL70 304 C~1x8j 2014 05 01.09208 10 19 14.502 +00 59 43.79 23.9r 14FL70 304 C~1x8j 2014 05 02.08895 10 19 13.487 +00 59 58.21 14FL70 304 C~1x8j 2014 06 23.98699 10 19 45.849 +01 04 43.07 14FL70 I11 C~1x8j 2014 06 26.96820 10 19 52.504 +01 04 28.81 14FL70 I11 C~1x8j 2015 01 18.31331 10 26 27.106 +00 13 17.47 14FL70 I11 C~1x8j 2015 04 18.03857 10 22 03.994 +00 40 02.41 14FL70 304 C~1x8j 2015 04 18.14556 10 22 03.785 +00 40 04.44 14FL70 304 C~1x8j 2018 01 09.54915 10 34 32.92 -00 37 28.6 23.2y 14FL70 T09 C~7mw0 2018 01 09.58098 10 34 32.86 -00 37 28.7 23.0y 14FL70 T09 C~7mw0 2018 01 09.60825 10 34 32.79 -00 37 28.6 23.7y 14FL70 T09 C~7mw0 2018 01 09.64905 10 34 32.69 -00 37 28.4 23.0y 14FL70 T09 C~7mw0 2018 04 10.15385 10 30 01.800 -00 11 53.14 23.4R 14FL70 G37 C~2bH7 2018 04 10.22268 10 30 01.660 -00 11 51.99 14FL70 G37 C~2bH7 2022 03 02.249010 10 42 40.959 -01 34 36.31 23.6G 14FL70 G37 C~5S0Z 2022 03 02.305740 10 42 40.806 -01 34 36.31 14FL70 G37 C~5S0Z
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 0.51 0.00 -0.00
2 0.0028 0.00 0.47 0.00 0.25
3 0.0029 0.00 0.42 0.00 0.32
4 0.1012 0.00 -0.17 0.00 -0.16
5 0.1015 0.00 -0.24 0.00 -0.03
6 0.1042 0.00 -0.37 0.00 0.03
7 0.2490 0.00 -0.54 0.00 -0.14
8 0.2572 0.00 0.04 0.00 0.26
9 0.8194 0.00 0.03 0.00 -0.30
10 1.0650 0.00 0.01 0.00 -0.06
11 1.0653 0.00 -0.13 0.00 0.04
12 3.7961 0.00 -0.14 0.00 0.15
13 3.7961 0.00 0.01 0.00 -0.10
14 3.7962 0.00 -0.15 0.00 -0.13
15 3.7963 0.00 -0.31 0.00 -0.12
16 4.0441 0.00 -0.03 0.00 0.02
17 4.0443 0.00 0.31 0.00 -0.23
18 7.9376 0.00 -0.25 0.00 0.70
19 7.9378 0.00 0.44 0.00 -0.48
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.
14FL70 quality flag:3 Type: 5:2EEE 5:2EEE 5:2EEE axisobj 55.302 55.302 55.303 ecceobj 0.412 0.412 0.412 incobj 8.889 8.889 8.889 qmin 31.997 31.983 32.011 qmax 80.128 80.124 80.397 amean 55.462 55.462 55.462 amin 54.696 54.704 54.690 amax 56.445 56.442 56.444 emean 0.409 0.409 0.409 emin 0.396 0.396 0.396 emax 0.423 0.423 0.424 imean 10.874 10.872 10.876 imin 10.233 10.235 10.237 imax 11.378 11.378 11.378 excite_mean 0.451 0.451 0.451 fracstop 1.000 1.000 1.000 cjmean 2.975 2.975 2.975 libcent 0 179.7 180.7 180.0 libamp 0 88.1 89.0 88.2 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 93.4 93.5 93.2 kozaiamp 74.2 74.8 74.0