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: 14FB62 # Created Fri Nov 22 02:09:51 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 41 observations of 41 # Arc: 21.18y # First observation: 2001/02/20 # Last observation: 2022/04/26 # Chi-squared of fit: 29.65 DOF: 76 RMS: 0.15 # Min/Max residuals: -0.29 0.43 # Exact a, adot, b, bdot, g, gdot: 1.900517E-05 3.787310E-02 2.053767E-06 3.633790E-03 3.177248E-02 -1.452143E-03 # Covariance matrix: 4.8991E-13 3.3438E-13 7.8844E-16 5.4329E-14 6.0232E-14 7.1552E-13 3.3438E-13 6.0157E-11 1.2695E-13 9.1206E-12 -2.9114E-11 1.2041E-10 7.8844E-16 1.2695E-13 4.8488E-13 -2.0507E-14 -6.1611E-14 2.5427E-13 5.4329E-14 9.1206E-12 -2.0507E-14 1.4211E-12 -4.6144E-12 1.8294E-11 6.0232E-14 -2.9114E-11 -6.1611E-14 -4.6144E-12 3.3728E-11 -6.1056E-11 7.1552E-13 1.2041E-10 2.5427E-13 1.8294E-11 -6.1056E-11 2.4152E-10 # lat0 lon0 xBary yBary zBary JD0 -2.645230 163.075975 0.186997 -0.045050 -0.971406 2451960.908151 # Heliocentric elements and errors Epoch: 2451960.5000 = 2001/02/20 Mean Anomaly: 349.59218 +/- 0.151 Argument of Peri: 350.16936 +/- 0.000 Long of Asc Node: 187.74825 +/- 0.000 Inclination: 6.05023 +/- 0.000 Eccentricity: 0.18399945 +/- 0.0096 Semi-Major Axis: 39.53972521 +/- 0.0000 Time of Perihelion: 2454585.9644 +/- 38.1 Perihelion: 32.26443763 +/- 0.3788 Aphelion: 46.81501279 +/- 0.3788 Period (y) 248.6329 +/- 0.00 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X -30.95047115 +/- 0.0010 Ecliptic Y 9.61887738 +/- 0.0003 Ecliptic Z -1.45247600 +/- 0.0001 Ecliptic XDOT -0.00085257 +/- 0.0000 Ecliptic YDOT -0.00315110 +/- 0.0000 Ecliptic ZDOT 0.00031875 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 32.44326958 +/- 0.0010 Geocenter to KBO 31.47382979 +/- 0.0011 # Hcoef: 7.70
The following table shows the complete astrometric record for 14FB62. 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 (14FB62) followed by the observatory code and reference code for the source of the astrometry.
2001 02 20.407408 10 53 32.60 +04 12 18.5 23.0V 14FB62 645 C~1zPr 2001 02 20.408238 10 53 32.60 +04 12 18.5 22.7V 14FB62 645 C~1zPr 2001 02 20.410726 10 53 32.59 +04 12 18.5 23.9V 14FB62 645 C~1zPr 2007 04 20.263951 11 38 49.92 +00 52 55.7 24.0V 14FB62 645 C~2hhz 2007 04 20.264780 11 38 49.92 +00 52 55.7 22.1V 14FB62 645 C~2hhz 2007 04 20.267268 11 38 49.92 +00 52 55.7 14FB62 645 C~2hhz 2014 03 30.053925 12 39 28.00 -03 55 14.4 22.8w 14FB62 W84 C~143s 2014 03 30.065200 12 39 27.93 -03 55 14.0 22.8w 14FB62 W84 C~143s 2014 03 30.076329 12 39 27.86 -03 55 13.6 22.8w 14FB62 W84 C~143s 2014 03 30.089055 12 39 27.78 -03 55 13.0 22.9w 14FB62 W84 C~143s 2014 03 30.102474 12 39 27.71 -03 55 12.6 22.6w 14FB62 W84 C~143s 2014 03 30.114996 12 39 27.64 -03 55 12.0 22.6w 14FB62 W84 C~143s 2014 03 30.126183 12 39 27.59 -03 55 11.8 22.9w 14FB62 W84 C~143s 2014 03 30.137299 12 39 27.51 -03 55 11.3 22.7w 14FB62 W84 C~143s 2014 03 30.150522 12 39 27.44 -03 55 10.7 22.7w 14FB62 W84 C~143s 2014 03 30.160122 12 39 27.39 -03 55 10.4 22.6w 14FB62 W84 C~143s 2014 03 30.295039 12 39 26.62 -03 55 05.3 22.5w 14FB62 W84 C~143s 2014 03 30.305870 12 39 26.56 -03 55 04.9 22.5w 14FB62 W84 C~143s 2014 03 31.085704 12 39 22.23 -03 54 35.1 22.8w 14FB62 W84 C~143s 2014 03 31.096460 12 39 22.15 -03 54 34.6 22.6w 14FB62 W84 C~143s 2014 03 31.106041 12 39 22.09 -03 54 34.1 22.3w 14FB62 W84 C~143s 2014 03 31.178527 12 39 21.72 -03 54 31.6 22.2w 14FB62 W84 C~143s 2014 03 31.188499 12 39 21.66 -03 54 31.3 22.3w 14FB62 W84 C~143s 2014 03 31.198109 12 39 21.60 -03 54 30.9 22.5w 14FB62 W84 C~143s 2014 04 07.171877 12 38 42.75 -03 50 06.3 22.8w 14FB62 W84 C~14R3 2014 04 07.184958 12 38 42.68 -03 50 05.9 22.8w 14FB62 W84 C~14R3 2014 04 08.248008 12 38 36.79 -03 49 25.7 22.7w 14FB62 W84 C~14R3 2014 04 08.258639 12 38 36.74 -03 49 25.4 22.8w 14FB62 W84 C~14R3 2014 05 18.23262 12 35 30.98 -03 28 12.1 22.9R 14FB62 695 C~156r 2014 05 18.24912 12 35 30.95 -03 28 12.0 23.0R 14FB62 695 C~156r 2014 05 18.26650 12 35 30.87 -03 28 11.4 23.1R 14FB62 695 C~156r 2014 05 21.19122 12 35 21.62 -03 27 06.8 23.0R 14FB62 695 C~156r 2014 05 21.20268 12 35 21.59 -03 27 06.6 22.9R 14FB62 695 C~156r 2014 05 21.25856 12 35 21.41 -03 27 05.4 23.0R 14FB62 695 C~156r 2014 05 21.27341 12 35 21.36 -03 27 05.0 22.8R 14FB62 695 C~156r 2015 03 16.30019 12 49 09.09 -04 42 17.4 22.8R 14FB62 G37 C~1zPr 2015 03 16.37248 12 49 08.70 -04 42 15.2 14FB62 G37 C~1zPr 2016 03 13.25808 12 57 44.72 -05 21 27.9 22.8R 14FB62 G37 C~1zPr 2016 03 13.30670 12 57 44.47 -05 21 26.0 14FB62 G37 C~1zPr 2022 04 26.246920 13 43 54.202 -08 30 19.22 23.1G 14FB62 G37 C~5ZZr 2022 04 26.313140 13 43 53.832 -08 30 16.99 14FB62 G37 C~5ZZr
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 -0.05 0.00 -0.03
2 0.0000 0.00 0.02 0.00 -0.06
3 0.0000 0.00 0.08 0.00 -0.15
4 6.1598 0.00 -0.22 0.00 0.02
5 6.1598 0.00 -0.16 0.00 -0.01
6 6.1598 0.00 0.00 0.00 -0.08
7 13.1024 0.00 0.25 0.00 0.05
8 13.1024 0.00 0.15 0.00 0.02
9 13.1024 0.00 0.05 0.00 0.00
10 13.1025 0.00 -0.08 0.00 0.12
11 13.1025 0.00 0.01 0.00 0.01
12 13.1026 0.00 0.03 0.00 0.13
13 13.1026 0.00 0.23 0.00 -0.09
14 13.1026 0.00 -0.02 0.00 -0.02
15 13.1027 0.00 0.05 0.00 0.08
16 13.1027 0.00 0.12 0.00 0.02
17 13.1030 0.00 0.06 0.00 -0.02
18 13.1031 0.00 0.08 0.00 -0.04
19 13.1052 0.00 0.13 0.00 0.07
20 13.1052 0.00 -0.16 0.00 0.16
21 13.1053 0.00 -0.24 0.00 0.30
22 13.1055 0.00 0.38 0.00 0.04
23 13.1055 0.00 0.33 0.00 -0.04
24 13.1055 0.00 0.25 0.00 -0.00
25 13.1246 0.00 -0.08 0.00 -0.04
26 13.1246 0.00 -0.03 0.00 -0.13
27 13.1276 0.00 -0.18 0.00 0.05
28 13.1276 0.00 -0.04 0.00 -0.05
29 13.2370 0.00 -0.28 0.00 0.27
30 13.2371 0.00 0.11 0.00 -0.01
31 13.2371 0.00 -0.20 0.00 0.19
32 13.2451 0.00 -0.02 0.00 -0.17
33 13.2452 0.00 0.07 0.00 -0.21
34 13.2453 0.00 -0.01 0.00 -0.21
35 13.2454 0.00 -0.06 0.00 -0.13
36 14.0640 0.00 -0.21 0.00 0.43
37 14.0642 0.00 -0.29 0.00 0.04
38 15.0578 0.00 0.00 0.00 -0.11
39 15.0579 0.00 -0.02 0.00 0.12
40 21.1768 0.00 -0.11 0.00 -0.27
41 21.1770 0.00 -0.05 0.00 -0.25
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.
14FB62 quality flag:3 Type: 3:2E 3:2E 3:2E axisobj 39.376 39.376 39.376 ecceobj 0.181 0.181 0.181 incobj 6.055 6.055 6.055 qmin 31.505 31.594 31.554 qmax 48.217 48.191 48.224 amean 39.457 39.457 39.457 amin 38.909 38.916 38.929 amax 40.066 40.063 40.069 emean 0.183 0.183 0.184 emin 0.164 0.164 0.164 emax 0.204 0.203 0.204 imean 6.712 6.762 6.680 imin 5.900 5.880 5.919 imax 7.577 7.664 7.518 excite_mean 0.218 0.218 0.217 fracstop 1.000 1.000 1.000 cjmean 2.997 2.997 2.998 libcent 0 180.1 178.4 178.4 libamp 0 132.5 129.4 129.2 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 192.0 186.3 181.1 kozaiamp 179.9 179.9 180.0