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: 14SP363 # Created Thu Apr 25 01:16:11 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 73 observations of 73 # Arc: 9.09y # First observation: 2014/09/17 # Last observation: 2023/10/19 # Chi-squared of fit: 22.59 DOF: 140 RMS: 0.10 # Min/Max residuals: -0.33 0.35 # Exact a, adot, b, bdot, g, gdot: 1.489854E-05 2.235965E-02 -5.727750E-06 -8.459730E-03 2.272717E-02 -3.365555E-03 # Covariance matrix: 7.1529E-14 -2.1692E-14 -8.5332E-15 5.7477E-15 3.1340E-14 -8.0777E-14 -2.1692E-14 2.4605E-14 6.7464E-15 -8.0403E-15 1.5799E-14 1.1940E-13 -8.5332E-15 6.7464E-15 4.2662E-14 -1.1942E-14 -2.2094E-15 4.0838E-14 5.7477E-15 -8.0403E-15 -1.1942E-14 7.4296E-15 -4.8866E-15 -4.7353E-14 3.1340E-14 1.5799E-14 -2.2094E-15 -4.8866E-15 8.2101E-14 8.0343E-14 -8.0777E-14 1.1940E-13 4.0838E-14 -4.7353E-14 8.0343E-14 7.0181E-13 # lat0 lon0 xBary yBary zBary JD0 -24.284532 12.518555 0.320412 -0.392811 -0.870953 2456917.714598 # Heliocentric elements and errors Epoch: 2456918.5000 = 2014/09/18 Mean Anomaly: 341.05070 +/- 0.004 Argument of Peri: 268.15387 +/- 0.008 Long of Asc Node: 145.54457 +/- 0.000 Inclination: 31.26847 +/- 0.000 Eccentricity: 0.31624048 +/- 0.0000 Semi-Major Axis: 62.42231760 +/- 0.0048 Time of Perihelion: 2466400.4786 +/- 19.9 Perihelion: 42.68185387 +/- 0.0044 Aphelion: 82.16278134 +/- 0.0070 Period (y) 493.1943 +/- 0.06 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 40.15285881 +/- 0.0005 Ecliptic Y 8.58967719 +/- 0.0001 Ecliptic Z -18.09613447 +/- 0.0002 Ecliptic XDOT -0.00135849 +/- 0.0000 Ecliptic YDOT 0.00245406 +/- 0.0000 Ecliptic ZDOT -0.00076208 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 44.87220384 +/- 0.0005 Geocenter to KBO 44.00034230 +/- 0.0006 # Hcoef: 6.14
The following table shows the complete astrometric record for 14SP363. 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 (14SP363) followed by the observatory code and reference code for the source of the astrometry.
2014 09 17.21382 01 24 44.21 -17 22 55.0 14SP363 W84 C~2gaD 2014 09 17.29087 01 24 43.91 -17 22 58.0 23.1V 14SP363 W84 C~2gaD 2014 09 17.36648 01 24 43.63 -17 23 01.1 14SP363 W84 C~2gaD 2014 09 18.33506 01 24 40.07 -17 23 39.1 14SP363 W84 C~2gaD 2014 09 18.38072 01 24 39.89 -17 23 40.8 14SP363 W84 C~2gaD 2014 09 21.30612 01 24 28.87 -17 25 33.8 23.2V 14SP363 W84 C~2gaE 2014 09 22.31750 01 24 24.98 -17 26 12.2 14SP363 W84 C~2gaE 2014 09 22.39605 01 24 24.67 -17 26 15.2 14SP363 W84 C~2gaE 2014 11 21.19809 01 20 23.276 -17 46 40.71 22.7r 14SP363 W84 C~4yUV 2014 11 21.19809 01 20 23.28 -17 46 40.7 22.7r 14SP363 W84 C~3cnq 2014 11 21.21205 01 20 23.23 -17 46 40.8 22.5i 14SP363 W84 C~3cnq 2014 11 21.21205 01 20 23.232 -17 46 40.76 22.4i 14SP363 W84 C~4yUV 2014 11 21.21342 01 20 23.23 -17 46 40.7 23.6g 14SP363 W84 C~3cnq 2014 11 21.21479 01 20 23.22 -17 46 40.8 22.3i 14SP363 W84 C~3cnq 2014 11 21.21479 01 20 23.220 -17 46 40.77 22.3i 14SP363 W84 C~4yUV 2014 12 12.15687 01 19 29.53 -17 43 30.6 22.4z 14SP363 W84 C~3cnq 2014 12 12.15687 01 19 29.526 -17 43 30.58 22.4z 14SP363 W84 C~4yUV 2014 12 24.10560 01 19 13.85 -17 39 18.4 22.8i 14SP363 W84 C~3cnq 2014 12 24.10560 01 19 13.851 -17 39 18.42 22.7i 14SP363 W84 C~4yUV 2015 08 18.371435 01 31 50.77 -16 56 41.9 22.7r 14SP363 W84 C~352Q 2015 08 18.37196 01 31 50.798 -16 56 41.92 22.6r 14SP363 W84 C~4yUV 2015 08 18.37333 01 31 50.812 -16 56 41.67 24.0g 14SP363 W84 C~4yUV 2015 08 24.396331 01 31 39.18 -17 01 01.5 22.2i 14SP363 W84 C~352Q 2015 08 24.39686 01 31 39.185 -17 01 01.53 22.2i 14SP363 W84 C~4yUV 2015 09 04.36094 01 31 11.50 -17 08 54.6 22.4z 14SP363 W84 C~3cnq 2015 09 04.36094 01 31 11.501 -17 08 54.62 22.2z 14SP363 W84 C~4yUV 2015 10 07.20284 01 29 10.30 -17 29 52.7 22.3i 14SP363 W84 C~3cnq 2015 10 07.20284 01 29 10.300 -17 29 52.68 22.2i 14SP363 W84 C~4yUV 2015 10 07.220359 01 29 10.22 -17 29 53.0 23.4g 14SP363 W84 C~352Q 2015 10 07.22088 01 29 10.221 -17 29 52.99 23.1g 14SP363 W84 C~4yUV 2015 10 07.22227 01 29 10.22 -17 29 53.2 22.7r 14SP363 W84 C~3cnq 2015 10 07.22227 01 29 10.218 -17 29 53.15 22.4r 14SP363 W84 C~4yUV 2015 11 07.13886 01 26 58.87 -17 41 06.1 22.4i 14SP363 W84 C~3cnq 2015 11 07.13886 01 26 58.868 -17 41 06.14 22.5i 14SP363 W84 C~4yUV 2015 11 16.16422 01 26 24.44 -17 42 11.4 21.2z 14SP363 W84 C~3cnq 2015 11 16.16422 01 26 24.440 -17 42 11.44 21.3z 14SP363 W84 C~4yUV 2016 09 30.28185 01 35 22.91 -17 20 59.9 22.4i 14SP363 W84 C~3cnq 2016 09 30.28185 01 35 22.910 -17 20 59.89 22.4i 14SP363 W84 C~4yUV 2016 09 30.28321 01 35 22.90 -17 20 59.9 22.9r 14SP363 W84 C~3cnq 2016 09 30.28321 01 35 22.898 -17 20 59.90 22.8r 14SP363 W84 C~4yUV 2016 09 30.28459 01 35 22.89 -17 21 00.0 23.6g 14SP363 W84 C~3cnq 2016 09 30.28459 01 35 22.886 -17 20 59.99 23.5g 14SP363 W84 C~4yUV 2016 12 05.16558 01 31 07.12 -17 35 55.3 22.7r 14SP363 W84 C~3cnq 2016 12 05.16558 01 31 07.119 -17 35 55.30 22.2r 14SP363 W84 C~4yUV 2016 12 05.16698 01 31 07.12 -17 35 55.3 22.4i 14SP363 W84 C~3cnq 2016 12 05.16698 01 31 07.112 -17 35 55.27 22.0i 14SP363 W84 C~4yUV 2016 12 05.16834 01 31 07.11 -17 35 55.2 23.6g 14SP363 W84 C~3cnq 2016 12 05.16834 01 31 07.107 -17 35 55.23 23.5g 14SP363 W84 C~4yUW 2016 12 07.17436 01 31 02.17 -17 35 30.5 22.2z 14SP363 W84 C~3cnq 2016 12 07.17436 01 31 02.168 -17 35 30.55 22.2z 14SP363 W84 C~4yUW 2017 11 10.140961 01 38 18.42 -17 30 47.8 22.9r 14SP363 W84 C~352Q 2017 11 10.14149 01 38 18.426 -17 30 47.73 22.8r 14SP363 W84 C~4yUW 2017 11 10.142326 01 38 18.42 -17 30 47.6 22.5i 14SP363 W84 C~352Q 2017 11 10.14286 01 38 18.421 -17 30 47.73 22.4i 14SP363 W84 C~4yUW 2017 11 10.143692 01 38 18.41 -17 30 47.6 23.7g 14SP363 W84 C~352Q 2017 11 10.14422 01 38 18.410 -17 30 47.72 23.7g 14SP363 W84 C~4yUW 2017 11 24.103171 01 37 26.55 -17 31 36.4 22.4z 14SP363 W84 C~352Q 2017 11 24.10370 01 37 26.549 -17 31 36.46 22.5z 14SP363 W84 C~4yUW 2017 11 27.065694 01 37 16.82 -17 31 26.4 22.4i 14SP363 W84 C~352Q 2017 11 27.06623 01 37 16.817 -17 31 26.38 22.2i 14SP363 W84 C~4yUW 2017 12 08.063275 01 36 45.53 -17 29 48.0 22.9r 14SP363 W84 C~352Q 2017 12 08.06381 01 36 45.537 -17 29 47.96 22.8r 14SP363 W84 C~4yUW 2017 12 08.064664 01 36 45.52 -17 29 47.8 23.3g 14SP363 W84 C~352Q 2017 12 08.06519 01 36 45.523 -17 29 47.78 23.2g 14SP363 W84 C~4yUW 2018 09 10.28839 01 48 15.199 -16 54 18.71 22.2r 14SP363 W84 C~4yUW 2018 10 21.17169 01 45 34.964 -17 18 28.15 22.5z 14SP363 W84 C~4yUW 2020 10 14.46210 01 57 49.464 -17 00 04.27 22.7w 14SP363 F51 C~4A4f 2020 10 14.47242 01 57 49.437 -17 00 04.80 22.2w 14SP363 F51 C~4A4f 2020 10 14.48274 01 57 49.392 -17 00 05.24 22.5w 14SP363 F51 C~4A4f 2020 10 14.49307 01 57 49.333 -17 00 05.42 22.4w 14SP363 F51 C~4A4f 2023 10 19.444204 02 15 25.847 -16 33 29.87 22.6w 14SP363 F51 C~7Mkv 2023 10 19.456475 02 15 25.830 -16 33 30.07 22.3w 14SP363 F51 C~7Mkv 2023 10 19.468752 02 15 25.753 -16 33 30.54 22.4w 14SP363 F51 C~7Mkv
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 0.14 0.00 0.03
2 0.0002 0.00 -0.04 0.00 0.07
3 0.0004 0.00 -0.01 0.00 -0.06
4 0.0031 0.00 0.09 0.00 -0.02
5 0.0032 0.00 -0.03 0.00 0.06
6 0.0112 0.00 -0.03 0.00 0.03
7 0.0140 0.00 -0.00 0.00 -0.01
8 0.0142 0.00 -0.03 0.00 -0.06
9 0.1779 0.00 0.02 0.00 0.02
10 0.1779 0.00 -0.04 0.00 0.01
11 0.1780 0.00 -0.00 0.00 -0.06
12 0.1780 0.00 -0.03 0.00 -0.10
13 0.1780 0.00 0.03 0.00 -0.00
14 0.1780 0.00 -0.05 0.00 -0.07
15 0.1780 0.00 -0.05 0.00 -0.10
16 0.2353 0.00 -0.09 0.00 0.06
17 0.2353 0.00 -0.03 0.00 0.04
18 0.2680 0.00 -0.03 0.00 -0.00
19 0.2680 0.00 -0.04 0.00 0.02
20 0.9176 0.00 -0.33 0.00 -0.31
21 0.9176 0.00 0.11 0.00 -0.31
22 0.9176 0.00 0.35 0.00 0.00
23 0.9341 0.00 -0.12 0.00 0.09
24 0.9341 0.00 -0.03 0.00 0.08
25 0.9641 0.00 0.07 0.00 0.04
26 0.9641 0.00 0.05 0.00 0.06
27 1.0540 0.00 -0.03 0.00 -0.02
28 1.0540 0.00 -0.03 0.00 -0.04
29 1.0541 0.00 -0.10 0.00 0.21
30 1.0541 0.00 -0.05 0.00 0.24
31 1.0541 0.00 0.03 0.00 0.07
32 1.0541 0.00 -0.00 0.00 0.12
33 1.1387 0.00 0.02 0.00 -0.01
34 1.1387 0.00 0.05 0.00 0.03
35 1.1635 0.00 0.16 0.00 0.00
36 1.1635 0.00 0.16 0.00 0.04
37 2.0371 0.00 0.09 0.00 -0.03
38 2.0371 0.00 0.09 0.00 -0.04
39 2.0372 0.00 -0.01 0.00 0.01
40 2.0372 0.00 0.02 0.00 0.01
41 2.0372 0.00 -0.10 0.00 -0.03
42 2.0372 0.00 -0.04 0.00 -0.04
43 2.2175 0.00 0.03 0.00 0.01
44 2.2175 0.00 0.05 0.00 0.01
45 2.2175 0.00 -0.02 0.00 0.02
46 2.2175 0.00 0.10 0.00 -0.01
47 2.2175 0.00 -0.04 0.00 0.05
48 2.2175 0.00 0.01 0.00 0.08
49 2.2230 0.00 0.07 0.00 -0.03
50 2.2230 0.00 0.10 0.00 0.02
51 3.1483 0.00 -0.04 0.00 -0.08
52 3.1483 0.00 0.09 0.00 -0.01
53 3.1483 0.00 0.05 0.00 0.13
54 3.1483 0.00 0.10 0.00 0.00
55 3.1483 0.00 -0.02 0.00 0.14
56 3.1483 0.00 0.01 0.00 0.03
57 3.1866 0.00 0.04 0.00 -0.03
58 3.1866 0.00 0.05 0.00 -0.09
59 3.1947 0.00 0.04 0.00 -0.04
60 3.1947 0.00 0.03 0.00 -0.02
61 3.2248 0.00 -0.11 0.00 -0.05
62 3.2248 0.00 0.02 0.00 -0.02
63 3.2248 0.00 -0.21 0.00 0.13
64 3.2248 0.00 -0.14 0.00 0.14
65 3.9810 0.00 0.12 0.00 -0.05
66 4.0930 0.00 0.06 0.00 0.02
67 6.0760 0.00 -0.23 0.00 0.16
68 6.0760 0.00 0.05 0.00 -0.06
69 6.0760 0.00 0.06 0.00 -0.20
70 6.0761 0.00 -0.14 0.00 -0.07
71 9.0876 0.00 -0.25 0.00 -0.06
72 9.0876 0.00 0.32 0.00 0.09
73 9.0876 0.00 -0.01 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.
14SP363 quality flag:3 Type: SCATNEAR SCATNEAR SCATNEAR axisobj 63.156 63.155 63.156 ecceobj 0.323 0.323 0.323 incobj 31.196 31.196 31.196 qmin 41.898 42.021 41.552 qmax 84.364 84.472 84.896 amean 62.583 62.646 62.631 amin 61.807 61.814 61.847 amax 63.595 63.604 63.598 emean 0.300 0.300 0.300 emin 0.278 0.275 0.277 emax 0.329 0.329 0.336 imean 30.575 30.599 30.587 imin 29.835 29.884 29.681 imax 31.200 31.271 31.190 excite_mean 0.591 0.591 0.591 fracstop 1.000 1.000 1.000 cjmean 2.849 2.849 2.849 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 178.8 176.7 179.2 kozaiamp 180.0 180.0 179.9