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: 13AS105 # Created Fri Nov 22 02:09:21 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 74 observations of 74 # Arc: 7.43y # First observation: 2007/09/15 # Last observation: 2015/02/20 # Chi-squared of fit: 374.99 DOF: 142 RMS: 0.40 # Min/Max residuals: -1.44 1.38 # Exact a, adot, b, bdot, g, gdot: 3.453499E-05 2.774190E-01 -5.966708E-06 -3.866348E-02 1.279121E-01 -1.683887E-01 # Covariance matrix: 3.9151E-10 3.8308E-07 -8.8974E-10 1.5950E-07 5.8404E-10 -8.0275E-07 3.8308E-07 4.8643E-04 -8.9482E-07 2.0234E-04 5.8608E-07 -1.0170E-03 -8.8974E-10 -8.9482E-07 2.0291E-09 -3.7278E-07 -1.3315E-09 1.8751E-06 1.5950E-07 2.0234E-04 -3.7278E-07 8.7263E-05 2.4405E-07 -4.2536E-04 5.8404E-10 5.8608E-07 -1.3315E-09 2.4405E-07 8.7384E-10 -1.2281E-06 -8.0275E-07 -1.0170E-03 1.8751E-06 -4.2536E-04 -1.2281E-06 2.1379E-03 # lat0 lon0 xBary yBary zBary JD0 -14.564008 -11.890667 -0.071611 -0.252278 -0.971210 2454358.734384 # Heliocentric elements and errors Epoch: 2454358.5000 = 2007/09/15 Mean Anomaly: 340.90893 +/- 0.000 Argument of Peri: 326.16795 +/- 0.000 Long of Asc Node: 106.64886 +/- 0.000 Inclination: 14.57478 +/- 0.015 Eccentricity: 0.64242768 +/- 0.0000 Semi-Major Axis: 16.06323951 +/- 0.0000 Time of Perihelion: 2455605.5274 +/- 0.0 Perihelion: 5.74376981 +/- 0.0000 Aphelion: 26.38270922 +/- 0.0000 Period (y) 64.3810 +/- 0.00 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 8.40016973 +/- 0.0000 Ecliptic Y -1.70031898 +/- 0.0000 Ecliptic Z -1.96590579 +/- 0.0000 Ecliptic XDOT -0.00238741 +/- 0.0000 Ecliptic YDOT 0.00657062 +/- 0.0000 Ecliptic ZDOT 0.00010525 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 8.79326520 +/- 0.0000 Geocenter to KBO 7.81805170 +/- 0.0000 # Hcoef: 12.14
The following table shows the complete astrometric record for 13AS105. 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 (13AS105) followed by the observatory code and reference code for the source of the astrometry.
2007 09 15.23363 23 39 58.82 -18 03 41.4 21.8V 13AS105 G96 C~0o32 2007 09 15.25563 23 39 58.42 -18 03 44.5 21.0V 13AS105 G96 C~0o32 2007 09 15.26076 23 39 58.32 -18 03 44.9 20.9V 13AS105 G96 C~0o32 2007 09 15.26588 23 39 58.24 -18 03 45.9 21.6V 13AS105 G96 C~0o32 2009 10 02.32671 02 31 54.22 -02 26 45.2 20.4V 13AS105 G96 C~0o32 2009 10 02.33288 02 31 54.15 -02 26 46.6 20.9V 13AS105 G96 C~0o32 2009 10 02.33918 02 31 54.01 -02 26 47.8 20.3V 13AS105 G96 C~0o32 2009 10 02.34530 02 31 53.97 -02 26 48.1 20.0V 13AS105 G96 C~0o32 2010 01 15.786762 02 09 48.74 -01 37 48.3 13AS105 C51 S~0Ijq 2010 01 15.91907 02 09 50.13 -01 37 17.7 13AS105 C51 S~0Ijq 2010 01 16.05137 02 09 51.71 -01 36 49.3 13AS105 C51 S~0Ijq 2010 01 16.117587 02 09 52.37 -01 36 33.8 13AS105 C51 S~0Ijq 2010 01 16.183803 02 09 53.15 -01 36 18.5 13AS105 C51 S~0Ijq 2010 01 16.249891 02 09 53.83 -01 36 02.5 13AS105 C51 S~0Ijq 2010 01 16.316108 02 09 54.55 -01 35 46.9 13AS105 C51 S~0Ijq 2010 01 16.382324 02 09 55.28 -01 35 33.5 13AS105 C51 S~0Ijq 2010 01 16.514628 02 09 56.79 -01 35 01.2 13AS105 C51 S~0Ijq 2010 01 16.646933 02 09 58.26 -01 34 30.3 13AS105 C51 S~0Ijq 2010 11 14.36904 04 33 49.53 +10 12 49.8 19.5V 13AS105 703 C~0o32 2010 11 14.37653 04 33 49.35 +10 12 49.8 19.9V 13AS105 703 C~0o32 2010 11 14.38407 04 33 49.10 +10 12 49.3 20.0V 13AS105 703 C~0o32 2010 11 14.39161 04 33 48.92 +10 12 49.7 19.6V 13AS105 703 C~0o32 2010 12 04.27716 04 25 44.43 +10 15 18.0 19.2V 13AS105 G96 C~0o32 2010 12 04.28472 04 25 44.22 +10 15 18.2 19.1V 13AS105 G96 C~0o32 2010 12 04.29226 04 25 44.04 +10 15 18.4 19.2V 13AS105 G96 C~0o32 2010 12 04.29982 04 25 43.86 +10 15 18.5 19.1V 13AS105 G96 C~0o32 2010 12 15.23440 04 21 18.46 +10 23 35.5 19.2V 13AS105 G96 C~0o32 2010 12 15.24060 04 21 18.32 +10 23 35.9 19.3V 13AS105 G96 C~0o33 2010 12 15.24686 04 21 18.18 +10 23 36.4 19.2V 13AS105 G96 C~0o33 2010 12 15.25317 04 21 18.03 +10 23 36.6 19.2V 13AS105 G96 C~0o33 2012 01 05.15701 06 49 43.29 +21 29 09.5 20.1V 13AS105 691 C~0o33 2012 01 05.17480 06 49 42.83 +21 29 11.2 20.2V 13AS105 691 C~0o33 2012 01 05.19259 06 49 42.34 +21 29 13.7 20.3V 13AS105 691 C~0o33 2013 01 07.35153 09 03 09.86 +23 19 51.4 20.6V 13AS105 691 C~0nie 2013 01 07.36924 09 03 09.55 +23 19 54.1 21.2V 13AS105 691 C~0nie 2013 01 07.38695 09 03 09.22 +23 19 58.0 20.9V 13AS105 691 C~0nie 2013 01 15.07146 09 00 34.55 +23 41 19.4 20.2R 13AS105 J04 C~0nie 2013 01 15.08303 09 00 34.30 +23 41 21.2 20.6R 13AS105 J04 C~0nie 2013 01 15.09461 09 00 34.03 +23 41 23.1 20.6R 13AS105 J04 C~0nie 2013 01 15.10618 09 00 33.80 +23 41 25.2 20.9R 13AS105 J04 C~0nie 2013 01 15.93094 09 00 16.24 +23 43 41.6 20.2R 13AS105 J04 C~0nie 2013 01 15.95115 09 00 15.80 +23 43 44.9 20.0R 13AS105 J04 C~0nie 2013 01 15.97141 09 00 15.36 +23 43 48.5 20.0R 13AS105 J04 C~0nie 2013 01 16.272865 09 00 08.83 +23 44 38.3 20.4R 13AS105 711 C~0nie 2013 01 16.276500 09 00 08.75 +23 44 38.9 20.4R 13AS105 711 C~0nie 2013 01 16.280126 09 00 08.67 +23 44 39.6 20.4R 13AS105 711 C~0nie 2013 01 16.283752 09 00 08.61 +23 44 40.4 20.2R 13AS105 711 C~0nie 2013 01 16.287377 09 00 08.53 +23 44 41.0 20.5R 13AS105 711 C~0nie 2013 01 16.58764 09 00 01.97 +23 45 31.1 20.1R 13AS105 F65 C~0nie 2013 01 16.59427 09 00 01.83 +23 45 32.2 19.8R 13AS105 F65 C~0nie 2013 01 16.60027 09 00 01.68 +23 45 33.4 20.0R 13AS105 F65 C~0nie 2013 01 17.31231 08 59 46.39 +23 47 30.2 13AS105 H06 C~0nie 2013 01 17.31531 08 59 46.32 +23 47 31.0 20.8V 13AS105 H06 C~0nie 2013 01 17.33086 08 59 45.94 +23 47 33.6 20.8V 13AS105 G84 C~0nie 2013 01 17.35751 08 59 45.35 +23 47 38.0 20.4V 13AS105 G84 C~0nie 2013 01 17.38235 08 59 44.78 +23 47 41.9 20.5V 13AS105 G84 C~0nie 2013 01 18.329896 08 59 24.09 +23 50 18.5 20.4V 13AS105 H21 C~0nie 2013 01 18.336170 08 59 23.94 +23 50 19.2 20.5V 13AS105 H21 C~0nif 2013 01 18.342630 08 59 23.80 +23 50 19.9 20.7V 13AS105 H21 C~0nif 2013 01 18.348799 08 59 23.65 +23 50 20.9 20.4V 13AS105 H21 C~0nif 2013 01 20.27530 08 58 41.06 +23 55 37.3 20.4V 13AS105 691 C~0o33 2013 01 20.29299 08 58 40.63 +23 55 40.1 20.6V 13AS105 691 C~0o33 2013 01 20.31069 08 58 40.25 +23 55 43.0 20.5V 13AS105 691 C~0o33 2013 01 22.27175 08 57 56.26 +24 01 00.8 20.2V 13AS105 G96 C~0o33 2013 01 22.27889 08 57 56.08 +24 01 02.0 20.4V 13AS105 G96 C~0o33 2013 01 22.28602 08 57 55.90 +24 01 02.5 20.2V 13AS105 G96 C~0o33 2013 01 22.29317 08 57 55.76 +24 01 04.4 20.5V 13AS105 G96 C~0o33 2013 02 19.27066 08 47 30.58 +25 05 31.8 20.5V 13AS105 G96 C~0p6Y 2013 02 19.28150 08 47 30.37 +25 05 32.1 19.9V 13AS105 G96 C~0p6Y 2013 02 19.29228 08 47 30.15 +25 05 33.4 20.4V 13AS105 G96 C~0p6Y 2013 02 19.30297 08 47 29.94 +25 05 34.4 20.3V 13AS105 G96 C~0p6Y 2015 02 20.56929 11 26 10.563 +18 29 36.98 22.1w 13AS105 F51 C~1LLe 2015 02 20.58286 11 26 10.331 +18 29 38.61 22.3w 13AS105 F51 C~1LLe 2015 02 20.59647 11 26 10.137 +18 29 40.99 21.8w 13AS105 F51 C~1LLe
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 -0.15 0.00 0.20
2 0.0001 0.00 0.05 0.00 0.01
3 0.0001 0.00 -0.01 0.00 0.29
4 0.0001 0.00 0.24 0.00 -0.04
5 2.0482 0.00 -0.28 0.00 0.41
6 2.0482 0.00 0.18 0.00 -0.12
7 2.0482 0.00 -0.37 0.00 -0.44
8 2.0482 0.00 0.54 0.00 0.12
9 2.3369 0.00 -0.10 0.00 1.24
10 2.3373 0.00 -0.80 0.00 1.38
11 2.3376 0.00 1.21 0.00 -0.72
12 2.3378 0.00 0.19 0.00 -0.51
13 2.3380 0.00 0.93 0.00 -0.51
14 2.3382 0.00 0.15 0.00 0.21
15 2.3384 0.00 -0.09 0.00 0.49
16 2.3385 0.00 -0.21 0.00 -1.44
17 2.3389 0.00 0.18 0.00 0.19
18 2.3393 0.00 -0.17 0.00 0.37
19 3.1653 0.00 0.32 0.00 0.48
20 3.1653 0.00 0.22 0.00 0.58
21 3.1654 0.00 -0.92 0.00 0.19
22 3.1654 0.00 -1.01 0.00 0.69
23 3.2198 0.00 0.37 0.00 -0.12
24 3.2199 0.00 0.14 0.00 -0.15
25 3.2199 0.00 0.34 0.00 -0.18
26 3.2199 0.00 0.56 0.00 -0.31
27 3.2498 0.00 0.11 0.00 -0.23
28 3.2498 0.00 0.22 0.00 -0.20
29 3.2499 0.00 0.35 0.00 -0.08
30 3.2499 0.00 0.35 0.00 -0.26
31 4.3064 0.00 -0.06 0.00 -0.03
32 4.3065 0.00 -0.02 0.00 -0.54
33 4.3065 0.00 -0.41 0.00 -0.25
34 5.3145 0.00 -0.72 0.00 0.03
35 5.3145 0.00 -0.21 0.00 -0.22
36 5.3146 0.00 0.01 0.00 0.72
37 5.3356 0.00 0.38 0.00 0.19
38 5.3357 0.00 0.42 0.00 0.06
39 5.3357 0.00 0.16 0.00 0.03
40 5.3357 0.00 0.50 0.00 0.20
41 5.3380 0.00 -0.09 0.00 -0.10
42 5.3380 0.00 -0.09 0.00 -0.21
43 5.3381 0.00 -0.06 0.00 -0.02
44 5.3389 0.00 -0.41 0.00 -0.25
45 5.3389 0.00 -0.41 0.00 -0.26
46 5.3389 0.00 -0.41 0.00 -0.17
47 5.3389 0.00 -0.11 0.00 0.03
48 5.3390 0.00 -0.11 0.00 0.02
49 5.3398 0.00 -0.06 0.00 0.21
50 5.3398 0.00 0.04 0.00 0.23
51 5.3398 0.00 -0.22 0.00 0.45
52 5.3418 0.00 0.67 0.00 -0.33
53 5.3418 0.00 0.62 0.00 -0.02
54 5.3418 0.00 0.00 0.00 -0.00
55 5.3419 0.00 0.07 0.00 -0.01
56 5.3420 0.00 -0.16 0.00 -0.21
57 5.3445 0.00 0.31 0.00 0.37
58 5.3446 0.00 0.17 0.00 0.04
59 5.3446 0.00 0.25 0.00 -0.31
60 5.3446 0.00 0.07 0.00 -0.32
61 5.3499 0.00 -0.11 0.00 0.28
62 5.3499 0.00 -0.51 0.00 0.17
63 5.3500 0.00 -0.14 0.00 0.17
64 5.3553 0.00 0.47 0.00 -0.07
65 5.3554 0.00 0.25 0.00 -0.04
66 5.3554 0.00 0.02 0.00 -0.69
67 5.3554 0.00 0.40 0.00 0.05
68 5.4320 0.00 -0.47 0.00 0.84
69 5.4320 0.00 -0.29 0.00 -0.02
70 5.4321 0.00 -0.27 0.00 0.13
71 5.4321 0.00 -0.13 0.00 -0.00
72 7.4342 0.00 -0.11 0.00 0.17
73 7.4342 0.00 -0.16 0.00 -0.18
74 7.4343 0.00 0.37 0.00 0.22
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.
13AS105 quality flag:3 Type: CENTAURR CENTAURR CENTAURR axisobj 16.106 16.106 16.107 ecceobj 0.643 0.643 0.643 incobj 14.587 14.587 14.587 qmin 5.742 5.742 5.742 qmax 26.471 26.470 36.625 amean 15.224 14.122 17.154 amin 14.342 11.824 15.078 amax 16.106 16.106 21.283 emean 0.620 0.581 0.649 emin 0.596 0.497 0.596 emax 0.643 0.643 0.721 imean 13.144 12.212 13.022 imin 13.008 10.894 12.662 imax 13.280 13.614 13.630 excite_mean 0.660 0.619 0.687 fracstop 0.000 0.001 0.002 cjmean 3.066 3.236 2.885 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 328.9 213.2 124.2 kozaiamp 2.9 171.6 174.8