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: 15KL199
# Created Wed May 8 01:17:12 2024
# Orbit generated from Bernstein formalism
# Fitting 34 observations of 35
# Arc: 2.10y
# First observation: 2014/05/29
# Last observation: 2016/07/05
Preliminary a, adot, b, bdot, g, gdot:
-0.000019 0.024007 0.000000 0.000561 0.024086 0.000000
# Chi-squared of fit: 20.42 DOF: 62 RMS: 0.14
# Min/Max residuals: -0.32 0.28
# Exact a, adot, b, bdot, g, gdot:
1.544084E-05 2.407418E-02 4.745237E-07 5.632781E-04 2.438478E-02 2.681375E-05
# Covariance matrix:
2.8270E-13 -3.8450E-13 6.1744E-16 -4.6783E-15 -1.6276E-13 -4.7942E-12
-3.8450E-13 8.1409E-13 -1.8908E-15 1.2145E-14 3.9727E-13 1.2770E-11
6.1744E-16 -1.8908E-15 1.8340E-13 -1.2053E-13 3.3951E-17 -3.0546E-14
-4.6783E-15 1.2145E-14 -1.2053E-13 1.0406E-13 8.8917E-15 2.2499E-13
-1.6276E-13 3.9727E-13 3.3951E-17 8.8917E-15 4.1528E-13 7.7527E-12
-4.7942E-12 1.2770E-11 -3.0546E-14 2.2499E-13 7.7527E-12 2.3152E-10
# lat0 lon0 xBary yBary zBary JD0
5.651986 -127.250723 -0.264102 0.096533 -0.974832 2456806.847808
# Heliocentric elements and errors
Epoch: 2456800.5000 = 2014/05/23
Mean Anomaly: 14.41383 +/- 0.906
Argument of Peri: 61.27800 +/- 0.980
Long of Asc Node: 156.35428 +/- 0.008
Inclination: 5.67027 +/- 0.000
Eccentricity: 0.03690507 +/- 0.0002
Semi-Major Axis: 43.53671536 +/- 0.0035
Time of Perihelion: 2452599.4407 +/- 264.2
Perihelion: 41.92998983 +/- 0.0087
Aphelion: 45.14344089 +/- 0.0088
Period (y) 287.2709 +/- 0.03
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -25.08639835 +/- 0.0006
Ecliptic Y -33.42255664 +/- 0.0009
Ecliptic Z 4.03889979 +/- 0.0001
Ecliptic XDOT 0.00214825 +/- 0.0000
Ecliptic YDOT -0.00163719 +/- 0.0000
Ecliptic ZDOT 0.00006336 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 41.98460892 +/- 0.0008
Geocenter to KBO 41.00918212 +/- 0.0011
# Hcoef: 8.61
The following table shows the complete astrometric record for 15KL199. 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 (15KL199) followed by the observatory code and reference code for the source of the astrometry.
2014 05 29.34703 15 27 16.109 -12 59 13.22 24.9r 15KL199 568 C~4n9s 2014 05 29.38590 15 27 15.943 -12 59 12.61 25.0r 15KL199 568 C~4n9s 2014 05 29.42474 15 27 15.721 -12 59 11.92 24.5r 15KL199 568 C~4n9s 2014 05 30.45456 15 27 10.989 -12 58 56.21 24.8r 15KL199 568 C~4n9s 2014 05 31.37090 15 27 06.833 -12 58 42.71 25.4r 15KL199 568 C~4n9s 2015 02 20.65666 15 37 53.262 -13 43 21.33 24.8r 15KL199 568 C~4n9s 2015 03 19.57074 15 37 31.674 -13 38 21.94 25.2r 15KL199 568 C~4n9s 2015 04 12.48811 15 36 20.824 -13 31 39.52 24.5r 15KL199 568 C~4n9s 2015 04 12.52910 15 36 20.641 -13 31 38.57 24.9r 15KL199 568 C~4n9s 2015 05 17.38343 15 33 45.530 -13 20 53.57 24.4r 15KL199 568 C~4n9s 2015 05 17.42514 15 33 45.314 -13 20 52.70 24.4r 15KL199 568 C~4n9s 2015 05 17.46733 15 33 45.120 -13 20 52.23 24.8r 15KL199 568 C~4n9s 2015 05 24.36910 15 33 12.187 -13 18 56.60 24.5r 15KL199 568 C~4n9s 2015 05 24.41533 15 33 11.979 -13 18 55.87 24.6r 15KL199 568 C~4n9s 2015 05 24.45620 15 33 11.746 -13 18 55.16 24.3r 15KL199 568 C~4n9s 2015 05 26.44379 15 33 02.363 -13 18 23.68 24.5r 15KL199 568 C~4n9s 2015 06 18.34328 15 31 21.923 -13 13 25.39 25.0r 15KL199 568 C~4n9s 2015 06 18.38434 15 31 21.764 -13 13 24.86 24.7r 15KL199 568 C~4n9s 2015 06 21.35896 15 31 10.343 -13 12 56.95 24.8r 15KL199 568 C~4n9s 2015 07 10.39102 15 30 10.238 -13 11 06.58 24.1r 15KL199 568 C~4n9s 2015 07 17.34619 15 29 54.858 -13 10 57.81 25.3r 15KL199 568 C~4n9s 2015 07 18.31678 15 29 53.012 -13 10 58.00 24.8r 15KL199 568 C~4n9s 2016 02 12.61062 15 43 10.994 -14 01 12.30 25.3w 15KL199 568 C~4n9s 2016 03 15.61859 15 43 07.069 -13 56 26.56 25.2w 15KL199 568 C~4n9s 2016 04 03.53855 15 42 20.937 -13 51 36.25 25.4w 15KL199 568 C~4n9s 2016 04 03.54259 15 42 20.924 -13 51 36.36 25.6w 15KL199 568 C~4n9s 2016 04 08.58811 15 42 04.054 -13 50 09.10 24.9w 15KL199 568 C~4n9s 2016 04 08.59215 15 42 04.022 -13 50 08.90 25.1w 15KL199 568 C~4n9s 2016 04 29.46970 15 40 39.105 -13 43 50.00 15KL199 568 C~4n9s 2016 04 29.47374 15 40 39.116 -13 43 49.92 25.4w 15KL199 568 C~4n9s 2016 05 04.40478 15 40 16.487 -13 42 19.78 24.8w 15KL199 568 C~4n9s 2016 05 04.40882 15 40 16.479 -13 42 19.81 24.9w 15KL199 568 C~4n9s 2016 07 04.28603 15 35 54.532 -13 29 24.51 24.8w 15KL199 568 C~4n9s 2016 07 05.35431 15 35 51.353 -13 29 19.64 15KL199 568 C~4n9s 2016 07 05.37863 15 35 51.327 -13 29 19.52 25.1w 15KL199 568 C~4n9s
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 0.04 0.00 -0.02
2 0.0001 -2.50 0.27 -0.01 0.05
3 0.0002 -5.82 -0.32 -0.14 -0.00
4 0.0030 -76.72 -0.23 -2.01 0.05
5 0.0055 -138.92 0.22 -3.95 -0.08
6 0.7319 9670.25 0.03 -319.76 -0.01
7 0.8055 9292.85 -0.14 -103.19 0.23
8 0.8710 8191.80 0.25 42.29 0.00
9 0.8711 8188.98 -0.14 42.58 0.11
10 0.9666 5834.65 0.01 126.70 0.00
11 0.9667 5831.38 -0.20 126.78 0.10
12 0.9668 5828.51 0.03 126.56 -0.11
13 0.9857 5333.77 0.06 122.87 0.08
14 0.9858 5330.64 0.28 122.84 0.12
15 0.9859 5327.17 -0.24 122.71 0.04
16 0.9914 5186.57 -0.04 120.19 -0.09
17 1.0541 3690.89 -0.14 54.17 -0.17
18 1.0542 3688.51 -0.09 54.12 -0.03
19 1.0623 3519.90 0.12 40.62 -0.16
20 1.1144 2641.53 0.08 -66.38 -0.26
21 1.1335 2421.55 0.18 -112.79 0.02
22 1.1361 2395.45 -0.02 -119.56 0.00
23 1.7091 14435.80 0.17 -278.22 0.06
24 1.7968 14313.50 0.03 -12.81 0.04
25 1.8486 13589.48 -0.05 114.13 0.03
26 1.8486 13589.32 -0.00 113.97 -0.15
27 1.8624 13328.97 0.15 141.80 0.05
28 1.8624 13328.47 -0.13 141.88 0.12
29 1.9196 12032.25 -0.14 221.87 -0.14
30 1.9196 12032.39 0.28 221.98 -0.04
31 1.9331 11689.57 -0.24 232.40 0.14
32 1.9331 11689.46 -0.06 232.34 0.08
33 2.0998 7786.59 0.13 81.97 -0.12
34 2.1027 7740.33 -0.17 75.63 0.08
35 2.1028 7739.94 ( 0.49) 75.65 ( 0.26)
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.
15KL199 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 43.278 43.289 43.268 ecceobj 0.031 0.031 0.031 incobj 5.679 5.679 5.679 qmin 41.527 41.508 41.513 qmax 45.835 45.878 45.822 amean 43.601 43.612 43.591 amin 43.269 43.280 43.262 amax 43.939 43.951 43.937 emean 0.029 0.029 0.029 emin 0.013 0.013 0.013 emax 0.044 0.044 0.044 imean 5.273 5.270 5.276 imin 4.603 4.604 4.605 imax 5.974 5.969 5.978 excite_mean 0.097 0.097 0.097 fracstop 1.000 1.000 1.000 cjmean 3.086 3.086 3.086 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 176.6 176.8 176.8 kozaiamp 180.0 180.0 180.0