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: 14MH105
# Created Fri May 3 01:16:03 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 39 observations of 39
# Arc: 6.14y
# First observation: 2014/06/25
# Last observation: 2020/08/15
# Chi-squared of fit: 2.30 DOF: 72 RMS: 0.04
# Min/Max residuals: -0.11 0.15
# Exact a, adot, b, bdot, g, gdot:
1.342463E-05 1.848064E-02 1.127588E-06 1.474696E-03 2.153992E-02 -3.276507E-03
# Covariance matrix:
2.4046E-13 -1.3455E-13 5.8723E-15 -8.3310E-15 -1.0252E-13 -8.3201E-13
-1.3455E-13 1.6072E-13 -8.6717E-15 1.2316E-14 1.6872E-13 1.2284E-12
5.8723E-15 -8.6717E-15 1.6987E-13 -3.1179E-14 -9.4808E-15 -6.9291E-14
-8.3310E-15 1.2316E-14 -3.1179E-14 7.9754E-15 1.3625E-14 9.8400E-14
-1.0252E-13 1.6872E-13 -9.4808E-15 1.3625E-14 3.9879E-13 1.3394E-12
-8.3201E-13 1.2284E-12 -6.9291E-14 9.8400E-14 1.3394E-12 9.8153E-12
# lat0 lon0 xBary yBary zBary JD0
1.847950 -79.015352 0.130637 0.032621 -1.009397 2456833.840208
# Heliocentric elements and errors
Epoch: 2456834.5000 = 2014/06/26
Mean Anomaly: 253.72527 +/- 0.046
Argument of Peri: 147.62921 +/- 0.034
Long of Asc Node: 259.29731 +/- 0.001
Inclination: 4.91872 +/- 0.000
Eccentricity: 0.19573558 +/- 0.0001
Semi-Major Axis: 43.64412459 +/- 0.0049
Time of Perihelion: 2487924.0635 +/- 18.4
Perihelion: 35.10141645 +/- 0.0066
Aphelion: 52.18683272 +/- 0.0079
Period (y) 288.3347 +/- 0.05
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X 8.90441546 +/- 0.0003
Ecliptic Y -46.56559911 +/- 0.0013
Ecliptic Z 1.49720488 +/- 0.0000
Ecliptic XDOT 0.00222035 +/- 0.0000
Ecliptic YDOT 0.00085832 +/- 0.0000
Ecliptic ZDOT 0.00017404 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 47.43306776 +/- 0.0013
Geocenter to KBO 46.42555872 +/- 0.0014
# Hcoef: 8.73
The following table shows the complete astrometric record for 14MH105. 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 (14MH105) followed by the observatory code and reference code for the source of the astrometry.
2014 06 25.33943 18 47 07.739 -21 08 35.46 25.0r 14MH105 266 C~7B1v 2014 06 25.45033 18 47 07.223 -21 08 35.93 25.0r 14MH105 266 C~7B1v 2014 06 25.56643 18 47 06.683 -21 08 36.39 25.0r 14MH105 266 C~7B1v 2014 06 27.34219 18 46 58.550 -21 08 43.70 25.5r 14MH105 266 C~7B1v 2014 06 27.36877 18 46 58.426 -21 08 43.81 25.5r 14MH105 266 C~7B1v 2014 06 27.39518 18 46 58.302 -21 08 43.93 25.5r 14MH105 266 C~7B1v 2016 06 05.44847 18 57 32.340 -20 45 47.30 25.3r 14MH105 266 C~7B1v 2016 06 05.52553 18 57 32.029 -20 45 47.57 25.3r 14MH105 266 C~7B1v 2016 06 05.60261 18 57 31.717 -20 45 47.83 25.3r 14MH105 266 C~7B1v 2017 07 20.25325 18 58 46.315 -20 38 06.52 25.4r 14MH105 266 C~7B1v 2017 07 20.39364 18 58 45.678 -20 38 07.41 25.4r 14MH105 266 C~7B1v 2017 07 20.53088 18 58 45.055 -20 38 08.24 25.4r 14MH105 266 C~7B1v 2017 07 21.24888 18 58 41.875 -20 38 12.69 25.3r 14MH105 266 C~7B1v 2017 07 21.40707 18 58 41.160 -20 38 13.69 25.3r 14MH105 266 C~7B1v 2017 07 21.50353 18 58 40.724 -20 38 14.28 25.3r 14MH105 266 C~7B1v 2020 05 28.44674 19 16 18.385 -19 55 34.87 24.8r 14MH105 266 C~7B1v 2020 05 28.50129 19 16 18.200 -19 55 35.06 24.8r 14MH105 266 C~7B1v 2020 05 28.55756 19 16 18.009 -19 55 35.24 24.8r 14MH105 266 C~7B1v 2020 05 30.43935 19 16 11.667 -19 55 41.65 25.4r 14MH105 266 C~7B1v 2020 05 30.53044 19 16 11.347 -19 55 41.98 25.4r 14MH105 266 C~7B1v 2020 05 30.61862 19 16 11.037 -19 55 42.29 25.4r 14MH105 266 C~7B1v 2020 06 01.43269 19 16 04.722 -19 55 49.03 25.8r 14MH105 266 C~7B1v 2020 06 01.47325 19 16 04.576 -19 55 49.19 25.8r 14MH105 266 C~7B1v 2020 06 01.60571 19 16 04.095 -19 55 49.70 25.8r 14MH105 266 C~7B1v 2020 06 20.45583 19 14 48.673 -19 57 24.43 25.4r 14MH105 266 C~7B1v 2020 06 20.52860 19 14 48.350 -19 57 24.88 25.4r 14MH105 266 C~7B1v 2020 06 20.62233 19 14 47.934 -19 57 25.43 25.4r 14MH105 266 C~7B1v 2020 06 22.44948 19 14 39.909 -19 57 36.75 25.4r 14MH105 266 C~7B1v 2020 06 22.52092 19 14 39.588 -19 57 37.20 25.4r 14MH105 266 C~7B1v 2020 06 22.59118 19 14 39.272 -19 57 37.63 25.4r 14MH105 266 C~7B1v 2020 06 25.44823 19 14 26.535 -19 57 55.98 25.1r 14MH105 266 C~7B1v 2020 06 25.53213 19 14 26.151 -19 57 56.53 25.1r 14MH105 266 C~7B1v 2020 06 25.61487 19 14 25.773 -19 57 57.05 25.1r 14MH105 266 C~7B1v 2020 08 13.24332 19 10 52.191 -20 04 00.75 25.4r 14MH105 266 C~7B1v 2020 08 13.33331 19 10 51.854 -20 04 01.42 25.4r 14MH105 266 C~7B1v 2020 08 13.42301 19 10 51.517 -20 04 02.06 25.4r 14MH105 266 C~7B1v 2020 08 15.24331 19 10 44.944 -20 04 15.25 25.6r 14MH105 266 C~7B1v 2020 08 15.33985 19 10 44.592 -20 04 15.95 25.6r 14MH105 266 C~7B1v 2020 08 15.42111 19 10 44.297 -20 04 16.53 25.6r 14MH105 266 C~7B1v
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 0.03 0.00 -0.01
2 0.0003 0.00 0.03 0.00 -0.01
3 0.0006 0.00 0.03 0.00 -0.01
4 0.0055 0.00 -0.00 0.00 -0.02
5 0.0056 0.00 -0.00 0.00 -0.01
6 0.0056 0.00 -0.01 0.00 -0.02
7 1.9469 0.00 -0.04 0.00 0.00
8 1.9471 0.00 -0.03 0.00 0.00
9 1.9473 0.00 -0.03 0.00 -0.00
10 3.0689 0.00 0.00 0.00 0.02
11 3.0693 0.00 0.01 0.00 0.02
12 3.0697 0.00 0.01 0.00 0.02
13 3.0716 0.00 0.02 0.00 0.03
14 3.0721 0.00 0.01 0.00 0.04
15 3.0723 0.00 0.01 0.00 0.03
16 5.9250 0.00 -0.10 0.00 0.03
17 5.9252 0.00 -0.11 0.00 0.02
18 5.9253 0.00 -0.10 0.00 0.03
19 5.9305 0.00 -0.03 0.00 -0.01
20 5.9307 0.00 -0.03 0.00 -0.00
21 5.9309 0.00 -0.03 0.00 -0.00
22 5.9359 0.00 0.14 0.00 -0.06
23 5.9360 0.00 0.15 0.00 -0.06
24 5.9364 0.00 0.15 0.00 -0.06
25 5.9880 0.00 -0.03 0.00 0.02
26 5.9882 0.00 -0.02 0.00 0.01
27 5.9885 0.00 -0.01 0.00 0.01
28 5.9935 0.00 -0.04 0.00 0.03
29 5.9937 0.00 -0.02 0.00 0.02
30 5.9938 0.00 -0.02 0.00 0.02
31 6.0017 0.00 -0.02 0.00 0.02
32 6.0019 0.00 -0.02 0.00 0.02
33 6.0021 0.00 -0.03 0.00 0.02
34 6.1353 0.00 -0.04 0.00 -0.02
35 6.1355 0.00 -0.03 0.00 -0.02
36 6.1358 0.00 -0.04 0.00 -0.02
37 6.1407 0.00 0.00 0.00 -0.04
38 6.1410 0.00 0.00 0.00 -0.04
39 6.1412 0.00 0.01 0.00 -0.04
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.
14MH105 quality flag:3 Type: 7:4EEE 7:4EEE 7:4EEE axisobj 43.689 43.689 43.689 ecceobj 0.199 0.199 0.199 incobj 4.924 4.924 4.924 qmin 34.828 34.818 34.791 qmax 53.281 53.324 53.349 amean 43.727 43.727 43.726 amin 43.183 43.205 43.206 amax 44.289 44.311 44.331 emean 0.191 0.191 0.191 emin 0.179 0.178 0.177 emax 0.204 0.204 0.203 imean 7.075 7.073 7.056 imin 5.687 5.699 5.705 imax 7.963 7.956 7.972 excite_mean 0.228 0.228 0.227 fracstop 1.000 1.000 1.000 cjmean 3.035 3.035 3.035 libcent 0 180.5 177.8 177.4 libamp 0 144.6 142.8 142.0 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 179.0 177.9 177.2 kozaiamp 180.0 180.0 180.0