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: 14FO69 # Created Sun Nov 24 02:09:49 2024 # Orbit generated from Bernstein formalism # Fitting 10 observations of 10 # Arc: 3.97y # First observation: 2014/03/24 # Last observation: 2018/03/12 Preliminary a, adot, b, bdot, g, gdot: 0.000003 0.014068 0.000004 -0.000061 0.018222 0.000000 # Chi-squared of fit: 2.87 DOF: 14 RMS: 0.09 # Min/Max residuals: -0.17 0.18 # Exact a, adot, b, bdot, g, gdot: 1.315243E-05 1.385360E-02 3.590648E-07 -5.708005E-05 1.778770E-02 -4.087172E-03 # Covariance matrix: 5.6527E-13 6.8627E-12 9.4931E-14 -8.7367E-14 1.5232E-11 1.3032E-10 6.8627E-12 5.1342E-10 6.7235E-12 -6.1872E-12 1.0910E-09 9.5605E-09 9.4931E-14 6.7235E-12 4.6682E-13 -1.9076E-13 1.4305E-11 1.2523E-10 -8.7367E-14 -6.1872E-12 -1.9076E-13 1.2595E-13 -1.3164E-11 -1.1524E-10 1.5232E-11 1.0910E-09 1.4305E-11 -1.3164E-11 2.3205E-09 2.0320E-08 1.3032E-10 9.5605E-09 1.2523E-10 -1.1524E-10 2.0320E-08 1.7805E-07 # lat0 lon0 xBary yBary zBary JD0 -16.331133 -156.176713 0.346962 -0.262294 -0.895589 2456740.734038 # Heliocentric elements and errors Epoch: 2456740.5000 = 2014/03/24 Mean Anomaly: 277.05575 +/- 6.098 Argument of Peri: 24.84057 +/- 3.078 Long of Asc Node: 294.21179 +/- 0.031 Inclination: 16.06875 +/- 0.001 Eccentricity: 0.28973755 +/- 0.0239 Semi-Major Axis: 54.55511923 +/- 1.2111 Time of Perihelion: 2490651.0996 +/- 2222.5 Perihelion: 38.74845286 +/- 1.5603 Aphelion: 70.36178560 +/- 2.0334 Period (y) 402.9596 +/- 13.42 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X -50.34856205 +/- 0.1337 Ecliptic Y -21.84964261 +/- 0.0590 Ecliptic Z -15.80801002 +/- 0.0428 Ecliptic XDOT 0.00141020 +/- 0.0001 Ecliptic YDOT -0.00170896 +/- 0.0000 Ecliptic ZDOT 0.00016859 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 57.11635286 +/- 0.1205 Geocenter to KBO 56.21863129 +/- 0.1522 # Hcoef: 7.09
The following table shows the complete astrometric record for 14FO69. 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 (14FO69) followed by the observatory code and reference code for the source of the astrometry.
2014 03 24.23326 13 02 04.726 -24 20 28.76 24.6r 14FO69 807 C~1MjU 2014 03 24.30306 13 02 04.495 -24 20 27.64 14FO69 807 C~1MjU 2014 03 25.30436 13 02 00.856 -24 20 13.13 14FO69 807 C~1MjU 2015 04 20.24304 13 03 38.030 -24 31 07.26 14FO69 304 C~2b7w 2016 05 03.05873 13 06 04.995 -24 44 48.21 14FO69 304 C~2b7w 2016 05 03.27716 13 06 04.226 -24 44 42.55 14FO69 304 C~2b7w 2018 03 11.35232 13 15 57.738 -25 38 43.63 24.5r 14FO69 304 C~2b7w 2018 03 11.39089 13 15 57.618 -25 38 43.35 14FO69 304 C~2b7w 2018 03 12.35759 13 15 54.480 -25 38 36.65 14FO69 304 C~2b7w 2018 03 12.38577 13 15 54.385 -25 38 36.23 14FO69 304 C~2b7w
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 -0.17 0.00 -0.08
2 0.0002 -3.34 0.11 -0.23 0.16
3 0.0029 -54.73 0.10 -6.80 -0.02
4 1.0733 1423.13 -0.08 -78.44 -0.02
5 2.1104 3588.67 0.15 -41.64 -0.01
6 2.1110 3576.81 -0.10 -40.55 -0.07
7 3.9647 12273.30 -0.07 63.49 -0.08
8 3.9648 12271.68 0.01 63.14 -0.03
9 3.9675 12229.70 0.07 53.38 -0.01
10 3.9676 12228.34 -0.02 53.29 0.18
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.
14FO69 quality flag:1 Type: SCATNEAR SCATNEAR 9:4EEEEE axisobj 54.205 58.221 51.310 ecceobj 0.294 0.363 0.234 incobj 16.069 16.070 16.067 qmin 37.672 36.160 38.479 qmax 72.358 82.322 65.520 amean 54.639 58.611 51.700 amin 54.090 57.889 51.207 amax 55.299 59.562 52.291 emean 0.295 0.366 0.228 emin 0.282 0.350 0.196 emax 0.309 0.383 0.254 imean 17.500 17.385 17.709 imin 17.208 16.737 16.917 imax 17.817 18.230 18.790 excite_mean 0.422 0.473 0.381 fracstop 1.000 1.000 1.000 cjmean 3.006 2.991 3.012 libcent 0 -180.0 -180.0 178.6 libamp 0 -180.0 -180.0 99.6 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 172.4 175.8 172.5 kozaiamp 180.0 180.0 180.0