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: 14SK350 # Created Tue Apr 1 01:10:05 2025 # Orbit generated from Bernstein formalism # Fitting 8 observations of 8 # Arc: 60.00d # First observation: 2014/09/21 # Last observation: 2014/11/20 Preliminary a, adot, b, bdot, g, gdot: -0.000002 0.013967 0.000001 -0.003558 0.017531 0.000000 # WARNING Fitting with energy constraint # Chi-squared of fit: 10.14 DOF: 11 RMS: 0.20 # Min/Max residuals: -0.24 0.51 # Exact a, adot, b, bdot, g, gdot: 1.025347E-05 1.300593E-02 -5.442029E-06 -3.289091E-03 1.740005E-02 -8.922046E-03 # Covariance matrix: 4.9995E-13 5.1588E-12 8.2879E-15 -2.2908E-12 2.3812E-12 -7.9747E-11 5.1588E-12 2.5302E-09 5.7852E-12 -6.8918E-10 3.8982E-10 -1.7735E-07 8.2879E-15 5.7852E-12 4.3675E-13 -4.8893E-12 6.7034E-13 -5.3003E-10 -2.2908E-12 -6.8918E-10 -4.8893E-12 2.3678E-10 -1.0712E-10 4.9689E-08 2.3812E-12 3.8982E-10 6.7034E-13 -1.0712E-10 8.3292E-11 -1.6903E-08 -7.9747E-11 -1.7735E-07 -5.3003E-10 4.9689E-08 -1.6903E-08 1.8047E-05 # lat0 lon0 xBary yBary zBary JD0 -10.402865 -29.702555 -0.463670 -0.161202 -0.878815 2456921.559878 # Heliocentric elements and errors Epoch: 2456920.5000 = 2014/09/20 Mean Anomaly: 326.77685 +/- 26.883 Argument of Peri: 318.31957 +/- 6.152 Long of Asc Node: 115.22137 +/- 0.168 Inclination: 17.27258 +/- 0.067 Eccentricity: 0.59186416 +/- 0.2740 Semi-Major Axis: 79.19371093 +/- 40.3262 Time of Perihelion: 2480676.4721 +/- 6344.4 Perihelion: 32.32179145 +/- 27.2343 Aphelion: 126.06563041 +/- 67.7619 Period (y) 704.7649 +/- 538.31 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 50.10306300 +/- 0.0257 Ecliptic Y -28.04677060 +/- 0.0147 Ecliptic Z -10.37777824 +/- 0.0054 Ecliptic XDOT -0.00027120 +/- 0.0006 Ecliptic YDOT 0.00250349 +/- 0.0003 Ecliptic ZDOT -0.00025542 +/- 0.0001 # Distances at JD0 (AU) Heliocenter to KBO 58.34926344 +/- 0.0232 Geocenter to KBO 57.47111442 +/- 0.0301 # Hcoef: 6.71
The following table shows the complete astrometric record for 14SK350. 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 (14SK350) followed by the observatory code and reference code for the source of the astrometry.
2014 09 21.05910 22 25 08.141 -21 04 15.91 24.3r 14SK350 807 C~1x8m 2014 09 21.14703 22 25 07.835 -21 04 17.98 14SK350 807 C~1x8m 2014 09 21.20835 22 25 07.648 -21 04 18.85 14SK350 807 C~1x8m 2014 10 22.09518 22 23 48.044 -21 08 30.69 14SK350 304 C~1x8m 2014 10 22.16844 22 23 47.897 -21 08 30.84 14SK350 304 C~1x8m 2014 10 24.07105 22 23 44.581 -21 08 33.12 14SK350 304 C~1x8m 2014 11 19.05775 22 23 22.430 -21 06 32.75 14SK350 304 C~1x8m 2014 11 20.05427 22 23 22.492 -21 06 22.61 14SK350 304 C~1x8m
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 0.32 0.00 0.51
2 0.0002 -4.75 -0.24 -0.34 -0.16
3 0.0004 -7.50 -0.09 -0.18 -0.23
4 0.0850 -1135.72 0.02 177.16 -0.18
5 0.0852 -1137.69 -0.13 177.78 -0.15
6 0.0904 -1181.66 0.13 192.74 0.07
7 0.1615 -1425.57 0.07 418.72 0.09
8 0.1643 -1421.03 -0.08 427.83 0.05
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.
14SK350 quality flag:0 Type: ERR2LARGE ERR2LARGE ERR2LARGE axisobj 0.000 0.000 0.000 ecceobj -1.000 -1.000 -1.000 incobj -1.000 -1.000 -1.000 qmin 0.000 0.000 0.000 qmax 0.000 0.000 0.000 amean 0.000 0.000 0.000 amin 0.000 0.000 0.000 amax 0.000 0.000 0.000 emean 0.000 0.000 0.000 emin 0.000 0.000 0.000 emax 0.000 0.000 0.000 imean 0.000 0.000 0.000 imin 0.000 0.000 0.000 imax 0.000 0.000 0.000 excite_mean 0.000 0.000 0.000 fracstop 0.000 0.000 0.000 cjmean 0.000 0.000 0.000 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 0.0 0.0 0.0 kozaiamp 0.0 0.0 0.0