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: 14SE350 # Created Fri Nov 1 01:09:47 2024 # Orbit generated from Bernstein formalism # Fitting 10 observations of 10 # Arc: 58.92d # First observation: 2014/09/22 # Last observation: 2014/11/20 Preliminary a, adot, b, bdot, g, gdot: -0.000000 0.025919 0.000002 -0.009541 0.024487 0.000000 # Chi-squared of fit: 5.82 DOF: 14 RMS: 0.13 # Min/Max residuals: -0.30 0.20 # Exact a, adot, b, bdot, g, gdot: 1.531833E-05 2.241516E-02 -6.871567E-06 -8.929732E-03 2.396462E-02 5.880084E-03 # Covariance matrix: 2.5734E-13 1.6749E-11 9.8667E-15 -3.2684E-12 3.0414E-12 -4.6361E-10 1.6749E-11 2.6466E-08 1.6503E-11 -4.4898E-09 3.4973E-09 -9.7750E-07 9.8667E-15 1.6503E-11 2.4001E-13 -4.5072E-12 2.1170E-12 -6.3482E-10 -3.2684E-12 -4.4898E-09 -4.5072E-12 8.0024E-10 -5.9937E-10 1.6412E-07 3.0414E-12 3.4973E-09 2.1170E-12 -5.9937E-10 4.8673E-10 -1.2055E-07 -4.6361E-10 -9.7750E-07 -6.3482E-10 1.6412E-07 -1.2055E-07 3.9380E-05 # lat0 lon0 xBary yBary zBary JD0 -11.363474 -17.527029 -0.281879 -0.190207 -0.947132 2456922.599698 # Heliocentric elements and errors Epoch: 2456920.5000 = 2014/09/20 Mean Anomaly: 43.05968 +/- 9.815 Argument of Peri: 136.17683 +/- 20.744 Long of Asc Node: 137.13094 +/- 0.204 Inclination: 24.33706 +/- 0.160 Eccentricity: 0.28434659 +/- 0.2640 Semi-Major Axis: 50.57358057 +/- 7.6557 Time of Perihelion: 2441207.7479 +/- 311.1 Perihelion: 36.19315526 +/- 14.4328 Aphelion: 64.95400587 +/- 16.5822 Period (y) 359.6613 +/- 81.67 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 40.01474027 +/- 0.0359 Ecliptic Y -12.34049044 +/- 0.0113 Ecliptic Z -8.22209396 +/- 0.0076 Ecliptic XDOT 0.00120289 +/- 0.0007 Ecliptic YDOT 0.00229957 +/- 0.0002 Ecliptic ZDOT -0.00113243 +/- 0.0001 # Distances at JD0 (AU) Heliocenter to KBO 42.67399644 +/- 0.0339 Geocenter to KBO 41.72817650 +/- 0.0384 # Hcoef: 6.87
The following table shows the complete astrometric record for 14SE350. 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 (14SE350) followed by the observatory code and reference code for the source of the astrometry.
2014 09 22.09892 23 13 27.394 -17 21 02.22 22.9r 14SE350 807 C~1x8l 2014 09 22.09893 23 13 27.42 -17 21 02.4 14SE350 W84 C~2JA3 2014 09 22.16880 23 13 27.073 -17 21 04.29 14SE350 807 C~1x8l 2014 09 22.16881 23 13 27.11 -17 21 04.3 23.4V 14SE350 W84 C~2JA3 2014 09 22.24194 23 13 26.767 -17 21 06.24 14SE350 807 C~1x8l 2014 09 22.24195 23 13 26.78 -17 21 06.3 14SE350 W84 C~2JA3 2014 10 22.02537 23 11 32.388 -17 30 51.33 14SE350 304 C~1x8l 2014 10 23.04885 23 11 29.249 -17 31 02.73 14SE350 304 C~1x8l 2014 11 19.02383 23 10 35.144 -17 31 58.16 14SE350 304 C~1x8l 2014 11 20.02368 23 10 34.291 -17 31 51.64 14SE350 304 C~1x8l
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 -0.11 0.00 0.20
2 0.0000 0.27 0.16 -0.31 -0.11
3 0.0002 -5.04 -0.30 -0.07 0.11
4 0.0002 -4.56 0.18 -0.29 -0.11
5 0.0004 -9.84 -0.04 -0.12 0.02
6 0.0004 -9.69 0.11 -0.25 -0.10
7 0.0819 -1744.61 0.09 111.28 0.07
8 0.0847 -1790.37 -0.10 118.54 -0.09
9 0.1586 -2523.46 0.16 372.92 0.11
10 0.1613 -2532.10 -0.15 383.72 -0.09
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.
14SE350 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