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: 14SX349 # Created Sun Dec 22 02:10:02 2024 # Orbit generated from Bernstein formalism # Fitting 12 observations of 12 # Arc: 1.07y # First observation: 2014/09/19 # Last observation: 2015/10/16 Preliminary a, adot, b, bdot, g, gdot: -0.000005 0.013656 -0.000001 0.001738 0.018210 0.000000 # Chi-squared of fit: 2.85 DOF: 18 RMS: 0.09 # Min/Max residuals: -0.17 0.17 # Exact a, adot, b, bdot, g, gdot: 1.133678E-05 1.378709E-02 1.163903E-06 1.750638E-03 1.842326E-02 3.604254E-03 # Covariance matrix: 2.3930E-13 2.7555E-13 -1.8433E-14 9.0555E-14 5.5415E-13 3.9300E-11 2.7555E-13 9.8860E-11 -1.7190E-12 2.7568E-11 4.6271E-11 1.0883E-08 -1.8433E-14 -1.7190E-12 1.9538E-13 -6.6102E-13 -8.5923E-13 -1.8920E-10 9.0555E-14 2.7568E-11 -6.6102E-13 8.6066E-12 1.2836E-11 3.0667E-09 5.5415E-13 4.6271E-11 -8.5923E-13 1.2836E-11 2.3395E-11 5.0836E-09 3.9300E-11 1.0883E-08 -1.8920E-10 3.0667E-09 5.0836E-09 1.2101E-06 # lat0 lon0 xBary yBary zBary JD0 -9.829637 -21.626723 -0.301392 -0.163939 -0.946961 2456919.570608 # Heliocentric elements and errors Epoch: 2456910.5000 = 2014/09/10 Mean Anomaly: 107.04770 +/- 11.404 Argument of Peri: 171.37430 +/- 8.545 Long of Asc Node: 31.45483 +/- 0.021 Inclination: 12.06772 +/- 0.003 Eccentricity: 0.29700482 +/- 0.0442 Semi-Major Axis: 47.79246998 +/- 1.3551 Time of Perihelion: 2421025.5393 +/- 3505.1 Perihelion: 33.59787592 +/- 2.3179 Aphelion: 61.98706404 +/- 2.7485 Period (y) 330.4056 +/- 14.05 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 50.71977569 +/- 0.0131 Ecliptic Y -19.78345390 +/- 0.0052 Ecliptic Z -9.26644442 +/- 0.0024 Ecliptic XDOT 0.00128234 +/- 0.0002 Ecliptic YDOT 0.00168922 +/- 0.0001 Ecliptic ZDOT 0.00016501 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 55.22452070 +/- 0.0121 Geocenter to KBO 54.27919643 +/- 0.0143 # Hcoef: 6.96
The following table shows the complete astrometric record for 14SX349. 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 (14SX349) followed by the observatory code and reference code for the source of the astrometry.
2014 09 19.06983 22 55 23.592 -17 31 21.72 24.0r 14SX349 807 C~1x8l 2014 09 19.06984 22 55 23.58 -17 31 21.9 24.7V 14SX349 W84 C~2JA3 2014 09 19.14530 22 55 23.304 -17 31 23.13 14SX349 807 C~1x8l 2014 09 19.14530 22 55 23.31 -17 31 23.1 14SX349 W84 C~2JA3 2014 09 19.22379 22 55 23.027 -17 31 24.36 14SX349 807 C~1x8l 2014 09 19.22379 22 55 23.03 -17 31 24.5 14SX349 W84 C~2JA3 2014 10 22.11046 22 53 41.251 -17 37 17.22 14SX349 304 C~1x8l 2014 10 22.18054 22 53 41.089 -17 37 17.43 14SX349 304 C~1x8l 2014 11 19.04182 22 52 58.321 -17 36 04.90 14SX349 304 C~1x8l 2014 11 20.03527 22 52 57.767 -17 35 55.60 14SX349 304 C~1x8l 2015 10 16.22317 22 56 48.584 -17 13 03.46 14SX349 304 C~1x8l 2015 10 16.24767 22 56 48.534 -17 13 03.36 14SX349 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 0.10 0.00 0.07
2 0.0000 -0.23 -0.13 -0.10 -0.03
3 0.0002 -4.34 -0.11 0.30 0.01
4 0.0002 -4.25 -0.02 0.29 0.00
5 0.0004 -8.49 0.04 0.55 -0.12
6 0.0004 -8.47 0.06 0.70 0.03
7 0.0905 -1487.12 -0.03 238.14 -0.05
8 0.0907 -1489.34 0.11 238.84 -0.05
9 0.1669 -2025.69 -0.10 541.36 0.09
10 0.1697 -2029.42 0.07 552.99 0.06
11 1.0737 1547.94 -0.17 539.09 -0.08
12 1.0737 1547.32 0.17 539.47 0.07
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.
14SX349 quality flag:1 Type: 2:1E CENTAURR SCATNEAR axisobj 48.043 54.271 45.932 ecceobj 0.292 0.436 0.208 incobj 12.041 12.035 12.047 qmin 32.810 29.092 34.842 qmax 63.716 78.179 57.158 amean 47.796 50.885 45.804 amin 47.153 46.678 45.272 amax 48.544 54.393 46.364 emean 0.281 0.417 0.216 emin 0.249 0.358 0.198 emax 0.313 0.439 0.237 imean 12.401 10.072 11.441 imin 10.571 9.552 10.277 imax 13.896 11.939 12.663 excite_mean 0.354 0.452 0.294 fracstop 1.000 0.093 1.000 cjmean 2.991 2.915 3.017 libcent 0 92.8 -180.0 -180.0 libamp 0 61.6 -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 211.9 267.0 181.2 kozaiamp 179.9 81.0 180.0