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: 14YK92 # Created Fri Apr 26 01:16:55 2024 # Orbit generated from Bernstein formalism # Fitting 14 observations of 14 # Arc: 1.15y # First observation: 2013/12/24 # Last observation: 2015/02/16 Preliminary a, adot, b, bdot, g, gdot: 0.000009 0.026213 0.000000 -0.010628 0.027036 0.000000 # Chi-squared of fit: 3.17 DOF: 22 RMS: 0.08 # Min/Max residuals: -0.16 0.20 # Exact a, adot, b, bdot, g, gdot: 1.538490E-05 2.624738E-02 -6.017325E-06 -1.062901E-02 2.697440E-02 1.155269E-03 # Covariance matrix: 1.4056E-12 7.0778E-12 -6.6548E-14 -3.3333E-12 7.9064E-12 3.2187E-10 7.0778E-12 9.1956E-11 -7.5566E-13 -3.9143E-11 9.3180E-11 3.7684E-09 -6.6548E-14 -7.5566E-13 7.4905E-13 -3.6742E-13 -7.4805E-13 -3.1908E-11 -3.3333E-12 -3.9143E-11 -3.6742E-13 1.7551E-11 -4.0001E-11 -1.6170E-09 7.9064E-12 9.3180E-11 -7.4805E-13 -4.0001E-11 9.5535E-11 3.8403E-09 3.2187E-10 3.7684E-09 -3.1908E-11 -1.6170E-09 3.8403E-09 1.5598E-07 # lat0 lon0 xBary yBary zBary JD0 -52.741462 89.151607 -0.055912 -0.779632 -0.593217 2456650.826638 # Heliocentric elements and errors Epoch: 2456650.5000 = 2013/12/24 Mean Anomaly: 28.20411 +/- 9.091 Argument of Peri: 221.33197 +/- 10.692 Long of Asc Node: 206.53818 +/- 0.019 Inclination: 54.78416 +/- 0.004 Eccentricity: 0.06716180 +/- 0.0077 Semi-Major Axis: 39.99806410 +/- 0.0213 Time of Perihelion: 2449411.6969 +/- 2333.2 Perihelion: 37.31172227 +/- 0.3069 Aphelion: 42.68440594 +/- 0.3071 Period (y) 252.9686 +/- 0.20 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 0.28940861 +/- 0.0002 Ecliptic Y 23.42401168 +/- 0.0081 Ecliptic Z -29.50637864 +/- 0.0107 Ecliptic XDOT -0.00268152 +/- 0.0000 Ecliptic YDOT -0.00075037 +/- 0.0000 Ecliptic ZDOT -0.00074632 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 37.67485184 +/- 0.0098 Geocenter to KBO 37.07218107 +/- 0.0134 # Hcoef: 7.04
The following table shows the complete astrometric record for 14YK92. 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 (14YK92) followed by the observatory code and reference code for the source of the astrometry.
2013 12 24.32586 05 57 38.643 -29 18 14.06 22.7z 14YK92 W84 C~55TR 2014 01 05.29848 05 56 24.543 -29 16 58.74 23.1g 14YK92 W84 C~55TR 2014 12 23.334051 06 04 44.29 -29 53 29.8 23.8g 14YK92 W84 C~55TR 2014 12 24.296377 06 04 38.20 -29 53 33.7 22.9r 14YK92 W84 C~55TR 2014 12 24.297778 06 04 38.21 -29 53 33.6 22.4i 14YK92 W84 C~55TR 2014 12 26.263866 06 04 25.78 -29 53 37.8 23.2g 14YK92 W84 C~55TR 2014 12 26.265231 06 04 25.78 -29 53 37.7 22.5r 14YK92 W84 C~55TR 2015 01 20.189641 06 01 57.03 -29 47 00.1 22.3i 14YK92 W84 C~55TR 2015 01 31.09000 06 01 02.737 -29 40 04.74 23.4z 14YK92 W84 C~55TR 2015 02 10.18487 06 00 21.576 -29 31 52.09 22.7z 14YK92 W84 C~55TR 2015 02 10.195984 06 00 21.54 -29 31 51.8 22.7i 14YK92 W84 C~55TR 2015 02 11.193796 06 00 18.01 -29 30 58.1 22.6z 14YK92 W84 C~55TR 2015 02 16.181412 06 00 01.94 -29 26 18.4 22.8r 14YK92 W84 C~55TR 2015 02 16.182789 06 00 01.93 -29 26 18.3 22.6i 14YK92 W84 C~55TR
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 0.00 0.00 -0.04
2 0.0328 -968.95 0.01 80.59 0.07
3 0.9966 5522.05 -0.09 -2195.87 -0.15
4 0.9992 5442.73 -0.16 -2198.02 -0.06
5 0.9992 5442.86 0.09 -2197.93 0.04
6 1.0046 5281.05 0.01 -2198.61 -0.03
7 1.0046 5281.05 0.13 -2198.51 0.06
8 1.0729 3352.38 -0.05 -1764.46 -0.06
9 1.1027 2651.28 -0.16 -1338.41 0.04
10 1.1303 2120.96 0.02 -838.59 0.20
11 1.1304 2120.49 0.07 -838.29 -0.10
12 1.1331 2075.08 0.06 -784.02 -0.01
13 1.1468 1868.63 0.07 -501.77 0.01
14 1.1468 1868.50 -0.01 -501.67 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.
14YK92 quality flag:3 Type: SCATEXTD SCATEXTD SCATEXTD axisobj 39.953 40.150 39.868 ecceobj 0.067 0.096 0.052 incobj 54.700 54.715 54.686 qmin 36.893 31.234 37.208 qmax 42.914 49.073 42.428 amean 39.805 39.973 39.709 amin 39.511 39.590 39.400 amax 40.114 40.363 40.028 emean 0.062 0.153 0.050 emin 0.052 0.067 0.038 emax 0.070 0.216 0.060 imean 55.104 54.789 55.087 imin 54.895 54.214 54.878 imax 55.314 55.336 55.302 excite_mean 0.823 0.832 0.822 fracstop 1.000 1.000 1.000 cjmean 2.070 2.066 2.072 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 180.8 200.7 201.1 kozaiamp 180.0 179.9 180.0