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: 14UC225 # Created Fri Nov 22 02:10:05 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 32 observations of 32 # Arc: 10.86y # First observation: 2013/11/22 # Last observation: 2024/10/01 # Chi-squared of fit: 8.04 DOF: 58 RMS: 0.09 # Min/Max residuals: -0.19 0.21 # Exact a, adot, b, bdot, g, gdot: 1.838372E-05 3.823754E-02 -1.360306E-06 -1.697619E-03 3.257711E-02 -2.712436E-03 # Covariance matrix: 1.7529E-13 -1.2252E-13 -4.7415E-15 4.9299E-15 -2.0107E-14 -2.2482E-13 -1.2252E-13 1.4864E-13 4.9413E-15 -6.0453E-15 -1.1536E-13 2.6530E-13 -4.7415E-15 4.9413E-15 6.7023E-14 -1.0093E-14 7.9145E-16 9.8477E-15 4.9299E-15 -6.0453E-15 -1.0093E-14 4.5666E-15 3.6977E-15 -1.1296E-14 -2.0107E-14 -1.1536E-13 7.9145E-16 3.6977E-15 6.8228E-13 -1.1692E-13 -2.2482E-13 2.6530E-13 9.8477E-15 -1.1296E-14 -1.1692E-13 5.0303E-13 # lat0 lon0 xBary yBary zBary JD0 -4.396979 18.710721 -0.646753 -0.056921 -0.742114 2456618.656888 # Heliocentric elements and errors Epoch: 2456618.5000 = 2013/11/22 Mean Anomaly: 336.80974 +/- 0.020 Argument of Peri: 269.65901 +/- 0.025 Long of Asc Node: 139.63821 +/- 0.001 Inclination: 4.94034 +/- 0.000 Eccentricity: 0.11760419 +/- 0.0001 Semi-Major Axis: 35.15633052 +/- 0.0045 Time of Perihelion: 2461523.1375 +/- 14.3 Perihelion: 31.02179870 +/- 0.0049 Aphelion: 39.29086233 +/- 0.0058 Period (y) 208.4556 +/- 0.04 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 29.48508768 +/- 0.0007 Ecliptic Y 10.67235163 +/- 0.0002 Ecliptic Z -2.35347956 +/- 0.0001 Ecliptic XDOT -0.00126267 +/- 0.0000 Ecliptic YDOT 0.00296544 +/- 0.0000 Ecliptic ZDOT -0.00012463 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 31.44535288 +/- 0.0007 Geocenter to KBO 30.69647719 +/- 0.0008 # Hcoef: 7.43
The following table shows the complete astrometric record for 14UC225. 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 (14UC225) followed by the observatory code and reference code for the source of the astrometry.
2013 11 22.15611 01 15 44.098 +03 15 40.16 22.1i 14UC225 W84 C~4yUy 2013 11 22.15611 01 15 44.10 +03 15 40.2 22.2i 14UC225 W84 C~3coL 2013 11 22.15893 01 15 44.093 +03 15 40.02 21.6z 14UC225 W84 C~4yUy 2013 11 22.15893 01 15 44.09 +03 15 40.0 21.7z 14UC225 W84 C~3coL 2014 10 21.22515 01 26 53.312 +04 15 20.16 22.9g 14UC225 W84 C~4yUy 2014 10 21.22515 01 26 53.31 +04 15 20.2 23.0g 14UC225 W84 C~3coL 2014 10 21.22651 01 26 53.286 +04 15 20.20 22.6r 14UC225 W84 C~4yUy 2014 10 21.22651 01 26 53.29 +04 15 20.2 22.6r 14UC225 W84 C~3coL 2014 10 28.21303 01 26 12.591 +04 11 22.82 22.2r 14UC225 W84 C~4yUy 2014 10 28.21303 01 26 12.59 +04 11 22.8 22.2r 14UC225 W84 C~3coL 2014 10 28.23025 01 26 12.486 +04 11 22.16 23.3g 14UC225 W84 C~4yUy 2014 10 28.23025 01 26 12.49 +04 11 22.1 23.4g 14UC225 W84 C~3coL 2014 11 14.071181 01 24 41.22 +04 03 03.2 22.6r 14UC225 W84 C~352R 2014 11 14.07171 01 24 41.223 +04 03 03.25 22.8r 14UC225 W84 C~4yUy 2014 11 14.07171 01 24 41.22 +04 03 03.2 22.6r 14UC225 W84 C~3coL 2014 11 14.13577 01 24 40.896 +04 03 01.56 22.2i 14UC225 W84 C~4yUy 2014 11 14.13577 01 24 40.90 +04 03 01.6 22.3i 14UC225 W84 C~3coL 2014 11 15.17294 01 24 35.754 +04 02 35.08 22.0i 14UC225 W84 C~4yUy 2014 11 15.17294 01 24 35.75 +04 02 35.1 22.1i 14UC225 W84 C~3coL 2014 11 17.15109 01 24 26.148 +04 01 46.32 21.8z 14UC225 W84 C~4yUy 2014 11 17.15109 01 24 26.15 +04 01 46.3 21.9z 14UC225 W84 C~3coL 2014 11 28.10420 01 23 38.333 +03 57 57.84 21.8z 14UC225 W84 C~4yUy 2014 11 28.10420 01 23 38.33 +03 57 57.8 21.9z 14UC225 W84 C~3coL 2015 11 06.18503 01 33 47.028 +04 50 56.36 22.1r 14UC225 W84 C~4yUy 2015 11 18.16042 01 32 43.99 +04 45 28.8 22.3z 14UC225 W84 C~3coL 2015 12 18.07433 01 30 55.282 +04 38 00.00 22.3z 14UC225 W84 C~4yUy 2015 12 18.07433 01 30 55.28 +04 38 00.0 22.5z 14UC225 W84 C~3coL 2017 09 23.37758 01 54 50.69 +06 42 49.5 22.2R 14UC225 G37 C~2LT9 2017 09 23.46046 01 54 50.25 +06 42 46.7 14UC225 G37 C~2LT9 2024 10 01.479802 02 54 57.369 +11 25 17.67 22.5w 14UC225 F52 C~8H4Q 2024 10 01.491737 02 54 57.312 +11 25 16.97 22.4w 14UC225 F52 C~8H4Q 2024 10 01.503681 02 54 57.248 +11 25 16.72 22.5w 14UC225 F52 C~8H4Q
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 -0.01 0.00 0.12
2 0.0000 0.00 -0.04 0.00 0.08
3 0.0000 0.00 0.07 0.00 -0.01
4 0.0000 0.00 0.02 0.00 -0.03
5 0.9119 0.00 0.18 0.00 -0.02
6 0.9119 0.00 0.21 0.00 -0.06
7 0.9119 0.00 -0.05 0.00 0.02
8 0.9119 0.00 0.01 0.00 0.02
9 0.9310 0.00 -0.02 0.00 -0.06
10 0.9310 0.00 -0.01 0.00 -0.04
11 0.9311 0.00 -0.01 0.00 -0.19
12 0.9311 0.00 -0.07 0.00 -0.13
13 0.9772 0.00 -0.05 0.00 -0.01
14 0.9772 0.00 -0.01 0.00 -0.00
15 0.9772 0.00 0.04 0.00 0.05
16 0.9774 0.00 0.09 0.00 0.05
17 0.9774 0.00 0.03 0.00 0.01
18 0.9802 0.00 -0.05 0.00 -0.04
19 0.9802 0.00 0.01 0.00 -0.06
20 0.9856 0.00 -0.06 0.00 -0.06
21 0.9856 0.00 -0.09 0.00 -0.04
22 1.0156 0.00 -0.04 0.00 0.00
23 1.0156 0.00 0.00 0.00 0.04
24 1.9549 0.00 -0.07 0.00 -0.05
25 1.9877 0.00 -0.08 0.00 -0.07
26 2.0696 0.00 0.05 0.00 0.14
27 2.0696 0.00 0.08 0.00 0.14
28 3.8363 0.00 0.11 0.00 0.20
29 3.8366 0.00 -0.18 0.00 0.16
30 10.8592 0.00 0.04 0.00 0.19
31 10.8592 0.00 0.03 0.00 -0.19
32 10.8593 0.00 -0.07 0.00 -0.12
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.
14UC225 quality flag:3 Type: 5:4E 5:4E 5:4E axisobj 35.337 35.351 35.323 ecceobj 0.120 0.121 0.120 incobj 4.933 4.933 4.933 qmin 30.591 30.569 30.582 qmax 39.820 39.921 39.721 amean 34.944 34.944 34.944 amin 34.516 34.480 34.537 amax 35.400 35.453 35.391 emean 0.104 0.105 0.104 emin 0.084 0.082 0.083 emax 0.125 0.128 0.124 imean 3.052 2.959 3.139 imin 1.913 1.758 1.931 imax 4.172 4.066 4.178 excite_mean 0.118 0.117 0.118 fracstop 1.000 1.000 1.000 cjmean 3.002 3.002 3.001 libcent 0 181.1 181.2 180.7 libamp 0 119.0 131.0 114.7 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 182.1 188.0 186.7 kozaiamp 180.0 179.9 180.0