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: 14UY277 # Created Sun Dec 22 02:10:10 2024 # Orbit generated from Bernstein formalism # Fitting 17 observations of 17 # Arc: 4.03y # First observation: 2014/10/28 # Last observation: 2018/11/07 Preliminary a, adot, b, bdot, g, gdot: 0.000213 0.028289 0.000010 -0.012158 0.029478 0.000000 # Chi-squared of fit: 5.24 DOF: 28 RMS: 0.10 # Min/Max residuals: -0.20 0.23 # Exact a, adot, b, bdot, g, gdot: 1.517502E-05 2.807232E-02 -6.150810E-06 -1.200563E-02 2.832896E-02 -2.153662E-03 # Covariance matrix: 2.2274E-13 -7.2945E-14 -6.2012E-15 5.6706E-16 1.1696E-13 -1.2960E-13 -7.2945E-14 3.3120E-13 2.7990E-14 -1.3183E-13 3.1787E-13 3.0409E-12 -6.2012E-15 2.7990E-14 1.8934E-13 -7.6694E-14 1.2193E-14 2.9990E-13 5.6706E-16 -1.3183E-13 -7.6694E-14 1.0202E-13 -1.5614E-13 -1.3810E-12 1.1696E-13 3.1787E-13 1.2193E-14 -1.5614E-13 7.8434E-13 3.2001E-12 -1.2960E-13 3.0409E-12 2.9990E-13 -1.3810E-12 3.2001E-12 3.1985E-11 # lat0 lon0 xBary yBary zBary JD0 -32.326078 40.263673 0.099967 -0.529265 -0.836724 2456958.851634 # Heliocentric elements and errors Epoch: 2456950.5000 = 2014/10/20 Mean Anomaly: 315.40232 +/- 0.046 Argument of Peri: 291.11903 +/- 0.064 Long of Asc Node: 169.53940 +/- 0.001 Inclination: 38.42470 +/- 0.000 Eccentricity: 0.10603761 +/- 0.0002 Semi-Major Axis: 38.83193592 +/- 0.0050 Time of Perihelion: 2467899.9357 +/- 11.2 Perihelion: 34.71429018 +/- 0.0083 Aphelion: 42.94958166 +/- 0.0089 Period (y) 241.9868 +/- 0.05 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 23.57880376 +/- 0.0007 Ecliptic Y 19.84364709 +/- 0.0006 Ecliptic Z -18.87622744 +/- 0.0006 Ecliptic XDOT -0.00236554 +/- 0.0000 Ecliptic YDOT 0.00155076 +/- 0.0000 Ecliptic ZDOT -0.00086905 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 36.13920695 +/- 0.0006 Geocenter to KBO 35.29957022 +/- 0.0011 # Hcoef: 7.61
The following table shows the complete astrometric record for 14UY277. 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 (14UY277) followed by the observatory code and reference code for the source of the astrometry.
2014 10 28.350856 03 11 37.43 -15 51 53.5 22.6i 14UY277 W84 C~55Sh 2014 10 28.352222 03 11 37.41 -15 51 53.5 22.9r 14UY277 W84 C~55Sh 2014 10 29.353426 03 11 32.04 -15 52 30.5 23.0i 14UY277 W84 C~55Sh 2014 11 13.30690 03 10 09.486 -15 59 57.49 22.7z 14UY277 W84 C~55Sh 2014 11 16.297361 03 09 52.80 -16 01 01.4 23.2r 14UY277 W84 C~55Sh 2014 11 21.275868 03 09 25.19 -16 02 27.3 23.8g 14UY277 W84 C~55Sh 2014 12 16.216412 03 07 19.43 -16 03 01.8 23.2r 14UY277 W84 C~55Sh 2015 11 08.30856 03 17 54.980 -16 06 18.41 23.7g 14UY277 W84 C~55Sh 2016 11 03.31178 03 25 36.846 -16 11 48.24 23.3i 14UY277 W84 C~55Sh 2016 11 03.31314 03 25 36.841 -16 11 48.29 23.3r 14UY277 W84 C~55Sh 2016 11 03.31449 03 25 36.827 -16 11 48.24 23.3g 14UY277 W84 C~55Sh 2016 12 30.11113 03 20 48.191 -16 15 42.15 23.1r 14UY277 W84 C~55Sh 2017 02 17.05291 03 19 59.749 -15 39 55.00 24.0g 14UY277 W84 C~55Sh 2017 10 30.35109 03 33 20.048 -16 16 02.08 23.4i 14UY277 W84 C~55Sh 2018 02 03.08542 03 26 54.923 -15 59 59.47 23.4i 14UY277 W84 C~55Sh 2018 10 22.36494 03 41 24.447 -16 16 00.54 22.4z 14UY277 W84 C~55Sh 2018 11 07.27716 03 40 00.880 -16 26 18.93 23.5g 14UY277 W84 C~55Sh
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 -0.11
2 0.0000 -0.27 -0.05 0.09 -0.01
3 0.0027 -85.47 -0.07 -10.57 0.12
4 0.0437 -1356.37 -0.09 -60.17 0.23
5 0.0519 -1604.87 0.04 -45.38 -0.04
6 0.0655 -2009.82 0.06 -2.24 -0.20
7 0.1338 -3743.44 -0.04 530.41 0.05
8 1.0293 4884.72 0.22 -2557.72 0.07
9 2.0177 11076.99 -0.06 -5051.33 -0.03
10 2.0177 11076.91 -0.03 -5051.35 -0.05
11 2.0177 11076.73 -0.08 -5051.24 0.07
12 2.1732 7064.56 -0.15 -3901.79 -0.10
13 2.3072 7102.43 0.12 -1642.42 -0.08
14 3.0062 17310.48 0.05 -7546.29 0.03
15 3.2683 12378.14 -0.11 -4756.85 -0.10
16 3.9836 23935.09 0.04 -9981.25 0.07
17 4.0272 22573.92 0.05 -10138.95 0.08
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.
14UY277 quality flag:3 Type: SCATEXTD SCATEXTD SCATEXTD axisobj 39.048 39.061 39.035 ecceobj 0.106 0.107 0.106 incobj 38.321 38.321 38.321 qmin 34.190 34.242 33.898 qmax 43.643 43.677 43.931 amean 38.785 38.816 38.778 amin 38.476 38.524 38.470 amax 39.112 39.146 39.110 emean 0.101 0.101 0.107 emin 0.087 0.088 0.092 emax 0.116 0.116 0.123 imean 37.816 37.817 37.748 imin 37.480 37.478 37.418 imax 38.150 38.144 38.047 excite_mean 0.621 0.621 0.622 fracstop 1.000 1.000 1.000 cjmean 2.561 2.561 2.562 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 172.5 172.9 191.1 kozaiamp 180.0 180.0 180.0