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: 14UX277 # Created Thu Apr 25 01:16:36 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 17 observations of 17 # Arc: 8.15y # First observation: 2014/10/31 # Last observation: 2022/12/26 # Chi-squared of fit: 7.61 DOF: 28 RMS: 0.12 # Min/Max residuals: -0.30 0.27 # Exact a, adot, b, bdot, g, gdot: 1.490587E-05 1.993744E-02 -2.960013E-06 -3.963562E-03 2.057138E-02 -8.860197E-03 # Covariance matrix: 5.6983E-13 -4.2880E-14 -8.1999E-14 -5.5602E-15 6.8161E-13 -3.0067E-13 -4.2880E-14 1.5960E-13 -9.2131E-17 -3.0521E-14 2.6878E-13 8.2554E-13 -8.1999E-14 -9.2131E-17 1.8632E-13 -3.2631E-14 -1.4326E-13 5.1047E-14 -5.5602E-15 -3.0521E-14 -3.2631E-14 2.0036E-14 -6.9037E-14 -1.6784E-13 6.8161E-13 2.6878E-13 -1.4326E-13 -6.9037E-14 1.7119E-12 1.0802E-12 -3.0067E-13 8.2554E-13 5.1047E-14 -1.6784E-13 1.0802E-12 4.8234E-12 # lat0 lon0 xBary yBary zBary JD0 -31.013395 37.836816 0.007536 -0.512083 -0.852163 2456961.763688 # Heliocentric elements and errors Epoch: 2456962.5000 = 2014/11/01 Mean Anomaly: 342.47255 +/- 0.016 Argument of Peri: 319.57917 +/- 0.015 Long of Asc Node: 148.94597 +/- 0.001 Inclination: 32.18846 +/- 0.000 Eccentricity: 0.58133954 +/- 0.0002 Semi-Major Axis: 91.21289139 +/- 0.0564 Time of Perihelion: 2472454.2005 +/- 281.3 Perihelion: 38.18723078 +/- 0.0317 Aphelion: 144.23855199 +/- 0.0917 Period (y) 871.1492 +/- 0.81 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 33.68981433 +/- 0.0021 Ecliptic Y 26.16173618 +/- 0.0016 Ecliptic Z -25.04655531 +/- 0.0016 Ecliptic XDOT -0.00264490 +/- 0.0000 Ecliptic YDOT 0.00130410 +/- 0.0000 Ecliptic ZDOT 0.00015558 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 49.46516892 +/- 0.0019 Geocenter to KBO 48.61160163 +/- 0.0031 # Hcoef: 6.88
The following table shows the complete astrometric record for 14UX277. 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 (14UX277) followed by the observatory code and reference code for the source of the astrometry.
2014 10 31.26291 03 01 45.147 -15 17 01.74 24.5r 14UX277 W84 C~55Sh 2014 11 16.29015 03 00 39.675 -15 21 30.19 23.5r 14UX277 W84 C~55Sh 2014 12 01.25204 02 59 40.588 -15 22 54.94 23.4i 14UX277 W84 C~55Sh 2014 12 20.20018 02 58 36.581 -15 20 40.29 24.4g 14UX277 W84 C~55Sh 2015 12 14.21807 03 03 42.628 -15 12 36.25 24.0g 14UX277 W84 C~55Sh 2015 12 14.21945 03 03 42.647 -15 12 36.28 23.4i 14UX277 W84 C~55Sh 2015 12 14.22084 03 03 42.639 -15 12 36.15 24.0r 14UX277 W84 C~55Sh 2015 12 14.22221 03 03 42.634 -15 12 36.22 24.3g 14UX277 W84 C~55Sh 2016 11 10.30206 03 10 44.641 -15 00 41.48 23.7r 14UX277 W84 C~55Sh 2016 12 30.10564 03 07 44.744 -14 58 33.83 23.5r 14UX277 W84 C~55Sh 2017 12 08.22710 03 13 49.874 -14 52 54.65 23.2i 14UX277 W84 C~55Sh 2017 12 10.16610 03 13 42.709 -14 52 44.74 24.0r 14UX277 W84 C~55Sh 2017 12 10.16749 03 13 42.709 -14 52 44.66 23.7g 14UX277 W84 C~55Sh 2018 01 09.13511 03 12 17.536 -14 44 15.34 23.8r 14UX277 W84 C~55Sh 2018 01 09.13790 03 12 17.543 -14 44 15.21 24.4g 14UX277 W84 C~55Sh 2022 12 26.123800 03 38 41.929 -13 47 54.23 23.5G 14UX277 G37 C~69bM 2022 12 26.176780 03 38 41.759 -13 47 53.17 14UX277 G37 C~69bM
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 0.09 0.00 0.01
2 0.0439 0.00 -0.12 0.00 0.04
3 0.0848 0.00 0.27 0.00 -0.06
4 0.1367 0.00 -0.30 0.00 0.14
5 1.1197 0.00 -0.21 0.00 -0.09
6 1.1197 0.00 0.15 0.00 -0.14
7 1.1197 0.00 0.10 0.00 -0.02
8 1.1197 0.00 0.09 0.00 -0.10
9 2.0289 0.00 -0.05 0.00 0.20
10 2.1652 0.00 0.08 0.00 -0.01
11 3.1046 0.00 -0.13 0.00 0.04
12 3.1099 0.00 -0.06 0.00 -0.00
13 3.1099 0.00 0.02 0.00 0.07
14 3.1920 0.00 -0.03 0.00 -0.03
15 3.1920 0.00 0.16 0.00 0.03
16 8.1529 0.00 -0.08 0.00 -0.12
17 8.1531 0.00 0.08 0.00 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.
14UX277 quality flag:3 Type: SCATNEAR SCATNEAR SCATNEAR axisobj 92.235 92.233 92.236 ecceobj 0.583 0.583 0.583 incobj 32.137 32.137 32.137 qmin 36.584 36.614 36.559 qmax 148.114 148.386 148.501 amean 90.726 90.711 90.728 amin 89.265 89.282 89.317 amax 92.793 92.931 92.978 emean 0.578 0.578 0.578 emin 0.563 0.563 0.562 emax 0.597 0.597 0.597 imean 30.968 30.979 30.976 imin 30.095 30.114 30.112 imax 31.945 31.946 31.941 excite_mean 0.774 0.774 0.774 fracstop 1.000 1.000 1.000 cjmean 2.760 2.760 2.760 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 129.7 129.4 129.4 kozaiamp 180.0 180.0 180.0