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: 14VL43 # Created Wed Dec 4 02:10:06 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 17 observations of 17 # Arc: 5.01y # First observation: 2013/10/13 # Last observation: 2018/10/18 # Chi-squared of fit: 4.28 DOF: 28 RMS: 0.09 # Min/Max residuals: -0.14 0.17 # Exact a, adot, b, bdot, g, gdot: 1.622782E-05 2.451358E-02 1.183575E-06 1.691946E-03 2.478551E-02 1.519643E-03 # Covariance matrix: 5.8296E-13 -3.6181E-13 1.1977E-14 -1.7101E-14 -8.1655E-14 -2.0941E-12 -3.6181E-13 4.1744E-13 -1.8827E-14 2.6424E-14 1.7785E-13 3.2333E-12 1.1977E-14 -1.8827E-14 4.2004E-13 -1.1670E-13 -1.2631E-14 -1.6324E-13 -1.7101E-14 2.6424E-14 -1.1670E-13 4.1962E-14 1.4301E-14 2.2736E-13 -8.1655E-14 1.7785E-13 -1.2631E-14 1.4301E-14 4.8950E-13 1.7315E-12 -2.0941E-12 3.2333E-12 -1.6324E-13 2.2736E-13 1.7315E-12 2.7811E-11 # lat0 lon0 xBary yBary zBary JD0 -2.711857 5.257380 -0.246690 -0.045614 -0.965365 2456578.589948 # Heliocentric elements and errors Epoch: 2456578.5000 = 2013/10/13 Mean Anomaly: 60.56590 +/- 0.061 Argument of Peri: 258.04935 +/- 0.082 Long of Asc Node: 39.32622 +/- 0.003 Inclination: 4.76285 +/- 0.000 Eccentricity: 0.07269156 +/- 0.0002 Semi-Major Axis: 42.65570754 +/- 0.0047 Time of Perihelion: 2439459.0496 +/- 17.5 Perihelion: 39.55499755 +/- 0.0100 Aphelion: 45.75641753 +/- 0.0103 Period (y) 278.5954 +/- 0.05 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 41.07064344 +/- 0.0011 Ecliptic Y 4.03005983 +/- 0.0001 Ecliptic Z -1.90888568 +/- 0.0001 Ecliptic XDOT -0.00007851 +/- 0.0000 Ecliptic YDOT 0.00271115 +/- 0.0000 Ecliptic ZDOT 0.00017888 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 41.31197842 +/- 0.0011 Geocenter to KBO 40.34614855 +/- 0.0011 # Hcoef: 7.17
The following table shows the complete astrometric record for 14VL43. 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 (14VL43) followed by the observatory code and reference code for the source of the astrometry.
2013 10 13.08917 00 23 36.065 -00 24 04.18 23.2z 14VL43 W84 C~52UT 2013 10 13.11349 00 23 35.970 -00 24 04.75 23.0i 14VL43 W84 C~52UT 2014 11 13.06801 00 26 36.565 +00 03 22.37 23.0i 14VL43 W84 C~52UT 2014 11 15.15632 00 26 30.258 +00 02 50.48 22.8z 14VL43 W84 C~52UT 2016 09 09.31225 00 40 59.930 +01 46 46.75 23.7r 14VL43 W84 C~52UT 2016 09 09.31362 00 40 59.913 +01 46 46.76 22.8i 14VL43 W84 C~52UT 2016 09 09.31500 00 40 59.906 +01 46 46.82 23.8g 14VL43 W84 C~52UT 2016 09 10.31583 00 40 55.824 +01 46 20.15 23.2z 14VL43 W84 C~52UT 2016 11 08.14374 00 36 43.670 +01 21 02.42 22.9i 14VL43 W84 C~52UT 2016 11 25.06213 00 35 53.399 +01 16 46.55 23.7r 14VL43 W84 C~52UT 2016 11 30.09003 00 35 42.442 +01 15 58.61 22.0z 14VL43 W84 C~52UT 2017 08 22.32458 00 47 01.110 +02 31 59.68 23.6i 14VL43 W84 C~52UT 2017 08 22.32596 00 47 01.085 +02 31 59.85 23.3r 14VL43 W84 C~52UT 2017 10 20.16215 00 42 56.304 +02 06 21.65 23.7r 14VL43 W84 C~52UT 2017 10 20.16352 00 42 56.302 +02 06 21.54 23.3i 14VL43 W84 C~52UT 2018 10 18.19480 00 48 01.862 +02 45 16.25 23.5i 14VL43 W84 C~52UT 2018 10 18.19616 00 48 01.841 +02 45 16.15 22.9z 14VL43 W84 C~52UT
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 0.0001 0.00 0.11 0.00 0.00
3 1.0841 0.00 0.15 0.00 0.03
4 1.0898 0.00 -0.11 0.00 0.03
5 2.9082 0.00 0.06 0.00 -0.04
6 2.9082 0.00 -0.11 0.00 0.00
7 2.9082 0.00 -0.13 0.00 0.10
8 2.9110 0.00 0.15 0.00 0.01
9 3.0720 0.00 0.04 0.00 -0.01
10 3.1183 0.00 0.00 0.00 -0.10
11 3.1321 0.00 -0.05 0.00 0.11
12 3.8583 0.00 0.17 0.00 -0.09
13 3.8583 0.00 -0.14 0.00 0.11
14 4.0194 0.00 -0.02 0.00 0.06
15 4.0194 0.00 0.04 0.00 -0.01
16 5.0133 0.00 0.13 0.00 -0.00
17 5.0133 0.00 -0.09 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.
14VL43 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 42.908 42.908 42.908 ecceobj 0.077 0.077 0.077 incobj 4.756 4.756 4.756 qmin 38.852 38.856 38.848 qmax 46.768 46.776 46.761 amean 42.692 42.691 42.692 amin 42.351 42.359 42.367 amax 43.060 43.042 43.055 emean 0.064 0.065 0.063 emin 0.040 0.042 0.037 emax 0.087 0.087 0.087 imean 3.151 3.174 3.127 imin 1.647 1.663 1.613 imax 4.495 4.495 4.495 excite_mean 0.085 0.086 0.084 fracstop 1.000 1.000 1.000 cjmean 3.077 3.077 3.077 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 182.4 182.5 182.0 kozaiamp 180.0 180.0 180.0