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: 14WB556 # Created Sat Apr 27 01:16:48 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 32 observations of 32 # Arc: 7.03y # First observation: 2014/11/21 # Last observation: 2021/12/01 # Chi-squared of fit: 16.41 DOF: 58 RMS: 0.13 # Min/Max residuals: -0.50 0.34 # Exact a, adot, b, bdot, g, gdot: 1.922071E-05 2.818654E-02 -9.559884E-07 -1.945782E-03 2.262607E-02 5.639782E-03 # Covariance matrix: 1.5891E-13 -1.0825E-13 -2.9450E-15 6.0061E-15 -2.5263E-14 -4.5641E-13 -1.0825E-13 1.4327E-13 8.1741E-15 -9.8723E-15 -1.4400E-14 6.8991E-13 -2.9450E-15 8.1741E-15 9.4530E-14 -1.8922E-14 -1.4776E-14 4.1598E-14 6.0061E-15 -9.8723E-15 -1.8922E-14 7.9086E-15 4.0379E-15 -5.0072E-14 -2.5263E-14 -1.4400E-14 -1.4776E-14 4.0379E-15 1.9770E-13 -7.5375E-14 -4.5641E-13 6.8991E-13 4.1598E-14 -5.0072E-14 -7.5375E-14 3.4966E-12 # lat0 lon0 xBary yBary zBary JD0 -24.275931 14.988588 -0.679782 -0.294871 -0.654277 2456982.718308 # Heliocentric elements and errors Epoch: 2456982.5000 = 2014/11/21 Mean Anomaly: 1.22025 +/- 0.002 Argument of Peri: 235.36025 +/- 0.006 Long of Asc Node: 114.98649 +/- 0.000 Inclination: 24.16402 +/- 0.000 Eccentricity: 0.84535655 +/- 0.0001 Semi-Major Axis: 276.22210222 +/- 0.2575 Time of Perihelion: 2451298.7794 +/- 11.3 Perihelion: 42.71593831 +/- 0.0563 Aphelion: 509.72826613 +/- 0.4768 Period (y) 4590.8789 +/- 6.42 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 39.43253856 +/- 0.0008 Ecliptic Y 11.26388268 +/- 0.0002 Ecliptic Z -18.17079920 +/- 0.0004 Ecliptic XDOT -0.00037892 +/- 0.0000 Ecliptic YDOT 0.00342552 +/- 0.0000 Ecliptic ZDOT -0.00049510 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 44.85489363 +/- 0.0007 Geocenter to KBO 44.19667327 +/- 0.0009 # Hcoef: 7.17
The following table shows the complete astrometric record for 14WB556. 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 (14WB556) followed by the observatory code and reference code for the source of the astrometry.
2014 11 21.21753 01 33 20.066 -16 27 53.37 23.4r 14WB556 W84 C~4yVK 2014 11 21.21753 01 33 20.06 -16 27 53.4 23.7r 14WB556 W84 C~3cpS 2014 12 20.13696 01 32 11.059 -16 20 55.87 24.5g 14WB556 W84 C~4yVK 2014 12 20.13696 01 32 11.06 -16 20 55.9 24.6g 14WB556 W84 C~3cpS 2014 12 24.11398 01 32 06.500 -16 19 11.16 24.3g 14WB556 W84 C~4yVK 2014 12 24.11535 01 32 06.492 -16 19 11.18 23.7r 14WB556 W84 C~4yVK 2014 12 24.11535 01 32 06.49 -16 19 11.2 23.8r 14WB556 W84 C~3cpT 2015 01 12.07856 01 32 03.65 -16 08 40.7 23.4r 14WB556 W84 C~3cpT 2015 09 04.36649 01 44 29.889 -15 26 17.41 23.3z 14WB556 W84 C~4yVK 2015 09 13.28647 01 44 04.744 -15 31 46.79 24.1r 14WB556 W84 C~4yVK 2015 10 07.20558 01 42 38.132 -15 44 46.25 23.7g 14WB556 W84 C~4yVK 2015 10 07.20558 01 42 38.13 -15 44 46.3 24.3g 14WB556 W84 C~3cpT 2015 10 07.20699 01 42 38.117 -15 44 46.26 23.1i 14WB556 W84 C~4yVK 2015 12 01.09016 01 39 07.787 -15 54 08.40 24.0r 14WB556 W84 C~4yVK 2015 12 01.09016 01 39 07.79 -15 54 08.4 24.1r 14WB556 W84 C~3cpT 2016 09 30.26542 01 49 13.438 -15 08 15.98 23.7r 14WB556 W84 C~4yVK 2016 09 30.26680 01 49 13.436 -15 08 16.11 23.1i 14WB556 W84 C~4yVK 2016 09 30.26817 01 49 13.423 -15 08 16.00 23.5g 14WB556 W84 C~4yVK 2016 12 28.292751 01 44 23.26 -15 12 21.5 24.2r 14WB556 568 C~4qQP 2016 12 28.300595 01 44 23.23 -15 12 21.2 24.2r 14WB556 568 C~4qQP 2016 12 28.308679 01 44 23.23 -15 12 21.3 14WB556 568 C~4qQP 2017 11 09.20524 01 52 37.058 -14 48 09.48 23.7i 14WB556 W84 C~4yVK 2017 11 27.07762 01 51 32.540 -14 48 32.87 23.4i 14WB556 W84 C~4yVK 2018 12 03.05923 01 57 11.976 -14 14 34.02 23.4r 14WB556 W84 C~4yVK 2020 10 20.283020 02 11 32.005 -13 01 52.85 23.6G 14WB556 G37 C~4Kxw 2020 10 20.336010 02 11 31.785 -13 01 54.01 14WB556 G37 C~4Kxw 2021 11 05.263310 02 16 06.883 -12 32 38.74 23.6G 14WB556 G37 C~5BVN 2021 11 05.318760 02 16 06.659 -12 32 39.38 14WB556 G37 C~5BVN 2021 11 05.377910 02 16 06.411 -12 32 40.19 14WB556 G37 C~5BVN 2021 12 01.118300 02 14 30.516 -12 34 24.95 23.8G 14WB556 G37 C~5J6g 2021 12 01.170000 02 14 30.365 -12 34 24.39 14WB556 G37 C~5J6g 2021 12 01.221860 02 14 30.184 -12 34 24.77 14WB556 G37 C~5J6g
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 0.13 0.00 -0.04
2 0.0000 0.00 0.04 0.00 -0.07
3 0.0792 0.00 -0.07 0.00 0.01
4 0.0792 0.00 -0.05 0.00 -0.02
5 0.0901 0.00 0.02 0.00 0.10
6 0.0901 0.00 -0.07 0.00 0.04
7 0.0901 0.00 -0.10 0.00 0.02
8 0.1420 0.00 -0.03 0.00 0.13
9 0.7862 0.00 -0.05 0.00 0.24
10 0.8106 0.00 -0.07 0.00 0.03
11 0.8761 0.00 0.11 0.00 0.04
12 0.8761 0.00 0.14 0.00 0.09
13 0.8761 0.00 -0.00 0.00 0.12
14 1.0263 0.00 0.01 0.00 0.00
15 1.0263 0.00 -0.04 0.00 0.00
16 1.8591 0.00 -0.03 0.00 0.02
17 1.8591 0.00 0.02 0.00 -0.06
18 1.8591 0.00 -0.10 0.00 0.09
19 2.1029 0.00 0.34 0.00 -0.24
20 2.1029 0.00 0.00 0.00 -0.16
21 2.1029 0.00 0.12 0.00 -0.50
22 2.9678 0.00 -0.11 0.00 -0.07
23 3.0167 0.00 0.01 0.00 0.04
24 4.0324 0.00 -0.08 0.00 0.04
25 5.9139 0.00 0.08 0.00 0.04
26 5.9141 0.00 0.05 0.00 0.03
27 6.9570 0.00 -0.08 0.00 0.03
28 6.9572 0.00 -0.02 0.00 0.10
29 6.9573 0.00 -0.11 0.00 0.05
30 7.0278 0.00 -0.14 0.00 -0.02
31 7.0279 0.00 0.17 0.00 0.29
32 7.0281 0.00 0.03 0.00 -0.35
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.
14WB556 quality flag:3 Type: SCATNEAR SCATNEAR SCATNEAR axisobj 299.055 299.055 299.055 ecceobj 0.857 0.857 0.857 incobj 24.160 24.160 24.160 qmin 40.112 40.038 40.097 qmax 565.765 564.081 565.664 amean 280.955 280.958 280.951 amin 269.032 268.710 268.559 amax 304.279 303.419 304.228 emean 0.848 0.848 0.848 emin 0.838 0.838 0.838 emax 0.859 0.859 0.859 imean 22.687 22.660 22.685 imin 22.164 22.164 22.164 imax 23.176 23.091 23.142 excite_mean 0.931 0.931 0.931 fracstop 1.000 1.000 1.000 cjmean 3.099 3.099 3.099 libcent 0 158.5 159.2 158.8 libamp 0 126.4 125.7 126.1 libcent 1 252.7 258.1 254.7 libamp 1 67.6 62.2 65.5 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 238.7 239.5 238.8 kozaiamp 4.6 6.0 5.1