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: 14UY229
# Created Fri Nov 22 02:10:07 2024
# Orbit generated from Bernstein formalism
# Fitting 36 observations of 36
# Arc: 4.06y
# First observation: 2013/08/08
# Last observation: 2017/08/30
Preliminary a, adot, b, bdot, g, gdot:
-0.000085 0.013588 -0.000001 0.000622 0.017935 0.000000
# Chi-squared of fit: 14.43 DOF: 66 RMS: 0.11
# Min/Max residuals: -0.35 0.23
# Exact a, adot, b, bdot, g, gdot:
1.177731E-05 1.343082E-02 3.284135E-07 6.156810E-04 1.785722E-02 -1.270001E-03
# Covariance matrix:
1.5258E-13 -5.2037E-14 -6.1079E-16 -3.7690E-16 7.3528E-14 -2.2220E-13
-5.2037E-14 1.5529E-13 -3.8250E-15 6.7205E-15 8.2021E-14 2.7224E-12
-6.1079E-16 -3.8250E-15 8.2197E-14 -4.3519E-14 -3.8901E-15 -9.4260E-14
-3.7690E-16 6.7205E-15 -4.3519E-14 4.5322E-14 5.1730E-15 1.6575E-13
7.3528E-14 8.2021E-14 -3.8901E-15 5.1730E-15 1.5268E-13 2.0158E-12
-2.2220E-13 2.7224E-12 -9.4260E-14 1.6575E-13 2.0158E-12 6.7147E-11
# lat0 lon0 xBary yBary zBary JD0
2.134319 23.438950 0.938881 0.014473 -0.387386 2456513.056438
# Heliocentric elements and errors
Epoch: 2456510.5000 = 2013/08/06
Mean Anomaly: 217.98501 +/- 0.121
Argument of Peri: 192.76153 +/- 0.118
Long of Asc Node: 344.08345 +/- 0.010
Inclination: 3.40926 +/- 0.001
Eccentricity: 0.21271737 +/- 0.0002
Semi-Major Axis: 47.74587556 +/- 0.0051
Time of Perihelion: 2504047.7354 +/- 39.7
Perihelion: 37.58949840 +/- 0.0120
Aphelion: 57.90225272 +/- 0.0129
Period (y) 329.9225 +/- 0.05
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X 52.07204281 +/- 0.0011
Ecliptic Y 21.55556634 +/- 0.0005
Ecliptic Z 2.08561354 +/- 0.0000
Ecliptic XDOT -0.00100706 +/- 0.0000
Ecliptic YDOT 0.00180961 +/- 0.0000
Ecliptic ZDOT 0.00008722 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 56.39583199 +/- 0.0011
Geocenter to KBO 55.99976297 +/- 0.0012
# Hcoef: 7.00
The following table shows the complete astrometric record for 14UY229. 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 (14UY229) followed by the observatory code and reference code for the source of the astrometry.
2013 08 08.55566 01 23 33.001 +11 05 09.95 24.5r 14UY229 568 C~2SDm 2013 08 08.59934 01 23 32.954 +11 05 09.66 25.2r 14UY229 568 C~2SDm 2013 09 01.52570 01 22 49.270 +11 01 50.49 24.2r 14UY229 568 C~2SDm 2013 09 01.56454 01 22 49.198 +11 01 50.24 24.2r 14UY229 568 C~2SDm 2013 09 02.51296 01 22 46.842 +11 01 38.25 24.6r 14UY229 568 C~2SDm 2013 09 02.56252 01 22 46.706 +11 01 37.45 24.3r 14UY229 568 C~2SDm 2013 10 09.40083 01 20 50.518 +10 51 01.93 24.2r 14UY229 568 C~2SDm 2013 10 30.37669 01 19 36.436 +10 43 45.08 24.8r 14UY229 568 C~2SDm 2013 10 31.36761 01 19 33.032 +10 43 24.71 24.3r 14UY229 568 C~2SDm 2013 11 01.31349 01 19 29.846 +10 43 05.38 24.0r 14UY229 568 C~2SDm 2013 11 01.35271 01 19 29.694 +10 43 04.50 24.4r 14UY229 568 C~2SDm 2013 11 01.44470 01 19 29.390 +10 43 02.69 24.2r 14UY229 568 C~2SDm 2013 11 27.36654 01 18 12.505 +10 35 00.18 24.2r 14UY229 568 C~2SDm 2013 12 04.35092 01 17 56.812 +10 33 15.63 24.4r 14UY229 568 C~2SDm 2013 12 29.30196 01 17 24.666 +10 29 15.87 24.0r 14UY229 568 C~2SDm 2014 07 25.52468 01 26 33.867 +11 24 29.24 24.3r 14UY229 568 C~2SDm 2014 07 25.56621 01 26 33.856 +11 24 29.32 24.3r 14UY229 568 C~2SDm 2014 07 25.60786 01 26 33.852 +11 24 29.45 25.5r 14UY229 568 C~2SDm 2014 08 23.56417 01 26 02.353 +11 22 43.27 24.6r 14UY229 568 C~2SDm 2014 08 23.61113 01 26 02.257 +11 22 42.93 24.7r 14UY229 568 C~2SDm 2014 09 18.39229 01 24 55.644 +11 17 04.67 24.8r 14UY229 568 C~2SDm 2014 09 18.43188 01 24 55.526 +11 17 04.04 24.4r 14UY229 568 C~2SDm 2014 10 22.43319 01 22 58.073 +11 06 01.71 24.5r 14UY229 568 C~2SDm 2014 10 22.47264 01 22 57.934 +11 06 00.82 24.4r 14UY229 568 C~2SDm 2014 10 22.51153 01 22 57.795 +11 06 00.04 24.9r 14UY229 568 C~2SDm 2014 10 23.43094 01 22 54.509 +11 05 40.47 24.3r 14UY229 568 C~2SDm 2014 11 19.24343 01 21 26.713 +10 56 46.43 24.5r 14UY229 568 C~2SDm 2014 11 19.37639 01 21 26.320 +10 56 43.96 24.6r 14UY229 568 C~2SDm 2014 11 21.22330 01 21 21.128 +10 56 11.00 24.1r 14UY229 568 C~2SDm 2014 11 21.38502 01 21 20.687 +10 56 08.37 24.4r 14UY229 568 C~2SDm 2015 01 19.25297 01 20 19.077 +10 48 08.93 24.5r 14UY229 568 C~2SDm 2015 02 18.22314 01 21 16.416 +10 52 48.69 24.9r 14UY229 568 C~2SDm 2015 02 18.24376 01 21 16.472 +10 52 49.01 24.0r 14UY229 568 C~2SDm 2015 12 07.41609 01 23 35.114 +11 11 18.77 24.8w 14UY229 568 C~2SDm 2017 08 25.60179 01 34 39.708 +12 19 34.41 24.5w 14UY229 568 C~2SDm 2017 08 30.62297 01 34 29.105 +12 18 45.78 24.4w 14UY229 568 C~2SDm
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 0.02 0.00 0.04
2 0.0001 -0.75 0.05 -0.01 -0.09
3 0.0656 -671.77 -0.24 54.47 0.15
4 0.0657 -672.85 0.20 54.63 0.22
5 0.0683 -709.51 0.16 56.43 0.16
6 0.0685 -711.66 -0.01 56.43 0.05
7 0.1693 -2536.49 -0.25 105.51 0.09
8 0.2268 -3712.51 0.06 109.19 -0.17
9 0.2295 -3766.67 -0.19 109.11 0.02
10 0.2321 -3817.47 0.16 108.80 0.02
11 0.2322 -3819.87 -0.10 108.83 0.04
12 0.2324 -3824.71 0.11 108.83 0.04
13 0.3034 -5056.93 0.02 87.20 -0.10
14 0.3225 -5310.82 0.02 77.34 -0.28
15 0.3908 -5840.67 -0.01 33.61 -0.03
16 0.9609 2901.24 0.07 90.28 -0.06
17 0.9610 2901.12 0.04 90.42 -0.05
18 0.9611 2901.12 0.13 90.56 -0.03
19 1.0404 2431.43 -0.07 163.15 0.01
20 1.0405 2429.99 -0.06 163.36 0.10
21 1.1111 1394.57 -0.13 212.01 -0.00
22 1.1112 1392.73 -0.01 212.07 -0.02
23 1.2043 -457.95 0.01 239.36 0.06
24 1.2044 -460.18 0.03 239.30 -0.02
25 1.2045 -462.37 0.07 239.34 0.01
26 1.2071 -514.55 -0.35 239.18 -0.19
27 1.2805 -1913.16 0.05 225.79 0.04
28 1.2808 -1919.45 -0.04 225.66 -0.00
29 1.2859 -2002.70 -0.09 223.65 0.01
30 1.2863 -2009.71 0.23 223.64 0.11
31 1.4475 -3030.88 0.05 118.41 -0.06
32 1.5295 -2142.68 0.09 61.91 -0.11
33 1.5296 -2141.80 0.07 61.90 -0.09
34 2.3295 166.02 -0.08 330.80 0.04
35 4.0467 10757.51 0.06 554.94 0.14
36 4.0604 10594.64 -0.04 566.00 -0.05
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.
14UY229 quality flag:3 Type: 2:1E 2:1E 2:1E axisobj 47.952 47.966 47.938 ecceobj 0.207 0.207 0.206 incobj 3.397 3.397 3.397 qmin 36.044 36.146 35.665 qmax 60.206 60.023 60.526 amean 47.798 47.798 47.798 amin 47.304 47.297 47.265 amax 48.396 48.395 48.419 emean 0.227 0.225 0.231 emin 0.207 0.207 0.206 emax 0.245 0.242 0.252 imean 3.784 3.992 3.407 imin 3.363 3.610 2.397 imax 4.531 4.561 4.538 excite_mean 0.237 0.236 0.238 fracstop 1.000 1.000 1.000 cjmean 3.078 3.079 3.077 libcent 0 277.6 279.1 276.8 libamp 0 29.9 26.4 33.3 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 165.4 171.1 167.0 kozaiamp 180.0 180.0 180.0