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: 22LY14
# Created Mon Apr 28 01:11:30 2025
# Orbit generated from Bernstein formalism
# Fitting 15 observations of 15
# Arc: 1.27y
# First observation: 2022/06/02
# Last observation: 2023/09/10
Preliminary a, adot, b, bdot, g, gdot:
0.000000 0.027012 -0.000000 -0.000794 0.025710 0.000000
# Chi-squared of fit: 0.56 DOF: 24 RMS: 0.03
# Min/Max residuals: -0.07 0.07
# Exact a, adot, b, bdot, g, gdot:
1.624222E-05 2.685191E-02 -6.216638E-07 -7.997964E-04 2.558275E-02 -1.578439E-03
# Covariance matrix:
2.5888E-13 1.5121E-13 7.3938E-15 -3.4286E-13 1.1336E-12 3.0364E-10
1.5121E-13 7.4965E-11 -1.0954E-12 4.6339E-11 -4.4966E-11 -4.0668E-08
7.3938E-15 -1.0954E-12 1.8692E-13 -8.8511E-13 8.3113E-13 6.5687E-10
-3.4286E-13 4.6339E-11 -8.8511E-13 3.2086E-11 -3.5604E-11 -2.7944E-08
1.1336E-12 -4.4966E-11 8.3113E-13 -3.5604E-11 4.6386E-11 3.1287E-08
3.0364E-10 -4.0668E-08 6.5687E-10 -2.7944E-08 3.1287E-08 2.4538E-05
# lat0 lon0 xBary yBary zBary JD0
0.828427 -72.738677 0.599372 0.011577 -0.819264 2459732.944521
# Heliocentric elements and errors
Epoch: 2459730.5000 = 2022/05/31
Mean Anomaly: 332.67021 +/- 46.705
Argument of Peri: 190.68937 +/- 66.963
Long of Asc Node: 131.99512 +/- 0.064
Inclination: 1.87836 +/- 0.004
Eccentricity: 0.14395088 +/- 0.1179
Semi-Major Axis: 45.49166847 +/- 1.4009
Time of Perihelion: 2468238.5504 +/- 14534.5
Perihelion: 38.94310261 +/- 5.4970
Aphelion: 52.04023433 +/- 5.5988
Period (y) 306.8358 +/- 14.17
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X 11.27795790 +/- 0.0031
Ecliptic Y -38.28655026 +/- 0.0099
Ecliptic Z 0.56520883 +/- 0.0001
Ecliptic XDOT 0.00269624 +/- 0.0002
Ecliptic YDOT 0.00102182 +/- 0.0005
Ecliptic ZDOT -0.00008814 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 39.91706059 +/- 0.0096
Geocenter to KBO 39.08883192 +/- 0.0104
# Hcoef: 10.73
The following table shows the complete astrometric record for 22LY14. 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 (22LY14) followed by the observatory code and reference code for the source of the astrometry.
2022 06 02.44372 19 14 23.079 -21 30 12.34 26.6r 22LY14 266 C~6Ipa 2022 06 02.53086 19 14 22.716 -21 30 12.96 26.6r 22LY14 266 C~6Ipa 2022 06 02.61096 19 14 22.381 -21 30 13.51 26.6r 22LY14 266 C~6Ipa 2022 06 03.44086 19 14 18.990 -21 30 19.34 26.8r 22LY14 266 C~6Ipa 2022 06 03.52767 19 14 18.623 -21 30 19.97 26.8r 22LY14 266 C~6Ipa 2022 06 03.61505 19 14 18.253 -21 30 20.58 26.8r 22LY14 266 C~6Ipa 2022 06 29.45230 19 12 15.112 -21 33 56.30 26.6r 22LY14 266 C~6Ipa 2022 06 29.51813 19 12 14.763 -21 33 56.90 26.6r 22LY14 266 C~6Ipa 2022 06 29.58257 19 12 14.423 -21 33 57.48 26.6r 22LY14 266 C~6Ipa 2023 09 09.22891 19 13 40.843 -21 35 19.99 22LY14 266 C~8ecH 2023 09 09.32430 19 13 40.632 -21 35 20.49 22LY14 266 C~8ecH 2023 09 09.41985 19 13 40.423 -21 35 20.96 22LY14 266 C~8ecH 2023 09 10.22905 19 13 38.757 -21 35 25.21 22LY14 266 C~8ecH 2023 09 10.32490 19 13 38.554 -21 35 25.69 22LY14 266 C~8ecH 2023 09 10.42059 19 13 38.354 -21 35 26.15 22LY14 266 C~8ecH
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 0.07 0.00 0.03
2 0.0002 -5.10 0.06 0.03 0.03
3 0.0005 -9.81 0.03 0.08 0.03
4 0.0027 -57.49 -0.04 0.29 0.02
5 0.0030 -62.65 -0.06 0.32 0.01
6 0.0032 -67.85 -0.07 0.37 0.01
7 0.0739 -1799.55 -0.01 1.29 -0.05
8 0.0741 -1804.46 -0.00 1.30 -0.04
9 0.0743 -1809.24 0.01 1.31 -0.04
10 1.2698 -623.41 0.02 -230.76 0.02
11 1.2700 -626.39 0.03 -230.89 0.02
12 1.2703 -629.34 0.03 -230.99 0.02
13 1.2725 -652.93 -0.03 -232.28 -0.02
14 1.2728 -655.80 -0.03 -232.40 -0.02
15 1.2730 -658.62 -0.02 -232.51 -0.02
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.
22LY14 quality flag:1 Type: CLASSICAL 3:1EE CLASSICAL axisobj 45.025 62.277 44.991 ecceobj 0.138 0.488 0.144 incobj 1.879 1.894 1.878 qmin 38.242 31.269 37.911 qmax 52.715 96.352 52.920 amean 45.269 62.629 45.226 amin 44.891 61.576 44.850 amax 45.719 64.087 45.659 emean 0.137 0.490 0.143 emin 0.122 0.478 0.127 emax 0.153 0.503 0.159 imean 1.654 0.861 1.768 imin 0.771 0.773 0.769 imax 2.375 0.936 2.599 excite_mean 0.141 0.490 0.147 fracstop 1.000 1.000 1.000 cjmean 3.093 2.995 3.090 libcent 0 -180.0 180.6 -180.0 libamp 0 -180.0 155.9 -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 166.8 208.5 173.0 kozaiamp 180.0 83.8 179.9