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: 22LO14
# Created Wed Nov 27 02:11:10 2024
# Orbit generated from Bernstein formalism
# Fitting 9 observations of 9
# Arc: 28.14d
# First observation: 2022/06/02
# Last observation: 2022/06/30
Preliminary a, adot, b, bdot, g, gdot:
0.000000 0.027833 0.000000 -0.000192 0.025517 0.000000
# WARNING Fitting with energy constraint
# Chi-squared of fit: 0.00 DOF: 13 RMS: 0.00
# Min/Max residuals: -0.01 0.01
# Exact a, adot, b, bdot, g, gdot:
1.564667E-05 2.455571E-02 -9.722178E-08 -1.760929E-04 2.484029E-02 -2.628811E-03
# Covariance matrix:
4.8931E-11 7.7471E-08 -3.2925E-13 -3.7922E-10 1.4546E-08 5.6860E-07
7.7471E-08 1.2391E-04 -5.2653E-10 -6.0650E-07 2.3259E-05 9.0595E-04
-3.2925E-13 -5.2653E-10 4.8632E-13 -3.8696E-12 -9.8862E-11 -3.8693E-09
-3.7922E-10 -6.0650E-07 -3.8696E-12 3.0976E-09 -1.1385E-07 -4.4381E-06
1.4546E-08 2.3259E-05 -9.8862E-11 -1.1385E-07 4.3681E-06 1.7152E-04
5.6860E-07 9.0595E-04 -3.8693E-09 -4.4381E-06 1.7152E-04 7.5775E-03
# lat0 lon0 xBary yBary zBary JD0
0.660881 -72.630962 0.600911 0.009168 -0.818166 2459732.944521
# Heliocentric elements and errors
Epoch: 2459730.5000 = 2022/05/31
Mean Anomaly: 291.87596 +/- 177.141
Argument of Peri: 204.31373 +/- 192.920
Long of Asc Node: 164.62667 +/- 8.103
Inclination: 0.76302 +/- 0.069
Eccentricity: 0.12769505 +/- 3.4399
Semi-Major Axis: 42.47061362 +/- 14.4367
Time of Perihelion: 2478861.1229 +/- 48779.2
Perihelion: 37.04732631 +/- 146.6352
Aphelion: 47.89390094 +/- 146.9977
Period (y) 276.7840 +/- 141.13
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X 11.69730071 +/- 1.0109
Ecliptic Y -39.38109056 +/- 3.2326
Ecliptic Z 0.46441067 +/- 0.0391
Ecliptic XDOT 0.00249839 +/- 0.0038
Ecliptic YDOT 0.00109325 +/- 0.0089
Ecliptic ZDOT -0.00002286 +/- 0.0001
# Distances at JD0 (AU)
Heliocenter to KBO 41.08421613 +/- 3.1119
Geocenter to KBO 40.25717211 +/- 3.3872
# Hcoef: 7.97
The following table shows the complete astrometric record for 22LO14. 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 (22LO14) followed by the observatory code and reference code for the source of the astrometry.
2022 06 02.44372 19 14 56.156 -21 39 21.23 24.0r 22LO14 266 C~6IpZ 2022 06 02.53086 19 14 55.800 -21 39 21.82 24.0r 22LO14 266 C~6IpZ 2022 06 02.61096 19 14 55.471 -21 39 22.35 24.0r 22LO14 266 C~6IpZ 2022 06 29.45230 19 12 50.206 -21 42 56.40 23.9r 22LO14 266 C~6IpZ 2022 06 29.51813 19 12 49.862 -21 42 56.98 23.9r 22LO14 266 C~6IpZ 2022 06 29.58257 19 12 49.527 -21 42 57.54 23.9r 22LO14 266 C~6IpZ 2022 06 30.45132 19 12 45.077 -21 43 05.28 24.1r 22LO14 266 C~6IpZ 2022 06 30.51894 19 12 44.723 -21 43 05.88 24.1r 22LO14 266 C~6IpZ 2022 06 30.58668 19 12 44.369 -21 43 06.46 24.1r 22LO14 266 C~6IpZ
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 -0.00 0.00 -0.00
2 0.0002 -5.00 0.01 0.05 0.00
3 0.0005 -9.61 -0.00 0.11 0.00
4 0.0739 -1768.70 0.00 7.90 -0.00
5 0.0741 -1773.53 -0.00 7.92 -0.00
6 0.0743 -1778.23 0.00 7.94 -0.01
7 0.0767 -1840.73 0.00 7.97 0.00
8 0.0769 -1845.70 -0.00 7.99 0.00
9 0.0771 -1850.67 -0.00 8.03 0.01
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.
22LO14 quality flag:0 Type: ERR2LARGE ERR2LARGE ERR2LARGE axisobj 0.000 0.000 0.000 ecceobj -1.000 -1.000 -1.000 incobj -1.000 -1.000 -1.000 qmin 0.000 0.000 0.000 qmax 0.000 0.000 0.000 amean 0.000 0.000 0.000 amin 0.000 0.000 0.000 amax 0.000 0.000 0.000 emean 0.000 0.000 0.000 emin 0.000 0.000 0.000 emax 0.000 0.000 0.000 imean 0.000 0.000 0.000 imin 0.000 0.000 0.000 imax 0.000 0.000 0.000 excite_mean 0.000 0.000 0.000 fracstop 0.000 0.000 0.000 cjmean 0.000 0.000 0.000 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 0.0 0.0 0.0 kozaiamp 0.0 0.0 0.0