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: 20MF53
# Created Wed Nov 27 02:11:03 2024
# Orbit generated from Bernstein formalism
# Fitting 9 observations of 9
# Arc: 5.15d
# First observation: 2020/06/20
# Last observation: 2020/06/25
Preliminary a, adot, b, bdot, g, gdot:
0.000000 0.013837 -0.000000 0.005414 0.018042 0.000000
# WARNING Fitting with energy constraint
# Chi-squared of fit: 0.03 DOF: 13 RMS: 0.01
# Min/Max residuals: -0.02 0.01
# Exact a, adot, b, bdot, g, gdot:
1.243396E-05 1.431335E-02 4.697281E-06 5.404516E-03 1.811558E-02 2.505270E-03
# Covariance matrix:
5.5477E-11 6.4711E-08 -9.8014E-13 -8.9922E-10 1.0870E-08 -1.7135E-07
6.4711E-08 7.6013E-05 -1.1507E-09 -1.0558E-06 1.2762E-05 -2.0218E-04
-9.8014E-13 -1.1507E-09 3.4919E-13 -1.3519E-11 -1.9321E-10 3.0742E-09
-8.9922E-10 -1.0558E-06 -1.3519E-11 1.9829E-08 -1.7726E-07 2.8293E-06
1.0870E-08 1.2762E-05 -1.9321E-10 -1.7726E-07 2.1428E-06 -3.3862E-05
-1.7135E-07 -2.0218E-04 3.0742E-09 2.8293E-06 -3.3862E-05 9.1341E-04
# lat0 lon0 xBary yBary zBary JD0
2.687224 -72.180590 0.325705 0.044655 -0.954392 2459020.956631
# Heliocentric elements and errors
Epoch: 2459020.5000 = 2020/06/20
Mean Anomaly: 63.54711 +/- 172.318
Argument of Peri: 285.91758 +/- 12.857
Long of Asc Node: 280.50342 +/- 4.324
Inclination: 20.76969 +/- 11.656
Eccentricity: 0.16236016 +/- 1.8732
Semi-Major Axis: 59.06159916 +/- 30.3200
Time of Perihelion: 2429755.4331 +/- 76089.7
Perihelion: 49.47234822 +/- 113.5127
Aphelion: 68.65085010 +/- 116.1127
Period (y) 453.9061 +/- 349.53
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X 16.86210725 +/- 1.3632
Ecliptic Y -53.51109727 +/- 4.2420
Ecliptic Z 2.58836922 +/- 0.2092
Ecliptic XDOT 0.00217149 +/- 0.0009
Ecliptic YDOT 0.00034221 +/- 0.0046
Ecliptic ZDOT 0.00083342 +/- 0.0003
# Distances at JD0 (AU)
Heliocenter to KBO 56.16464945 +/- 4.0622
Geocenter to KBO 55.20111642 +/- 4.4605
# Hcoef: 8.51
The following table shows the complete astrometric record for 20MF53. 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 (20MF53) followed by the observatory code and reference code for the source of the astrometry.
2020 06 20.45583 19 15 43.880 -19 35 18.65 25.9r 20MF53 266 C~6c5f 2020 06 20.52860 19 15 43.608 -19 35 18.85 25.9r 20MF53 266 C~6c5f 2020 06 20.62233 19 15 43.258 -19 35 19.09 25.9r 20MF53 266 C~6c5f 2020 06 22.44948 19 15 36.513 -19 35 24.25 25.9r 20MF53 266 C~6c5f 2020 06 22.52092 19 15 36.243 -19 35 24.46 25.9r 20MF53 266 C~6c5f 2020 06 22.59118 19 15 35.977 -19 35 24.65 25.9r 20MF53 266 C~6c5f 2020 06 25.44823 19 15 25.277 -19 35 33.27 25.9r 20MF53 266 C~6c5f 2020 06 25.52653 19 15 24.976 -19 35 33.51 25.9r 20MF53 266 C~6c5f 2020 06 25.60788 19 15 24.665 -19 35 33.75 25.9r 20MF53 266 C~6c5f
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 0.01 0.00 0.00
2 0.0002 -3.84 0.01 0.30 0.00
3 0.0005 -8.77 0.01 0.70 0.00
4 0.0055 -103.96 -0.02 7.89 -0.00
5 0.0057 -107.77 -0.01 8.17 -0.01
6 0.0058 -111.52 -0.02 8.47 -0.00
7 0.0137 -262.58 0.00 19.41 -0.00
8 0.0139 -266.83 0.00 19.72 0.00
9 0.0141 -271.22 0.01 20.05 0.00
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.
20MF53 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