Orbit Fit and Astrometric record for 20MN53

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: 20MN53    
# Created Fri Nov  1 01:10:44 2024
# Orbit generated from Bernstein formalism
# Fitting      6 observations of      6
# Arc:   3.17d
# First observation: 2020/06/22
#  Last observation: 2020/06/25
# WARNING Fitting with energy constraint
# WARNING and with gdot fixed = 0
# WARNING MRQMIN stopped after  13 iterations -- oscilliatory solution
# Chi-squared of fit:    16.63 DOF:      8 RMS:  0.29
# Min/Max residuals:    -0.45    0.47
# Exact a, adot, b, bdot, g, gdot:
  1.603985E-05  2.488902E-02  2.969805E-06  8.058410E-03  2.648988E-02  0.000000E+00
# Covariance matrix:
  5.0604E-11  8.3698E-08 -4.9093E-13 -7.6206E-10  1.4042E-08  0.0000E+00
  8.3698E-08  1.3985E-04 -8.1967E-10 -1.2724E-06  2.3446E-05  0.0000E+00
 -4.9093E-13 -8.1967E-10  4.4864E-13 -4.6052E-11 -1.3743E-10  0.0000E+00
 -7.6206E-10 -1.2724E-06 -4.6052E-11  2.5960E-08 -2.1333E-07  0.0000E+00
  1.4042E-08  2.3446E-05 -1.3743E-10 -2.1333E-07  3.9310E-06  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  2.4460E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
    1.892543  -72.274568    0.291998    0.031771   -0.965706  2459022.950281
# Heliocentric elements and errors
Epoch:              2459020.5000  =  2020/06/20
Mean Anomaly:          192.23289 +/-   154.301
Argument of Peri:      174.62750 +/-   142.718
Long of Asc Node:      281.60323 +/-     2.775
Inclination:            17.98538 +/-     8.114
Eccentricity:         0.03813616 +/-    0.6086
Semi-Major Axis:     37.33163612 +/-   19.2100
Time of Perihelion: 2497846.1088 +/-  200104.1
Perihelion:          35.90795088 +/-   29.2859
Aphelion:            38.75532135 +/-   30.2317
Period (y)              228.0992 +/-    176.06
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           11.50885564 +/-    0.8595
Ecliptic Y          -36.95452081 +/-    2.6899
Ecliptic Z            1.24689349 +/-    0.0933
Ecliptic XDOT         0.00244993 +/-    0.0011
Ecliptic YDOT         0.00081324 +/-    0.0016
Ecliptic ZDOT         0.00083219 +/-    0.0001
# Distances at JD0 (AU)
Heliocenter to KBO   38.72525157 +/-    2.5796
Geocenter to KBO     37.75026045 +/-    2.8255
# Hcoef: 10.88

The following table shows the complete astrometric record for 20MN53. 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 (20MN53) followed by the observatory code and reference code for the source of the astrometry.

2020 06  22.44948  19 15 46.321  -20 23 19.20  26.3r 20MN53    266  C~6c5f      
2020 06  22.52092  19 15 45.957  -20 23 19.86  26.3r 20MN53    266  C~6c5f      
2020 06  22.59118  19 15 45.599  -20 23 20.50  26.3r 20MN53    266  C~6c5f      
2020 06  25.44823  19 15 30.275  -20 23 32.25  27.0r 20MN53    266  C~6c5f      
2020 06  25.53072  19 15 29.847  -20 23 33.03  27.0r 20MN53    266  C~6c5f      
2020 06  25.61487  19 15 29.412  -20 23 33.81  27.0r 20MN53    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    -0.24       0.00     0.38
     2   0.0002     -5.16     0.02       0.01    -0.02
     3   0.0004    -10.23     0.26       0.02    -0.41
     4   0.0082   -225.41    -0.30      16.16     0.47
     5   0.0084   -231.47    -0.01      16.16     0.02
     6   0.0087   -237.64     0.29      16.18    -0.45

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.

20MN53    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