Orbit Fit and Astrometric record for 20BR60

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: 20BR60    
# Created Tue Apr  1 01:11:18 2025
# Orbit generated from Bernstein formalism
# Fitting      6 observations of      6
# Arc:   0.97y
# First observation: 2020/01/26
#  Last observation: 2021/01/16
Preliminary a, adot, b, bdot, g, gdot:
  -0.000001   0.011207  -0.000001   0.000690   0.016134   0.000000
# WARNING Fitting with energy constraint
# WARNING MRQMIN stopped after  13 iterations -- oscilliatory solution
# Chi-squared of fit:     3.14 DOF:      7 RMS:  0.13
# Min/Max residuals:    -0.18    0.19
# Exact a, adot, b, bdot, g, gdot:
  1.053931E-05  1.113958E-02  1.173832E-08  6.873425E-04  1.621137E-02 -3.977000E-03
# Covariance matrix:
  1.5283E-12  8.3681E-11 -1.0661E-14  4.9768E-12  9.1899E-11  7.4277E-09
  8.3681E-11  8.9712E-09 -1.1381E-12  5.2859E-10  9.7673E-09  7.8899E-07
 -1.0661E-14 -1.1381E-12  7.3254E-13 -8.5200E-13 -1.2477E-12 -1.0031E-10
  4.9768E-12  5.2859E-10 -8.5200E-13  3.2412E-11  5.7570E-10  4.6497E-08
  9.1899E-11  9.7673E-09 -1.2477E-12  5.7570E-10  1.0647E-08  8.5942E-07
  7.4277E-09  7.8899E-07 -1.0031E-10  4.6497E-08  8.5942E-07  6.9406E-05
#      lat0       lon0       xBary       yBary       zBary        JD0
   -6.274728  121.697225   -0.062149   -0.108266   -0.984992  2458874.638531
# Heliocentric elements and errors
Epoch:              2458870.5000  =  2020/01/22
Mean Anomaly:          263.65333 +/-   101.291
Argument of Peri:       73.43912 +/-    60.037
Long of Asc Node:      181.63813 +/-     0.503
Inclination:             7.13131 +/-     0.037
Eccentricity:         0.36837411 +/-    0.4060
Semi-Major Axis:     54.11117104 +/-   19.2614
Time of Perihelion: 2497780.6606 +/-   35238.6
Perihelion:          34.17801649 +/-   25.1111
Aphelion:            74.04432560 +/-   34.3109
Period (y)              398.0509 +/-    212.54
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -32.78714352 +/-    0.2050
Ecliptic Y           52.97224639 +/-    0.3321
Ecliptic Z           -6.74199336 +/-    0.0429
Ecliptic XDOT        -0.00124827 +/-    0.0007
Ecliptic YDOT        -0.00154350 +/-    0.0012
Ecliptic ZDOT         0.00018857 +/-    0.0002
# Distances at JD0 (AU)
Heliocenter to KBO   62.66187152 +/-    0.3006
Geocenter to KBO     61.68509345 +/-    0.3926
# Hcoef:  6.91

The following table shows the complete astrometric record for 20BR60. 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 (20BR60) followed by the observatory code and reference code for the source of the astrometry.

2020 01  26.13773  08 10 02.992  +13 39 31.54  25.0r 20BR60    807  C~4Zh3      
2020 01  27.17729  08 09 59.364  +13 39 43.76  25.0r 20BR60    807  C~4Zh3      
2020 12  16.25246  08 14 49.585  +13 27 23.64  24.6r 20BR60    304  C~4Zh3      
2020 12  17.26821  08 14 46.842  +13 27 29.45  24.5r 20BR60    304  C~4Zh3      
2021 01  15.15796  08 13 14.610  +13 31 34.65        20BR60    304  C~4Zh3      
2021 01  16.13943  08 13 11.207  +13 31 45.64        20BR60    304  C~4Zh3      

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     0.14
     2   0.0028    -54.27    -0.07       0.56    -0.14
     3   0.8901   4237.97    -0.18     198.41    -0.14
     4   0.8929   4197.64     0.19     195.28     0.16
     5   0.9720   2830.90    -0.06     139.83    -0.12
     6   0.9747   2780.06     0.06     139.72     0.10

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.

20BR60    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