Orbit Fit and Astrometric record for 11UR411

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: 11UR411   
# Created Fri Apr 19 01:13:52 2024
# Orbit generated from Bernstein formalism
# Fitting     21 observations of     21
# Arc:   4.04y
# First observation: 2011/10/25
#  Last observation: 2015/11/08
Preliminary a, adot, b, bdot, g, gdot:
  -0.000207   0.030688  -0.000118   0.015151   0.027382   0.000000
# Chi-squared of fit:    11.74 DOF:     36 RMS:  0.13
# Min/Max residuals:    -0.30    0.23
# Exact a, adot, b, bdot, g, gdot:
  1.697159E-05  2.993666E-02  9.179708E-06  1.475017E-02  2.773604E-02 -6.035494E-03
# Covariance matrix:
  1.0828E-13 -1.2009E-13  8.8485E-15 -4.6188E-14  2.3219E-14 -7.8165E-13
 -1.2009E-13  5.6989E-13 -4.9428E-14  2.7131E-13  3.7598E-14  4.5858E-12
  8.8485E-15 -4.9428E-14  9.5868E-14 -5.7699E-14  2.7996E-15 -4.3593E-13
 -4.6188E-14  2.7131E-13 -5.7699E-14  1.8941E-13  1.5318E-14  2.3861E-12
  2.3219E-14  3.7598E-14  2.7996E-15  1.5318E-14  3.8369E-13  2.4633E-13
 -7.8165E-13  4.5858E-12 -4.3593E-13  2.3861E-12  2.4633E-13  4.0332E-11
#      lat0       lon0       xBary       yBary       zBary        JD0
    4.695605   32.585917    0.019292    0.081110   -0.987509  2455859.855936
# Heliocentric elements and errors
Epoch:              2455850.5000  =  2011/10/16
Mean Anomaly:          347.49339 +/-     0.011
Argument of Peri:       44.66301 +/-     0.032
Long of Asc Node:       23.34433 +/-     0.000
Inclination:            26.53636 +/-     0.000
Eccentricity:         0.43935999 +/-    0.0001
Semi-Major Axis:     62.55144285 +/-    0.0118
Time of Perihelion: 2462128.0691 +/-       5.1
Perihelion:          35.06884130 +/-    0.0102
Aphelion:            90.03404439 +/-    0.0187
Period (y)              494.7254 +/-      0.14
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           31.12514516 +/-    0.0007
Ecliptic Y           19.87116980 +/-    0.0004
Ecliptic Z            2.95179575 +/-    0.0001
Ecliptic XDOT        -0.00219586 +/-    0.0000
Ecliptic YDOT         0.00211103 +/-    0.0000
Ecliptic ZDOT         0.00140241 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   37.04525811 +/-    0.0006
Geocenter to KBO     36.05417039 +/-    0.0008
# Hcoef:  8.52

The following table shows the complete astrometric record for 11UR411. 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 (11UR411) followed by the observatory code and reference code for the source of the astrometry.

2011 10  25.35517  01 54 49.862  +16 46 30.48  24.1r 11UR411   568  C~1C6O      
2011 10  25.35517  01 54 49.84   +16 46 30.4         11UR411   568  C~3j8g      
2011 10  25.40962  01 54 49.553  +16 46 29.49  24.1r 11UR411   568  C~1C6O      
2011 10  26.31377  01 54 44.538  +16 46 10.59  23.9r 11UR411   568  C~1C6O      
2011 10  26.31377  01 54 44.53   +16 46 10.7   23.8r 11UR411   568  C~3j8g      
2011 10  26.35693  01 54 44.296  +16 46 09.65  24.1r 11UR411   568  C~1C6O      
2011 10  26.35693  01 54 44.28   +16 46 09.8   23.8r 11UR411   568  C~3j8g      
2011 10  26.41449  01 54 43.962  +16 46 08.37  23.9r 11UR411   568  C~1C6O      
2011 10  26.41449  01 54 43.95   +16 46 08.5   23.8r 11UR411   568  C~3j8g      
2011 10  31.40568  01 54 16.331  +16 44 21.90        11UR411   568  C~1C6O      
2011 10  31.42313  01 54 16.232  +16 44 21.65        11UR411   568  C~1C6O      
2011 11  24.29202  01 52 13.405  +16 35 47.22  24.3r 11UR411   568  C~1C6O      
2011 11  30.33825  01 51 46.770  +16 33 47.70  24.3r 11UR411   568  C~1C6O      
2012 01  26.31221  01 50 19.057  +16 26 59.55  24.5r 11UR411   568  C~1C6O      
2012 08  21.48978  02 04 57.770  +18 19 06.34  24.1r 11UR411   568  C~1C6O      
2012 08  24.55204  02 04 51.641  +18 19 27.51  24.4r 11UR411   568  C~1C6O      
2012 10  17.39531  02 01 04.179  +18 12 40.55  24.0r 11UR411   568  C~1C6O      
2012 10  20.49106  02 00 46.860  +18 11 41.63  24.0r 11UR411   568  C~1C6O      
2013 02  06.27170  01 56 02.918  +17 50 44.72  24.6r 11UR411   568  C~1C6O      
2015 11  08.26706  02 16 39.67   +22 18 48.2   23.8R 11UR411   G37  C~1ddG      
2015 11  08.33351  02 16 39.25   +22 18 46.4         11UR411   G37  C~1ddG      

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     0.02       0.00    -0.16
     2   0.0000     -0.32    -0.30       0.04    -0.12
     3   0.0001     -4.50     0.05       0.63    -0.02
     4   0.0026    -78.66    -0.00       8.28     0.19
     5   0.0026    -78.59     0.06       8.14     0.04
     6   0.0027    -82.33    -0.09       8.70     0.22
     7   0.0027    -82.17     0.07       8.48    -0.00
     8   0.0029    -87.23    -0.19       9.14     0.15
     9   0.0029    -87.11    -0.07       8.96    -0.03
    10   0.0166   -496.13    -0.04      48.32     0.03
    11   0.0166   -497.55    -0.01      48.58     0.16
    12   0.0820  -2330.77     0.07     188.21    -0.06
    13   0.0985  -2731.28     0.19     211.71    -0.05
    14   0.2545  -4055.88     0.11     277.26    -0.13
    15   0.8245  10082.75    -0.07    2228.91    -0.04
    16   0.8328  10007.58     0.11    2278.35    -0.19
    17   0.9803   6816.84     0.20    2997.21    -0.05
    18   0.9887   6564.52     0.11    3026.36    -0.13
    19   1.2866   2326.95    -0.16    3246.37     0.13
    20   4.0381  24266.80     0.23   12637.72     0.15
    21   4.0383  24260.60    -0.27   12637.86    -0.09

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.

11UR411    quality flag:3

Type:       SCATNEAR  SCATNEAR  SCATNEAR

axisobj        62.737    62.769    62.705
ecceobj         0.440     0.441     0.440
incobj         26.509    26.509    26.509
qmin           33.850    33.902    33.847
qmax           91.457    91.560    91.585
amean          61.967    61.997    61.929
amin           61.228    61.215    61.185
amax           63.035    63.057    63.010
emean           0.434     0.434     0.434
emin            0.414     0.414     0.414
emax            0.453     0.454     0.454
imean          26.380    26.393    26.375
imin           25.660    25.652    25.666
imax           27.371    27.380    27.370
excite_mean     0.621     0.621     0.621
fracstop        1.000     1.000     1.000
cjmean          2.801     2.801     2.801

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       159.4     159.1     159.7
kozaiamp        180.0     180.0     180.0