Orbit Fit and Astrometric record for 07TQ436

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: 07TQ436   
# Created Sat Apr 27 01:13:02 2024
# Orbit generated from Bernstein formalism
# Fitting      7 observations of      7
# Arc:  53.81d
# First observation: 2007/10/14
#  Last observation: 2007/12/07
Preliminary a, adot, b, bdot, g, gdot:
  -0.000001   0.054917   0.000002   0.006841   0.036452   0.000000
# WARNING Fitting with energy constraint
# Chi-squared of fit:    10.15 DOF:      9 RMS:  0.21
# Min/Max residuals:    -0.28    0.42
# Exact a, adot, b, bdot, g, gdot:
  1.819686E-05  4.227155E-02  3.726262E-06  7.021194E-03  3.451870E-02  2.938038E-02
# Covariance matrix:
  5.7928E-13  1.8453E-10  2.0860E-14 -3.1615E-12  2.6874E-11 -2.7522E-09
  1.8453E-10  3.9248E-07  4.7845E-11 -7.1877E-09  5.3889E-08 -6.3403E-06
  2.0860E-14  4.7845E-11  4.5335E-13 -4.5035E-12  6.5184E-12 -7.8734E-10
 -3.1615E-12 -7.1877E-09 -4.5035E-12  1.8940E-10 -9.7994E-10  1.1809E-07
  2.6874E-11  5.3889E-08  6.5184E-12 -9.7994E-10  7.4260E-09 -8.6350E-07
 -2.7522E-09 -6.3403E-06 -7.8734E-10  1.1809E-07 -8.6350E-07  1.0442E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
   -0.262153   14.456766   -0.108534   -0.004485   -0.994015  2454387.782024
# Heliocentric elements and errors
Epoch:              2454380.5000  =  2007/10/07
Mean Anomaly:            6.10348 +/-    11.911
Argument of Peri:      279.83944 +/-     5.540
Long of Asc Node:       16.17691 +/-     0.026
Inclination:             9.45794 +/-     0.159
Eccentricity:         0.82152398 +/-    0.2610
Semi-Major Axis:    107.10384184 +/-  139.0912
Time of Perihelion: 2447516.4397 +/-     807.9
Perihelion:          19.11546738 +/-   37.3877
Aphelion:           195.09221630 +/-  254.8957
Period (y)             1108.4492 +/-   2159.24
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           28.98689350 +/-    0.0700
Ecliptic Y            7.58110842 +/-    0.0180
Ecliptic Z           -0.13242481 +/-    0.0003
Ecliptic XDOT         0.00142824 +/-    0.0008
Ecliptic YDOT         0.00382772 +/-    0.0002
Ecliptic ZDOT         0.00054612 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   29.96215506 +/-    0.0679
Geocenter to KBO     28.96980722 +/-    0.0723
# Hcoef: 11.15

The following table shows the complete astrometric record for 07TQ436. 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 (07TQ436) followed by the observatory code and reference code for the source of the astrometry.

2007 10  14.28127  00 53 38.40   +05 27 26.7   25.5R 07TQ436   568  Cz6780      
2007 10  14.34479  00 53 37.98   +05 27 24.4         07TQ436   568  Cz6780      
2007 10  14.40680  00 53 37.59   +05 27 22.3         07TQ436   568  Cz6780      
2007 11  14.09305  00 50 47.45   +05 11 52.8         07TQ436   807  Cz6780      
2007 11  14.14236  00 50 47.25   +05 11 51.6         07TQ436   807  Cz6780      
2007 12  07.06250  00 49 27.85   +05 05 16.5         07TQ436   807  Cz6780      
2007 12  07.09027  00 49 27.78   +05 05 16.4         07TQ436   807  Cz6780      

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    -0.11
     2   0.0002     -6.67    -0.12       0.31    -0.10
     3   0.0003    -12.86    -0.12       0.62    -0.07
     4   0.0844  -2715.74    -0.21     128.35     0.42
     5   0.0845  -2718.96     0.21     128.40     0.24
     6   0.1472  -3965.84     0.01     224.85    -0.28
     7   0.1473  -3966.84    -0.00     225.16    -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.

07TQ436    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