Orbit Fit and Astrometric record for 10TP182

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: 10TP182   
# Created Sat Oct 21 01:37:54 2017
# Orbit generated from Bernstein formalism
# Fitting   37 observations of   38
# Arc:   1.96y
# First observation: 2008/10/29
#  Last observation: 2010/10/15
Preliminary a, adot, b, bdot, g, gdot:
   0.000038   0.027042   0.000038  -0.004639   0.025611   0.000000
# Chi-squared of fit:    93.28 DOF:   68 RMS:  0.28
# Min/Max residuals:    -0.87    0.73
# Exact a, adot, b, bdot, g, gdot:
  1.714946E-05  2.680903E-02 -1.526000E-06 -4.587852E-03  2.591675E-02 -3.693721E-03
# Covariance matrix:
  2.2036E-13 -1.9444E-13 -8.8369E-16  7.0301E-15  1.9453E-13 -7.7730E-13
 -1.9444E-13  1.0074E-12  3.0633E-14 -1.5073E-13  2.2193E-13  1.5932E-11
 -8.8369E-16  3.0633E-14  8.3849E-14 -6.0204E-14  1.4444E-14  5.7174E-13
  7.0301E-15 -1.5073E-13 -6.0204E-14  9.7455E-14 -6.5848E-14 -2.7766E-12
  1.9453E-13  2.2193E-13  1.4444E-14 -6.5848E-14  4.9627E-13  6.8934E-12
 -7.7730E-13  1.5932E-11  5.7174E-13 -2.7766E-12  6.8934E-12  2.9302E-10
#      lat0       lon0       xBary       yBary       zBary        JD0
    0.273939   28.179889   -0.143795    0.004745   -0.984138  2454768.897284
# Heliocentric elements and errors
Epoch:              2454760.5000  =  2008/10/21
Mean Anomaly:          321.20197 +/-     0.079
Argument of Peri:      232.39080 +/-     0.140
Long of Asc Node:      209.94152 +/-     0.000
Inclination:             9.71714 +/-     0.001
Eccentricity:         0.17761858 +/-    0.0006
Semi-Major Axis:     45.12617750 +/-    0.0108
Time of Perihelion: 2466693.4678 +/-      23.8
Perihelion:          37.11093007 +/-    0.0266
Aphelion:            53.14142493 +/-    0.0281
Period (y)              303.1454 +/-      0.11
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           34.81221590 +/-    0.0009
Ecliptic Y           18.80867283 +/-    0.0005
Ecliptic Z            0.18441788 +/-    0.0000
Ecliptic XDOT        -0.00167341 +/-    0.0000
Ecliptic YDOT         0.00231566 +/-    0.0000
Ecliptic ZDOT        -0.00048664 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   39.56880791 +/-    0.0008
Geocenter to KBO     38.58509047 +/-    0.0010
# Hcoef:  6.56

The following table shows the complete astrometric record for 10TP182. 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 (10TP182) followed by the observatory code and reference code for the source of the astrometry.

2008 10  29.396530 01 44 18.26   +11 04 58.9   22.3V 10TP182   645  C~1Qdp      
2008 10  29.397360 01 44 18.26   +11 04 58.9   22.0V 10TP182   645  C~1Qdp      
2008 10  29.399847 01 44 18.25   +11 04 58.9   22.8V 10TP182   645  C~1Qdp      
2008 11  02.383128 01 43 59.35   +11 03 01.0   22.7V 10TP182   645  C~262w      
2008 11  02.383957 01 43 59.35   +11 03 01.0   22.1V 10TP182   645  C~262w      
2008 11  02.386445 01 43 59.34   +11 03 00.9   23.2V 10TP182   645  C~262w      
2009 01  30.21618  01 41 19.98   +10 43 29.3         10TP182   568  C~0j6g      
2009 01  30.21880  01 41 19.98   +10 43 29.3         10TP182   568  C~0j6g      
2009 01  30.22175  01 41 19.99   +10 43 29.5         10TP182   568  C~0j6g      
2009 01  30.22541  01 41 19.99   +10 43 29.3         10TP182   568  C~0j6g      
2009 01  31.21545  01 41 22.26   +10 43 39.3         10TP182   568  C~0j6g      
2009 01  31.21933  01 41 22.27   +10 43 39.2         10TP182   568  C~0j6g      
2009 01  31.22161  01 41 22.28   +10 43 39.3         10TP182   568  C~0j6g      
2009 01  31.22519  01 41 22.28   +10 43 39.2         10TP182   568  C~0j6g      
2009 01  31.22929  01 41 22.31   +10 43 39.6         10TP182   568  C~0j6g      
2009 01  31.23295  01 41 22.31   +10 43 39.6         10TP182   568  C~0j6g      
2009 01  31.23586  01 41 22.32   +10 43 39.7         10TP182   568  C~0j6g      
2009 01  31.23869  01 41 22.33   +10 43 39.7         10TP182   568  C~0j6g      
2009 01  31.30414  01 41 22.48   +10 43 40.4         10TP182   568  C~0j6g      
2009 01  31.30639  01 41 22.50   +10 43 40.3         10TP182   568  C~0j6g      
2009 01  31.30995  01 41 22.49   +10 43 40.4         10TP182   568  C~0j6g      
2009 01  31.31326  01 41 22.50   +10 43 40.4         10TP182   568  C~0j6g      
2009 10  18.30129  01 51 29.15   +11 28 36.8   22.0r 10TP182   568  C~0j6g      
2009 10  18.40160  01 51 28.66   +11 28 33.8   22.1r 10TP182   568  C~0j6g      
2009 10  18.52862  01 51 28.04   +11 28 30.0   22.0r 10TP182   568  C~0j6g      
2009 11  22.23575  01 48 47.53   +11 12 04.6   22.8r 10TP182   568  C~0j6g      
2009 11  22.27811  01 48 47.34   +11 12 03.3   22.3r 10TP182   568  C~0j6g      
2009 12  21.27215  01 47 19.43   +11 02 34.6   22.1r 10TP182   568  C~0j6g      
2009 12  21.38381  01 47 19.20   +11 02 32.3   22.3r 10TP182   568  C~0j6g      
2010 10  07.38344  01 58 42.23   +11 51 35.5   22.6w 10TP182   F51  C~0SWU      
2010 10  07.39872  01 58 42.16   +11 51 35.0   22.6w 10TP182   F51  C~0SWU      
2010 10  07.41469  01 58 42.08   +11 51 34.6   22.7w 10TP182   F51  C~0SWU      
2010 10  12.47721  01 58 18.33   +11 49 11.2   22.8w 10TP182   F51  C~0SWU      
2010 10  12.49318  01 58 18.24   +11 49 10.8   22.6w 10TP182   F51  C~0SWU      
2010 10  12.50847  01 58 18.17   +11 49 10.4   22.8w 10TP182   F51  C~0SWU      
2010 10  12.52375  01 58 18.10   +11 49 10.2   22.6w 10TP182   F51  C~0SWU      
2010 10  15.42728  01 58 04.16   +11 47 46.9         10TP182   675  C~0j6g      
2010 10  15.47121  01 58 03.92   +11 47 45.7         10TP182   675  C~0j6g      

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    -0.16       0.00    -0.26
  2   0.0000      0.00    -0.10       0.00    -0.26
  3   0.0000     -0.14    -0.04       0.05    -0.20
  4   0.0109   -302.13    -0.03     -10.62    -0.23
  5   0.0109   -302.13     0.04     -10.62    -0.22
  6   0.0109   -302.30     0.05     -10.66    -0.26
  7   0.2541  -2913.87    -0.03    -262.68     0.10
  8   0.2541  -2913.87    -0.12    -262.68     0.10
  9   0.2541  -2913.66    -0.01    -262.55     0.25
 10   0.2542  -2913.73    -0.20    -262.74     0.07
 11   0.2569  -2878.91    -0.14    -265.43     0.17
 12   0.2569  -2878.81    -0.18    -265.58     0.04
 13   0.2569  -2878.64    -0.08    -265.54     0.08
 14   0.2569  -2878.67    -0.24    -265.63    -0.00
 15   0.2569  -2878.12     0.17    -265.42     0.22
 16   0.2569  -2878.12     0.04    -265.42     0.23
 17   0.2569  -2877.94     0.11    -265.38     0.28
 18   0.2569  -2877.81     0.15    -265.43     0.23
 19   0.2571  -2875.49     0.17    -265.57     0.27
 20   0.2571  -2875.25     0.33    -265.77     0.07
 21   0.2571  -2875.35     0.11    -265.63     0.23
 22   0.2571  -2875.22     0.13    -265.68     0.19
 23   0.9689   6431.65    -0.06    -921.10    -0.73
 24   0.9692   6423.85    -0.01    -921.38    -0.80
 25   0.9696   6413.97     0.08    -921.73    -0.87
 26   1.0646   3855.83     0.36   -1011.16     0.32
 27   1.0647   3852.75     0.05   -1011.39     0.18
 28   1.1441   2440.96 (   0.14)  -1084.66 (   1.42)
 29   1.1444   2436.97    -0.35   -1085.61     0.72
 30   1.9384  12890.09     0.25   -1848.76    -0.06
 31   1.9384  12888.95     0.25   -1848.87    -0.14
 32   1.9384  12887.70     0.20   -1848.84    -0.08
 33   1.9523  12509.52     0.08   -1862.76    -0.35
 34   1.9524  12508.13    -0.08   -1862.68    -0.23
 35   1.9524  12507.03    -0.01   -1862.70    -0.21
 36   1.9524  12505.99     0.13   -1862.53    -0.01
 37   1.9604  12284.33    -0.27   -1869.81     0.53
 38   1.9605  12280.59    -0.60   -1869.72     0.73

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.

10TP182    quality flag:1

Type:       SCATNEAR  SCATEXTD 11:6EEEEE

axisobj        45.551    45.582    45.521
ecceobj         0.184     0.185     0.183
incobj          9.679     9.679     9.679
qmin           35.876    35.821    36.376
qmax           54.955    54.738    54.340
amean          45.099    45.190    45.102
amin           44.635    44.786    44.657
amax           45.659    45.668    45.594
emean           0.181     0.183     0.179
emin            0.156     0.167     0.166
emax            0.205     0.203     0.192
imean          10.663    10.567    10.653
imin            9.612     9.717     9.976
imax           11.670    11.667    11.321
excite_mean     0.259     0.259     0.258
fracstop        1.000     1.000     1.000
cjmean          3.033     3.034     3.034

libcent 0      -180.0    -180.0     178.3
libamp  0      -180.0    -180.0     177.2
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       187.3     181.1     178.2
kozaiamp        180.0     180.0     180.0