Orbit Fit and Astrometric record for 15KV190

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: 15KV190   
# Created Tue May  7 01:16:39 2024
# Orbit generated from Bernstein formalism
# Fitting      5 observations of      5
# Arc:  25.10d
# First observation: 2015/05/18
#  Last observation: 2015/06/12
Preliminary a, adot, b, bdot, g, gdot:
   0.000001   0.015404   0.000000  -0.000448   0.017898   0.000000
# WARNING Fitting with energy constraint
# Chi-squared of fit:     1.65 DOF:      5 RMS:  0.10
# Min/Max residuals:    -0.13    0.18
# Exact a, adot, b, bdot, g, gdot:
  1.244708E-05  1.316719E-02 -4.175783E-07 -7.069853E-04  1.755491E-02  6.545604E-03
# Covariance matrix:
  2.4397E-11  2.6061E-08  2.2108E-12  2.9591E-09  4.4365E-09 -3.7154E-08
  2.6061E-08  2.8413E-05  2.4096E-09  3.2252E-06  4.8353E-06 -4.0624E-05
  2.2108E-12  2.4096E-09  6.8420E-13  2.6640E-10  4.1007E-10 -3.4469E-09
  2.9591E-09  3.2252E-06  2.6640E-10  3.6637E-07  5.4886E-07 -4.6205E-06
  4.4365E-09  4.8353E-06  4.1007E-10  5.4886E-07  8.2295E-07 -6.8480E-06
 -3.7154E-08 -4.0624E-05 -3.4469E-09 -4.6205E-06 -6.8480E-06  1.2224E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
   19.856848 -130.261559   -0.128179    0.340297   -0.941988  2457160.836278
# Heliocentric elements and errors
Epoch:              2457160.5000  =  2015/05/18
Mean Anomaly:           59.77007 +/-    63.101
Argument of Peri:      345.82170 +/-    42.235
Long of Asc Node:      130.92867 +/-    10.669
Inclination:            19.74123 +/-     0.551
Eccentricity:         0.44979434 +/-    0.7217
Semi-Major Axis:     60.04654117 +/-   31.1766
Time of Perihelion: 2428943.4446 +/-   20112.0
Perihelion:          33.03794656 +/-   46.6082
Aphelion:            87.05513579 +/-   62.6186
Period (y)              465.3077 +/-    362.39
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -35.17807747 +/-    1.7895
Ecliptic Y          -41.73247290 +/-    2.1126
Ecliptic Z           19.34910919 +/-    0.9999
Ecliptic XDOT         0.00091951 +/-    0.0015
Ecliptic YDOT        -0.00209456 +/-    0.0010
Ecliptic ZDOT         0.00024312 +/-    0.0005
# Distances at JD0 (AU)
Heliocenter to KBO   57.90927780 +/-    1.9003
Geocenter to KBO     56.96413479 +/-    2.9437
# Hcoef:  7.97

The following table shows the complete astrometric record for 15KV190. 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 (15KV190) followed by the observatory code and reference code for the source of the astrometry.

2015 05  18.33550  15 30 12.139  +01 29 53.45  25.5r 15KV190   568  C~4451      
2015 05  18.41907  15 30 11.851  +01 29 54.57        15KV190   568  C~4451      
2015 05  18.50510  15 30 11.549  +01 29 55.19        15KV190   568  C~4451      
2015 06  11.33340  15 28 51.329  +01 32 26.12        15KV190   568  C~4451      
2015 06  12.43530  15 28 47.918  +01 32 27.43        15KV190   568  C~4451      

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    -0.12       0.00    -0.05
     2   0.0002     -4.46    -0.02      -0.03     0.18
     3   0.0005     -9.00     0.14      -0.59    -0.13
     4   0.0657  -1210.26    -0.08    -163.98    -0.06
     5   0.0687  -1260.03     0.07    -175.86     0.06

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.

15KV190    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