Orbit Fit and Astrometric record for 19PT99

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: 19PT99    
# Created Wed May 21 01:11:19 2025
# Orbit generated from Bernstein formalism
# Fitting      8 observations of      8
# Arc:  23.97h
# First observation: 2019/08/06
#  Last observation: 2019/08/07
# WARNING Fitting with energy constraint
# WARNING and with gdot fixed = 0
# Chi-squared of fit:     0.84 DOF:     12 RMS:  0.06
# Min/Max residuals:    -0.09    0.10
# Exact a, adot, b, bdot, g, gdot:
  1.444770E-05  2.121723E-02 -4.331084E-06 -6.058825E-03  2.309727E-02  0.000000E+00
# Covariance matrix:
  3.3137E-11  4.7755E-08 -1.9282E-12 -2.7647E-09  8.2112E-09  0.0000E+00
  4.7755E-08  6.9611E-05 -2.8025E-09 -4.0180E-06  1.1934E-05  0.0000E+00
 -1.9282E-12 -2.8025E-09  3.4375E-13  9.1970E-11 -4.8116E-10  0.0000E+00
 -2.7647E-09 -4.0180E-06  9.1970E-11  3.3639E-07 -6.8987E-07  0.0000E+00
  8.2112E-09  1.1934E-05 -4.8116E-10 -6.8987E-07  2.0490E-06  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  1.6215E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
   -9.496223  -65.372553   -0.321348   -0.157493   -0.941439  2458701.537291
# Heliocentric elements and errors
Epoch:              2458700.5000  =  2019/08/05
Mean Anomaly:           13.69404 +/-   357.142
Argument of Peri:      196.44134 +/-    66.092
Long of Asc Node:       85.37017 +/-     7.804
Inclination:            18.28297 +/-     4.115
Eccentricity:         0.02960629 +/-    0.5699
Semi-Major Axis:     45.55389820 +/-   23.9330
Time of Perihelion: 2454428.6503 +/-  335997.0
Perihelion:          44.20521645 +/-   34.8328
Aphelion:            46.90257995 +/-   35.7932
Period (y)              307.4656 +/-    242.30
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           18.48754651 +/-    1.1026
Ecliptic Y          -39.55865763 +/-    2.4058
Ecliptic Z           -7.14310706 +/-    0.4427
Ecliptic XDOT         0.00224529 +/-    0.0010
Ecliptic YDOT         0.00115609 +/-    0.0014
Ecliptic ZDOT        -0.00070857 +/-    0.0003
# Distances at JD0 (AU)
Heliocenter to KBO   44.24591222 +/-    2.2008
Geocenter to KBO     43.29515356 +/-    2.6832
# Hcoef:  6.83

The following table shows the complete astrometric record for 19PT99. 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 (19PT99) followed by the observatory code and reference code for the source of the astrometry.

2019 08  06.03649  19 54 00.07   -30 31 52.31        19PT99    W84  C~8r9E      
2019 08  06.04376  19 54 00.04   -30 31 52.41  23.2r 19PT99    W84  C~8r9E      
2019 08  06.05105  19 53 59.99   -30 31 52.50        19PT99    W84  C~8r9E      
2019 08  06.05832  19 53 59.96   -30 31 52.70        19PT99    W84  C~8r9E      
2019 08  06.99897  19 53 55.37   -30 32 03.33        19PT99    W84  C~8r9E      
2019 08  07.00623  19 53 55.33   -30 32 03.25        19PT99    W84  C~8r9E      
2019 08  07.02813  19 53 55.22   -30 32 03.65        19PT99    W84  C~8r9E      
2019 08  07.03541  19 53 55.18   -30 32 03.68        19PT99    W84  C~8r9E      

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     0.04
     2   0.0000     -0.40     0.09      -0.02     0.01
     3   0.0000     -1.05    -0.08       0.01     0.04
     4   0.0001     -1.47    -0.03      -0.11    -0.09
     5   0.0026    -61.71     0.05       0.87    -0.08
     6   0.0027    -62.20     0.03       1.04     0.10
     7   0.0027    -63.67    -0.02       0.93    -0.04
     8   0.0027    -64.19    -0.06       1.00     0.02

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.

19PT99    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