Orbit Fit and Astrometric record for 19EV5

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: 19EV5     
# Created Sat Apr 27 01:18:24 2024
# Orbit generated from Bernstein formalism
# Fitting      8 observations of      8
# Arc:   2.01y
# First observation: 2019/03/05
#  Last observation: 2021/03/09
Preliminary a, adot, b, bdot, g, gdot:
  -0.000051   0.010280  -0.000001   0.000587   0.015527   0.000000
# Chi-squared of fit:     3.48 DOF:     10 RMS:  0.12
# Min/Max residuals:    -0.21    0.20
# Exact a, adot, b, bdot, g, gdot:
  1.133241E-05  1.035413E-02  6.516527E-07  5.918718E-04  1.574250E-02  4.634280E-03
# Covariance matrix:
  4.0415E-13 -3.1643E-12  5.8383E-14 -1.7435E-13 -3.9663E-13 -1.5004E-10
 -3.1643E-12  1.2610E-10 -2.4634E-12  7.4195E-12  1.7642E-11  6.3852E-09
  5.8383E-14 -2.4634E-12  3.8293E-13 -3.5090E-13 -3.2461E-13 -1.2490E-10
 -1.7435E-13  7.4195E-12 -3.5090E-13  7.2321E-13  1.0461E-12  3.7659E-10
 -3.9663E-13  1.7642E-11 -3.2461E-13  1.0461E-12  3.3083E-12  9.0027E-10
 -1.5004E-10  6.3852E-09 -1.2490E-10  3.7659E-10  9.0027E-10  3.2409E-07
#      lat0       lon0       xBary       yBary       zBary        JD0
    8.317357  169.156459    0.092386    0.143374   -0.980372  2458547.869951
# Heliocentric elements and errors
Epoch:              2458540.5000  =  2019/02/26
Mean Anomaly:           88.06404 +/-     7.438
Argument of Peri:      294.95017 +/-     3.683
Long of Asc Node:      101.52724 +/-     0.044
Inclination:             8.85158 +/-     0.003
Eccentricity:         0.42660204 +/-    0.0278
Semi-Major Axis:     55.97621242 +/-    1.7294
Time of Perihelion: 2421120.8434 +/-    2642.3
Perihelion:          32.09664616 +/-    1.8441
Aphelion:            79.85577868 +/-    2.9162
Period (y)              418.8066 +/-     19.41
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -62.68647582 +/-    0.0071
Ecliptic Y           12.09350261 +/-    0.0014
Ecliptic Z            9.18891520 +/-    0.0011
Ecliptic XDOT        -0.00109922 +/-    0.0001
Ecliptic YDOT        -0.00162272 +/-    0.0000
Ecliptic ZDOT         0.00021823 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   64.50025751 +/-    0.0069
Geocenter to KBO     63.52229739 +/-    0.0073
# Hcoef:  7.49

The following table shows the complete astrometric record for 19EV5. 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 (19EV5) followed by the observatory code and reference code for the source of the astrometry.

2019 03  05.36915  11 33 24.764  +11 55 58.24  25.4r 19EV5     568  C~5JzK      
2019 03  05.54179  11 33 24.232  +11 56 01.80  25.3r 19EV5     568  C~5JzK      
2019 04  04.41962  11 31 52.274  +12 05 17.58        19EV5     568  C~5JzK      
2019 04  04.51092  11 31 51.997  +12 05 18.93        19EV5     568  C~5JzK      
2019 12  27.32353  11 37 56.680  +11 22 33.25  25.5r 19EV5     304  C~5JzK      
2019 12  28.33144  11 37 56.312  +11 22 44.13  25.6r 19EV5     304  C~5JzK      
2021 03  09.17502  11 37 41.624  +11 32 57.01  25.6G 19EV5     304  C~5JzK      
2021 03  09.23217  11 37 41.455  +11 32 58.52  25.4G 19EV5     304  C~5JzK      

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    -0.19       0.00    -0.01
     2   0.0005     -8.58     0.02       0.15    -0.01
     3   0.0823  -1467.50     0.12     -28.01     0.08
     4   0.0825  -1471.76     0.01     -28.39     0.00
     5   0.8130   4464.13     0.16    -234.19     0.11
     6   0.8158   4454.79    -0.09    -226.41    -0.21
     7   2.0118   4010.07    -0.02     247.64    -0.17
     8   2.0119   4007.18    -0.01     248.02     0.20

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.

19EV5    quality flag:1

Type:       CENTAURR     3:1EE   REMOVED

axisobj        56.083    62.553    52.190
ecceobj         0.433     0.515     0.365
incobj          8.832     8.841     8.824
qmin           30.108    29.757    30.378
qmax           97.610    97.501    81.621
amean          57.530    62.630    51.023
amin           48.873    61.718    36.761
amax           64.678    63.926    56.727
emean           0.443     0.513     0.365
emin            0.372     0.502     0.164
emax            0.512     0.526     0.439
imean           6.726     6.862     5.344
imin            1.649     6.317     2.548
imax            9.859     7.385     8.276
excite_mean     0.460     0.527     0.378
fracstop        0.900     1.000     0.494
cjmean          2.981     2.939     3.000

libcent 0      -180.0     284.3    -180.0
libamp  0      -180.0      38.6    -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       178.1     171.4     185.2
kozaiamp        180.0     180.0     180.0