Orbit Fit and Astrometric record for 19CS30

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: 19CS30    
# Created Tue Apr  1 01:11:11 2025
# Orbit generated from Bernstein formalism
# Fitting     11 observations of     11
# Arc:  57.94d
# First observation: 2019/02/05
#  Last observation: 2019/04/04
Preliminary a, adot, b, bdot, g, gdot:
   0.000000   0.024271  -0.000001   0.000455   0.023963   0.000000
# Chi-squared of fit:     5.84 DOF:     16 RMS:  0.13
# Min/Max residuals:    -0.27    0.34
# Exact a, adot, b, bdot, g, gdot:
  1.552907E-05  2.310285E-02  2.834508E-07  4.757290E-04  2.362834E-02  1.499231E-03
# Covariance matrix:
  4.4057E-13  1.1755E-10 -7.3531E-14 -2.5733E-12  2.5275E-11  1.4987E-09
  1.1755E-10  1.9028E-07 -1.1132E-10 -4.1725E-09  3.8593E-08  1.8862E-06
 -7.3531E-14 -1.1132E-10  3.6860E-13  2.1476E-13 -2.2636E-11 -1.1210E-09
 -2.5733E-12 -4.1725E-09  2.1476E-13  1.2051E-10 -8.4558E-10 -4.1100E-08
  2.5275E-11  3.8593E-08 -2.2636E-11 -8.4558E-10  7.8444E-09  3.8756E-07
  1.4987E-09  1.8862E-06 -1.1210E-09 -4.1100E-08  3.8756E-07  2.0266E-05
#      lat0       lon0       xBary       yBary       zBary        JD0
    4.323451 -177.732903    0.717770    0.051678   -0.682694  2458520.055801
# Heliocentric elements and errors
Epoch:              2458520.5000  =  2019/02/06
Mean Anomaly:           40.95580 +/-    82.960
Argument of Peri:       27.32397 +/-   101.768
Long of Asc Node:      107.84331 +/-     0.487
Inclination:             4.43673 +/-     0.011
Eccentricity:         0.06560210 +/-    0.1699
Semi-Major Axis:     45.15720297 +/-    2.3083
Time of Perihelion: 2445910.8829 +/-   25523.6
Perihelion:          42.19479570 +/-    7.9686
Aphelion:            48.11961023 +/-    8.0559
Period (y)              303.4581 +/-     23.27
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -42.88003781 +/-    0.1581
Ecliptic Y           -0.98743572 +/-    0.0062
Ecliptic Z            3.19052509 +/-    0.0120
Ecliptic XDOT        -0.00005500 +/-    0.0005
Ecliptic YDOT        -0.00268321 +/-    0.0001
Ecliptic ZDOT         0.00006786 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   43.00990726 +/-    0.1576
Geocenter to KBO     42.32206521 +/-    0.1586
# Hcoef:  8.50

The following table shows the complete astrometric record for 19CS30. 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 (19CS30) followed by the observatory code and reference code for the source of the astrometry.

2019 02  05.55500  12 15 11.98   +03 03 55.4   24.5i 19CS30    T09  C~83G8      
2019 02  05.55837  12 15 11.99   +03 03 55.4   24.5i 19CS30    T09  C~83G8      
2019 02  05.60072  12 15 11.85   +03 03 56.4   24.7i 19CS30    T09  C~83G8      
2019 02  05.62764  12 15 11.77   +03 03 57.1   24.1i 19CS30    T09  C~83G8      
2019 03  03.52028  12 13 43.53   +03 15 17.5   24.8z 19CS30    T09  C~83G8      
2019 03  03.52832  12 13 43.46   +03 15 18.0   24.2z 19CS30    T09  C~83G8      
2019 03  03.58484  12 13 43.24   +03 15 19.5   24.4z 19CS30    T09  C~83G8      
2019 04  04.44950  12 11 26.64   +03 30 33.4   25.3g 19CS30    T09  C~83G8      
2019 04  04.46994  12 11 26.56   +03 30 34.0   25.5g 19CS30    T09  C~83G8      
2019 04  04.47203  12 11 26.54   +03 30 34.2   25.8g 19CS30    T09  C~83G8      
2019 04  04.49303  12 11 26.45   +03 30 34.7   25.4g 19CS30    T09  C~83G8      

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    -0.01       0.00     0.01
     2   0.0000      0.14     0.28       0.06     0.05
     3   0.0001     -2.18    -0.07       0.14    -0.05
     4   0.0002     -3.56    -0.20       0.31    -0.01
     5   0.0711  -1486.78     0.34      98.71     0.00
     6   0.0711  -1487.94    -0.27      98.75     0.03
     7   0.0713  -1491.56    -0.07      98.82    -0.02
     8   0.1585  -3732.10     0.01     124.50    -0.10
     9   0.1586  -3733.44     0.12     124.58     0.00
    10   0.1586  -3733.80    -0.09     124.64     0.07
    11   0.1586  -3735.23    -0.04     124.57     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.

19CS30    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