Orbit Fit and Astrometric record for 23VQ17

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: 23VQ17    
# Created Wed Mar 26 01:11:36 2025
# Orbit generated from Bernstein formalism
# Fitting     25 observations of     26
# Arc:   1.29y
# First observation: 2023/11/11
#  Last observation: 2025/02/23
Preliminary a, adot, b, bdot, g, gdot:
  -0.000062   0.129254   0.000047   0.032070   0.070330   0.000000
# Chi-squared of fit:    37.99 DOF:     44 RMS:  0.22
# Min/Max residuals:    -0.73    0.54
# Exact a, adot, b, bdot, g, gdot:
  2.914650E-05  1.348637E-01  7.997832E-06  3.357742E-02  7.173291E-02 -1.695082E-02
# Covariance matrix:
  2.0223E-13  5.4778E-12 -4.8730E-14  1.5756E-12  1.5914E-12  4.4115E-11
  5.4778E-12  1.1052E-09 -1.0387E-11  3.1872E-10  2.3046E-10  9.4188E-09
 -4.8730E-14 -1.0387E-11  1.6679E-13 -3.0708E-12 -2.1527E-12 -8.8669E-11
  1.5756E-12  3.1872E-10 -3.0708E-12  9.2525E-11  6.6384E-11  2.7183E-09
  1.5914E-12  2.3046E-10 -2.1527E-12  6.6384E-11  4.9860E-11  1.9517E-09
  4.4115E-11  9.4188E-09 -8.8669E-11  2.7183E-09  1.9517E-09  8.0405E-08
#      lat0       lon0       xBary       yBary       zBary        JD0
    7.995629   50.218879    0.028062    0.136489   -0.972971  2460259.824353
# Heliocentric elements and errors
Epoch:              2460250.5000  =  2023/11/02
Mean Anomaly:          352.21337 +/-     0.112
Argument of Peri:       51.55449 +/-     0.353
Long of Asc Node:       22.41022 +/-     0.003
Inclination:            15.75512 +/-     0.001
Eccentricity:         0.45782668 +/-    0.0008
Semi-Major Axis:     26.83670880 +/-    0.0222
Time of Perihelion: 2461348.8464 +/-      15.7
Perihelion:          14.55014761 +/-    0.0253
Aphelion:            39.12326999 +/-    0.0393
Period (y)              139.0279 +/-      0.17
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X            9.49137787 +/-    0.0009
Ecliptic Y           11.34900164 +/-    0.0010
Ecliptic Z            1.93917781 +/-    0.0002
Ecliptic XDOT        -0.00448418 +/-    0.0000
Ecliptic YDOT         0.00267175 +/-    0.0000
Ecliptic ZDOT         0.00117915 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   14.92134386 +/-    0.0010
Geocenter to KBO     13.94060356 +/-    0.0014
# Hcoef: 10.37

The following table shows the complete astrometric record for 23VQ17. 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 (23VQ17) followed by the observatory code and reference code for the source of the astrometry.

2023 11  11.323552 03 01 39.742  +25 29 20.29  21.9G 23VQ17    V00  C~7XVT      
2023 11  11.329687 03 01 39.648  +25 29 20.44  22.3G 23VQ17    V00  C~7XVT      
2023 11  11.335796 03 01 39.565  +25 29 19.97  21.9G 23VQ17    V00  C~7XVT      
2023 11  11.341908 03 01 39.511  +25 29 19.82  21.9G 23VQ17    V00  C~7XVT      
2023 11  18.323198 03 00 07.667  +25 25 19.42  22.2w 23VQ17    F52  C~7XVT      
2023 11  18.336265 03 00 07.485  +25 25 18.84  21.8w 23VQ17    F52  C~7XVT      
2023 11  18.349318 03 00 07.310  +25 25 18.51  21.8w 23VQ17    F52  C~7XVT      
2023 11  20.18051  02 59 43.52   +25 24 10.8   22.2R 23VQ17    291  C~7XVT      
2023 11  20.20984  02 59 43.13   +25 24 09.3         23VQ17    291  C~7XVT      
2023 11  20.23694  02 59 42.74   +25 24 08.1         23VQ17    291  C~7XVT      
2023 11  21.16310  02 59 30.84   +25 23 33.5   22.0G 23VQ17    291  C~7XVT      
2023 11  21.18408  02 59 30.59   +25 23 32.9   22.0G 23VQ17    291  C~7XVT      
2023 11  23.167574 02 59 05.180  +25 22 17.00  21.9G 23VQ17    I52  C~7XVT      
2023 11  23.178332 02 59 05.010  +25 22 16.90  21.8G 23VQ17    I52  C~7XVT      
2023 11  23.189088 02 59 04.880  +25 22 16.30  21.4G 23VQ17    I52  C~7XVT      
2023 12  03.27873  02 57 01.56   +25 15 28.9   22.0R 23VQ17    291  C~7XVT      
2023 12  03.32396  02 57 01.04   +25 15 27.0   21.8R 23VQ17    291  C~7XVT      
2023 12  03.36311  02 57 00.58   +25 15 24.9   21.8R 23VQ17    291  C~7XVT      
2023 12  04.08357  02 56 52.32   +25 14 55.0   22.1G 23VQ17    291  C~7XVT      
2023 12  04.09709  02 56 52.18   +25 14 54.6   21.8G 23VQ17    291  C~7XVT      
2023 12  04.11064  02 56 52.01   +25 14 53.9   22.2G 23VQ17    291  C~7XVT      
2023 12  16.87754  02 54 38.61   +25 06 06.5   21.5G 23VQ17    A05  C~7bVp      
2023 12  16.90414  02 54 38.36   +25 06 05.0   21.6G 23VQ17    A05  C~7bVp      
2023 12  16.93052  02 54 38.11   +25 06 04.0   21.4G 23VQ17    A05  C~7bVp      
2025 02  23.10783  03 23 37.971  +28 32 38.48  22.2G 23VQ17    G37              
2025 02  23.15240  03 23 38.335  +28 32 38.49        23VQ17    G37              

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    -0.12
     2   0.0000     -1.18     0.07       0.50     0.26
     3   0.0000     -2.39    -0.02       0.37    -0.00
     4   0.0001     -3.13     0.37       0.43    -0.06
     5   0.0192  -1264.20     0.14     122.35    -0.10
     6   0.0192  -1266.73     0.00     122.49    -0.17
     7   0.0192  -1269.10     0.02     122.85    -0.03
     8   0.0242  -1597.36    -0.07     149.84     0.21
     9   0.0243  -1602.86    -0.24     149.92    -0.18
    10   0.0244  -1608.26    -0.73     150.27    -0.24
    11   0.0269  -1772.69    -0.17     163.18    -0.02
    12   0.0270  -1776.11     0.20     163.57     0.06
    13   0.0324  -2127.81    -0.04     189.41     0.34
    14   0.0325  -2130.05 (  -0.35)    189.97 (   0.76)
    15   0.0325  -2131.91    -0.29     189.90     0.54
    16   0.0601  -3850.89    -0.08     282.16     0.22
    17   0.0602  -3858.20     0.12     282.39     0.16
    18   0.0603  -3864.78     0.02     282.19    -0.27
    19   0.0623  -3980.74     0.15     286.13    -0.28
    20   0.0624  -3982.67     0.42     286.30    -0.21
    21   0.0624  -3985.08     0.22     286.30    -0.31
    22   0.0973  -5872.17    -0.00     311.75     0.32
    23   0.0974  -5875.86    -0.11     311.32    -0.09
    24   0.0975  -5879.40    -0.11     311.36    -0.02
    25   1.2862  19941.20    -0.02    6030.74     0.09
    26   1.2863  19945.90     0.02    6029.60    -0.08

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.

23VQ17    quality flag:3

Type:       CENTAURR  CENTAURR  CENTAURR

axisobj        26.596    27.225    26.005
ecceobj         0.453     0.459     0.449
incobj         15.758    15.767    15.748
qmin           14.544    14.515    14.212
qmax           38.985    39.866    38.249
amean          26.600    27.027    25.993
amin           26.358    26.728    25.625
amax           26.864    27.427    26.265
emean           0.444     0.452     0.446
emin            0.436     0.444     0.435
emax            0.454     0.459     0.457
imean          15.950    15.982    15.907
imin           15.662    15.554    15.522
imax           16.379    16.538    16.585
excite_mean     0.522     0.529     0.523
fracstop        0.003     0.005     0.005
cjmean          2.746     2.733     2.753

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        62.1      64.2      62.5
kozaiamp          9.8      14.5      11.0