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 Fri Nov 22 02:11:17 2024
# Orbit generated from Bernstein formalism
# Fitting     24 observations of     24
# Arc:  35.61d
# First observation: 2023/11/11
#  Last observation: 2023/12/16
Preliminary a, adot, b, bdot, g, gdot:
  -0.000011   0.182867  -0.000023   0.035262   0.079216   0.000000
# Chi-squared of fit:    46.31 DOF:     42 RMS:  0.25
# Min/Max residuals:    -0.66    0.76
# Exact a, adot, b, bdot, g, gdot:
  2.937709E-05  1.341121E-01  8.590092E-06  3.355318E-02  7.162245E-02 -1.371561E-02
# Covariance matrix:
  2.9960E-13 -1.4014E-11 -4.4040E-15  5.4663E-13 -1.5439E-13  3.6897E-10
 -1.4014E-11  3.5234E-07 -1.7306E-10  1.1241E-08  5.3089E-08 -1.2293E-06
 -4.4040E-15 -1.7306E-10  2.5130E-13 -8.2690E-12 -2.6197E-11  5.7935E-10
  5.4663E-13  1.1241E-08 -8.2690E-12  4.3386E-10  1.7046E-09 -3.6989E-08
 -1.5439E-13  5.3089E-08 -2.6197E-11  1.7046E-09  8.0187E-09 -1.8143E-07
  3.6897E-10 -1.2293E-06  5.7935E-10 -3.6989E-08 -1.8143E-07  5.1015E-06
#      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:          353.04184 +/-     0.873
Argument of Peri:       47.85441 +/-     2.688
Long of Asc Node:       22.54200 +/-     0.102
Inclination:            15.82258 +/-     0.052
Eccentricity:         0.43806196 +/-    0.0136
Semi-Major Axis:     26.13240675 +/-    0.4728
Time of Perihelion: 2461193.6043 +/-     115.5
Perihelion:          14.68479345 +/-    0.4430
Aphelion:            37.58002005 +/-    0.7668
Period (y)              133.5910 +/-      3.63
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X            9.50499737 +/-    0.0111
Ecliptic Y           11.36536524 +/-    0.0133
Ecliptic Z            1.94217677 +/-    0.0024
Ecliptic XDOT        -0.00439057 +/-    0.0001
Ecliptic YDOT         0.00275169 +/-    0.0001
Ecliptic ZDOT         0.00119725 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   14.94284286 +/-    0.0123
Geocenter to KBO     13.96210360 +/-    0.0175
# Hcoef: 10.36

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      

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     0.05       0.00    -0.24
     2   0.0000     -1.18    -0.00       0.50     0.13
     3   0.0000     -2.39    -0.09       0.37    -0.12
     4   0.0001     -3.13     0.29       0.43    -0.18
     5   0.0192  -1264.20     0.20     122.35    -0.13
     6   0.0192  -1266.73     0.05     122.49    -0.21
     7   0.0192  -1269.10     0.08     122.85    -0.07
     8   0.0242  -1597.36    -0.00     149.84     0.19
     9   0.0243  -1602.86    -0.18     149.92    -0.20
    10   0.0244  -1608.26    -0.66     150.27    -0.26
    11   0.0269  -1772.69    -0.10     163.18    -0.03
    12   0.0270  -1776.11     0.27     163.57     0.05
    13   0.0324  -2127.81     0.03     189.41     0.35
    14   0.0325  -2130.05    -0.28     189.97     0.76
    15   0.0325  -2131.91    -0.22     189.90     0.55
    16   0.0601  -3850.89    -0.08     282.16     0.25
    17   0.0602  -3858.20     0.12     282.39     0.19
    18   0.0603  -3864.78     0.02     282.19    -0.24
    19   0.0623  -3980.74     0.15     286.13    -0.25
    20   0.0624  -3982.67     0.42     286.30    -0.18
    21   0.0624  -3985.08     0.22     286.30    -0.28
    22   0.0973  -5872.17    -0.02     311.75     0.23
    23   0.0974  -5875.86    -0.13     311.32    -0.19
    24   0.0975  -5879.40    -0.13     311.36    -0.11

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:1

Type:       CENTAURR  CENTAURR  CENTAURR

axisobj        25.898    30.647    22.906
ecceobj         0.433     0.486     0.424
incobj         15.829    16.133    15.493
qmin           14.634    15.642    13.150
qmax           38.373    46.110    32.638
amean          26.157    30.377    22.785
amin           25.769    29.792    22.343
amax           26.628    30.971    22.937
emean           0.432     0.475     0.417
emin            0.419     0.462     0.405
emax            0.442     0.489     0.424
imean          16.060    16.894    15.630
imin           15.715    16.058    15.420
imax           16.621    17.888    15.908
excite_mean     0.513     0.557     0.496
fracstop        0.009     0.007     0.002
cjmean          2.762     2.677     2.839

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        74.0      41.5      76.9
kozaiamp         25.5      11.5       9.8