Orbit Fit and Astrometric record for 20VR40

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: 20VR40    
# Created Sun Oct 19 01:12:11 2025
# Orbit generated from Bernstein formalism
# Fitting     21 observations of     21
# Arc:   2.21y
# First observation: 2020/08/15
#  Last observation: 2022/10/31
Preliminary a, adot, b, bdot, g, gdot:
  -0.000217   0.032252  -0.000053  -0.014825   0.030453   0.000000
# Chi-squared of fit:     1.71 DOF:     36 RMS:  0.05
# Min/Max residuals:    -0.10    0.18
# Exact a, adot, b, bdot, g, gdot:
  1.634470E-05  3.138818E-02 -7.688885E-06 -1.442917E-02  2.994371E-02 -5.344536E-03
# Covariance matrix:
  3.3527E-13 -1.8276E-13  4.0914E-14  1.5425E-14  1.9572E-13 -5.6758E-13
 -1.8276E-13  1.7101E-12  2.9092E-13 -1.0078E-12  5.0813E-13  2.7275E-11
  4.0914E-14  2.9092E-13  1.8894E-13 -2.8743E-13  1.5769E-13  5.3817E-12
  1.5425E-14 -1.0078E-12 -2.8743E-13  8.0628E-13 -3.7728E-13 -1.7822E-11
  1.9572E-13  5.0813E-13  1.5769E-13 -3.7728E-13  4.0903E-13  1.0049E-11
 -5.6758E-13  2.7275E-11  5.3817E-12 -1.7822E-11  1.0049E-11  4.8154E-10
#      lat0       lon0       xBary       yBary       zBary        JD0
  -17.239105   51.628242    1.003908   -0.007291   -0.023124  2459077.068335
# Heliocentric elements and errors
Epoch:              2459070.5000  =  2020/08/09
Mean Anomaly:          320.62437 +/-     0.046
Argument of Peri:      276.36006 +/-     0.105
Long of Asc Node:      197.79245 +/-     0.001
Inclination:            30.30816 +/-     0.001
Eccentricity:         0.23145646 +/-    0.0006
Semi-Major Axis:     39.35858249 +/-    0.0094
Time of Perihelion: 2468935.1702 +/-      10.9
Perihelion:          30.24878412 +/-    0.0238
Aphelion:            48.46838086 +/-    0.0254
Period (y)              246.9263 +/-      0.09
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           20.60692514 +/-    0.0004
Ecliptic Y           24.39562119 +/-    0.0005
Ecliptic Z           -9.89744751 +/-    0.0002
Ecliptic XDOT        -0.00277475 +/-    0.0000
Ecliptic YDOT         0.00111361 +/-    0.0000
Ecliptic ZDOT        -0.00111544 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   33.43278577 +/-    0.0005
Geocenter to KBO     33.39599989 +/-    0.0007
# Hcoef:  8.39

The following table shows the complete astrometric record for 20VR40. 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 (20VR40) followed by the observatory code and reference code for the source of the astrometry.

2020 08  15.567534 03 34 29.889  +01 29 11.60  23.9w 20VR40    T14  C~93U2      
2020 08  16.583841 03 34 31.420  +01 28 36.35  24.0w 20VR40    T14  C~93U2      
2020 10  18.572835 03 32 26.681  +00 44 00.68  23.8w 20VR40    T14  C~93U2      
2020 10  18.614348 03 32 26.468  +00 43 58.87  23.8w 20VR40    T14  C~93U2      
2020 10  19.468564 03 32 22.291  +00 43 23.04  23.8w 20VR40    T14  C~93U2      
2020 11  08.295522 03 30 34.930  +00 30 47.09  23.8w 20VR40    T14  C~93U2      
2020 11  09.406307 03 30 28.510  +00 30 09.97  23.7w 20VR40    T14  C~93U2      
2020 11  09.433038 03 30 28.360  +00 30 09.09  23.8w 20VR40    T14  C~93U2      
2020 11  09.458647 03 30 28.211  +00 30 08.21  24.2w 20VR40    T14  C~93U2      
2020 11  10.320844 03 30 23.230  +00 29 40.00  23.8w 20VR40    T14  C~93U2      
2020 11  10.346353 03 30 23.082  +00 29 39.15  23.7w 20VR40    T14  C~93U2      
2020 12  23.319418 03 26 30.727  +00 16 31.58  23.8w 20VR40    T14  C~93U2      
2020 12  23.344742 03 26 30.613  +00 16 31.57  23.9w 20VR40    T14  C~93U2      
2020 12  23.370057 03 26 30.503  +00 16 31.46  23.8w 20VR40    T14  C~93U2      
2021 01  17.294849 03 25 11.136  +00 19 18.39  24.0w 20VR40    T14  C~93U2      
2021 01  17.359532 03 25 11.024  +00 19 19.57  23.8w 20VR40    T14  C~93U2      
2021 10  11.557917 03 41 01.311  +00 27 00.66  23.9w 20VR40    T14  C~93U2      
2021 10  11.592759 03 41 01.159  +00 26 59.14  23.9w 20VR40    T14  C~93U2      
2022 08  21.592212 03 50 24.769  +00 42 33.20  24.1w 20VR40    T14  C~93U3      
2022 08  25.537790 03 50 29.479  +00 39 57.67  23.9w 20VR40    T14  C~93U3      
2022 10  31.469076 03 47 33.341  -00 09 17.10  23.7w 20VR40    T14  C~93U3      

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     0.01
     2   0.0028     13.54     0.02     -39.83     0.04
     3   0.1752  -2460.54     0.01   -2170.45    -0.00
     4   0.1754  -2464.08    -0.10   -2171.42    -0.04
     5   0.1777  -2533.66    -0.02   -2190.66    -0.01
     6   0.2320  -4281.52    -0.01   -2525.26     0.07
     7   0.2350  -4384.06    -0.07   -2537.43     0.00
     8   0.2351  -4386.46     0.04   -2537.72    -0.02
     9   0.2352  -4388.85     0.05   -2538.02    -0.06
    10   0.2375  -4468.26     0.00   -2546.90     0.02
    11   0.2376  -4470.62     0.02   -2547.17    -0.01
    12   0.3552  -8045.98    -0.03   -2448.52    -0.06
    13   0.3553  -8047.65    -0.04   -2448.10     0.00
    14   0.3554  -8049.27    -0.02   -2447.80    -0.05
    15   0.4236  -9163.27    -0.10   -1991.13    -0.02
    16   0.4238  -9164.61     0.18   -1989.57     0.09
    17   1.1553   4770.18    -0.01   -5065.94     0.01
    18   1.1554   4767.59    -0.01   -5066.85     0.04
    19   2.0151  13212.18     0.03   -6249.57     0.04
    20   2.0259  13242.75    -0.06   -6418.22    -0.03
    21   2.2092   9944.49     0.04   -8635.16    -0.03

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.

20VR40    quality flag:3

Type:           3:2E      3:2E      3:2E
Type:          6:4II     6:4II     6:4II

axisobj        39.775    39.785    39.765
ecceobj         0.236     0.236     0.236
incobj         30.221    30.221    30.221
qmin           27.273    27.347    27.260
qmax           52.261    51.823    51.994
amean          39.454    39.454    39.452
amin           39.029    39.025    39.040
amax           39.961    39.972    39.957
emean           0.268     0.267     0.268
emin            0.225     0.225     0.226
emax            0.308     0.305     0.307
imean          29.507    29.520    29.495
imin           28.525    28.550    28.494
imax           30.479    30.480    30.475
excite_mean     0.561     0.561     0.561
fracstop        1.000     1.000     1.000
cjmean          2.683     2.683     2.683

libcent 0       180.2     180.0     180.3
libamp  0        68.6      72.7      64.8
libcent 1       180.8     179.2     180.3
libamp  1       155.2     161.3     148.0
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       268.7     268.6     268.7
kozaiamp         19.4      19.4      19.4