Orbit Fit and Astrometric record for 17MP42

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: 17MP42    
# Created Wed Sep  3 01:11:40 2025
# Orbit generated from Bernstein formalism
# Fitting     20 observations of     20
# Arc:   1.06y
# First observation: 2016/07/29
#  Last observation: 2017/08/22
Preliminary a, adot, b, bdot, g, gdot:
  -0.000067   0.018745   0.000005   0.001389   0.022062   0.000000
# Chi-squared of fit:     5.76 DOF:     34 RMS:  0.09
# Min/Max residuals:    -0.15    0.19
# Exact a, adot, b, bdot, g, gdot:
  1.296118E-05  1.880016E-02  1.385635E-06  1.398923E-03  2.223741E-02  2.007538E-03
# Covariance matrix:
  3.6168E-13  6.5253E-13 -2.0301E-14  8.4341E-14  9.2613E-13  5.5584E-11
  6.5253E-13  9.6301E-12 -1.1218E-13  5.0082E-13  4.8783E-12  5.0737E-10
 -2.0301E-14 -1.1218E-13  1.5073E-13 -1.7414E-13 -9.5646E-14 -6.9408E-12
  8.4341E-14  5.0082E-13 -1.7414E-13  4.0266E-13  4.0489E-13  3.0504E-11
  9.2613E-13  4.8783E-12 -9.5646E-14  4.0489E-13  4.3117E-12  3.0515E-10
  5.5584E-11  5.0737E-10 -6.9408E-12  3.0504E-11  3.0515E-10  2.8612E-08
#      lat0       lon0       xBary       yBary       zBary        JD0
   15.120336  -24.994334    0.481591    0.233225   -0.862756  2457598.857009
# Heliocentric elements and errors
Epoch:              2457590.5000  =  2016/07/21
Mean Anomaly:          143.60177 +/-     2.143
Argument of Peri:      279.51274 +/-     2.092
Long of Asc Node:      261.20787 +/-     0.010
Inclination:            15.46131 +/-     0.001
Eccentricity:         0.18646632 +/-    0.0030
Semi-Major Axis:     39.51029248 +/-    0.0547
Time of Perihelion: 2421406.1248 +/-     534.8
Perihelion:          32.14295368 +/-    0.1284
Aphelion:            46.87763127 +/-    0.1368
Period (y)              248.3554 +/-      0.52
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           39.94992704 +/-    0.0037
Ecliptic Y          -19.15944985 +/-    0.0017
Ecliptic Z           11.73022649 +/-    0.0011
Ecliptic XDOT         0.00115480 +/-    0.0000
Ecliptic YDOT         0.00200905 +/-    0.0000
Ecliptic ZDOT         0.00023072 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   45.83316924 +/-    0.0033
Geocenter to KBO     44.96927256 +/-    0.0042
# Hcoef:  6.90

The following table shows the complete astrometric record for 17MP42. 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 (17MP42) followed by the observatory code and reference code for the source of the astrometry.

2016 07  29.35622  22 05 24.49   +04 25 12.4   23.4z 17MP42    T09  C~91XO      
2016 07  29.37997  22 05 24.40   +04 25 12.3   23.6z 17MP42    T09  C~91XO      
2016 07  29.38267  22 05 24.37   +04 25 12.1   23.5z 17MP42    T09  C~91XO      
2016 07  29.39345  22 05 24.33   +04 25 11.9   23.8z 17MP42    T09  C~91XO      
2016 08  28.28007  22 03 20.29   +04 16 09.1   23.3i 17MP42    T09  C~91XO      
2016 08  28.28962  22 03 20.24   +04 16 08.7   23.3i 17MP42    T09  C~91XO      
2016 08  28.29774  22 03 20.20   +04 16 08.6   23.2i 17MP42    T09  C~91XO      
2016 08  28.30585  22 03 20.18   +04 16 08.4   23.2i 17MP42    T09  C~91XO      
2016 08  28.30855  22 03 20.17   +04 16 08.4   23.2i 17MP42    T09  C~91XO      
2016 08  28.31395  22 03 20.14   +04 16 08.1   23.4i 17MP42    T09  C~91XO      
2016 08  28.32210  22 03 20.09   +04 16 08.1   23.6i 17MP42    T09  C~91XO      
2017 06  24.46265  22 11 02.86   +04 53 35.1   23.3i 17MP42    T09  C~91XO      
2017 06  24.48472  22 11 02.82   +04 53 35.4   23.5i 17MP42    T09  C~91XO      
2017 06  24.49006  22 11 02.82   +04 53 35.4   23.3i 17MP42    T09  C~91XO      
2017 06  24.49541  22 11 02.80   +04 53 35.4   23.2i 17MP42    T09  C~91XO      
2017 07  19.42071  22 09 55.38   +04 54 16.3   22.9y 17MP42    T09  C~91XO      
2017 07  19.43617  22 09 55.31   +04 54 16.3   22.8y 17MP42    T09  C~91XO      
2017 07  19.44685  22 09 55.28   +04 54 16.3   22.5y 17MP42    T09  C~91XO      
2017 07  21.214243 22 09 49.210  +04 54 05.90  24.3g 17MP42    W84  C~91XO      
2017 08  22.136788 22 07 42.139  +04 46 23.52  23.8g 17MP42    W84  C~91XO      

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     0.08       0.00    -0.08
     2   0.0001     -1.29     0.19       0.39     0.06
     3   0.0001     -1.78    -0.15       0.37     0.01
     4   0.0001     -2.41    -0.14       0.40    -0.08
     5   0.0819  -1928.40     0.12     165.86     0.05
     6   0.0820  -1929.24    -0.07     165.76    -0.06
     7   0.0820  -1929.84    -0.11     165.88     0.05
     8   0.0820  -1930.19     0.10     165.80    -0.03
     9   0.0820  -1930.33     0.14     165.86     0.02
    10   0.0820  -1930.86    -0.01     165.74    -0.10
    11   0.0820  -1931.55    -0.15     166.01     0.16
    12   0.9038   5333.59    -0.08    -236.59    -0.00
    13   0.9038   5333.14     0.00    -236.10     0.08
    14   0.9039   5333.14     0.13    -236.10    -0.02
    15   0.9039   5332.86    -0.02    -235.99    -0.02
    16   0.9721   4406.99     0.06     164.94    -0.05
    17   0.9722   4406.01    -0.14     165.32     0.12
    18   0.9722   4405.59    -0.03     165.48     0.13
    19   0.9770   4317.18     0.11     188.45    -0.08
    20   1.0644   2378.40    -0.02     441.86    -0.14

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.

17MP42    quality flag:2

Type:       SCATNEAR  SCATNEAR      3:2E

axisobj        39.673    39.846    39.534
ecceobj         0.179     0.187     0.174
incobj         15.488    15.490    15.486
qmin           31.580    30.630    30.340
qmax           48.169    49.360    48.925
amean          39.457    39.415    39.456
amin           38.849    38.796    39.046
amax           40.086    40.208    39.936
emean           0.171     0.165     0.199
emin            0.120     0.102     0.162
emax            0.203     0.229     0.228
imean          17.538    21.124    16.087
imin           16.678    16.906    15.232
imax           19.463    23.173    17.068
excite_mean     0.347     0.397     0.341
fracstop        1.000     1.000     1.000
cjmean          2.913     2.868     2.918

libcent 0      -180.0    -180.0     179.4
libamp  0      -180.0    -180.0      77.7
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     183.9     181.2
kozaiamp        180.0     179.8     180.0