Orbit Fit and Astrometric record for 14YD100

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: 14YD100   
# Created Wed May  8 01:16:49 2024
# Orbit generated from Bernstein formalism
# Fitting     20 observations of     20
# Arc:   2.93y
# First observation: 2014/11/24
#  Last observation: 2017/10/30
Preliminary a, adot, b, bdot, g, gdot:
  -0.000403   0.046429   0.000086  -0.014388   0.034803   0.000000
# Chi-squared of fit:    11.30 DOF:     34 RMS:  0.13
# Min/Max residuals:    -0.24    0.29
# Exact a, adot, b, bdot, g, gdot:
  2.019141E-05  4.523372E-02 -6.004080E-06 -1.417632E-02  3.600460E-02 -5.426005E-03
# Covariance matrix:
  3.9682E-13  1.8022E-12 -4.0209E-14 -5.5488E-13  1.0744E-12  1.3907E-11
  1.8022E-12  4.0035E-11 -2.0185E-13 -1.1063E-11  1.3746E-11  2.7725E-10
 -4.0209E-14 -2.0185E-13  1.6402E-13  8.1340E-15 -1.5680E-13 -1.6052E-12
 -5.5488E-13 -1.1063E-11  8.1340E-15  3.1083E-12 -3.9183E-12 -7.6962E-11
  1.0744E-12  1.3746E-11 -1.5680E-13 -3.9183E-12  5.9601E-12  9.8197E-11
  1.3907E-11  2.7725E-10 -1.6052E-12 -7.6962E-11  9.8197E-11  1.9287E-09
#      lat0       lon0       xBary       yBary       zBary        JD0
  -19.516501   51.392805   -0.175134   -0.324609   -0.916310  2456985.856878
# Heliocentric elements and errors
Epoch:              2456980.5000  =  2014/11/19
Mean Anomaly:          344.84407 +/-     0.103
Argument of Peri:      257.83600 +/-     0.209
Long of Asc Node:      185.56034 +/-     0.001
Inclination:            25.33482 +/-     0.000
Eccentricity:         0.29783946 +/-    0.0005
Semi-Major Axis:     39.70706651 +/-    0.0136
Time of Perihelion: 2460828.0151 +/-      26.1
Perihelion:          27.88073526 +/-    0.0214
Aphelion:            51.53339776 +/-    0.0260
Period (y)              250.2130 +/-      0.13
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           16.80134139 +/-    0.0011
Ecliptic Y           21.32724210 +/-    0.0014
Ecliptic Z           -9.27895376 +/-    0.0006
Ecliptic XDOT        -0.00315949 +/-    0.0000
Ecliptic YDOT         0.00155593 +/-    0.0000
Ecliptic ZDOT        -0.00087811 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   28.69207750 +/-    0.0012
Geocenter to KBO     27.77423201 +/-    0.0019
# Hcoef:  7.71

The following table shows the complete astrometric record for 14YD100. 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 (14YD100) followed by the observatory code and reference code for the source of the astrometry.

2014 11  24.3561   03 35 53.27   -00 46 30.9   22.7w 14YD100   F51  C~77rr      
2014 11  24.37113  03 35 53.16   -00 46 31.3   22.7w 14YD100   F51  C~77rr      
2014 11  24.38627  03 35 53.08   -00 46 31.5   22.4w 14YD100   F51  C~77rr      
2014 12  18.35636  03 33 26.54   -00 52 18.2   22.6w 14YD100   F51  C~77rr      
2014 12  18.36926  03 33 26.49   -00 52 18.1   22.5w 14YD100   F51  C~77rr      
2014 12  18.38216  03 33 26.40   -00 52 18.4   22.5w 14YD100   F51  C~77rr      
2014 12  18.39513  03 33 26.35   -00 52 18.1   22.7w 14YD100   F51  C~77rr      
2015 01  19.2779   03 31 23.97   -00 46 35.3   22.6w 14YD100   F51  C~77rr      
2015 01  19.29057  03 31 23.95   -00 46 34.9   22.8w 14YD100   F51  C~77rr      
2015 01  19.30309  03 31 23.93   -00 46 34.6   22.4w 14YD100   F51  C~77rr      
2017 09  19.59747  04 14 05.39   -00 24 26.9   22.7w 14YD100   F51  C~77rr      
2017 09  19.61449  04 14 05.36   -00 24 27.9   22.7w 14YD100   F51  C~77rr      
2017 09  19.623    04 14 05.36   -00 24 28.0   22.2w 14YD100   F51  C~77rr      
2017 10  01.60449  04 13 40.02   -00 34 59.0   22.4w 14YD100   F51  C~77rr      
2017 10  01.6117   04 13 40.01   -00 34 59.5   22.4w 14YD100   F51  C~77rr      
2017 10  01.61895  04 13 39.98   -00 34 59.6   22.4w 14YD100   F51  C~77rr      
2017 10  01.62616  04 13 39.94   -00 35 00.1   22.4w 14YD100   F51  C~77rr      
2017 10  30.51344  04 11 31.26   -00 58 32.5   22.6w 14YD100   F51  C~77rr      
2017 10  30.53866  04 11 31.13   -00 58 33.7   22.4w 14YD100   F51  C~77rr      
2017 10  30.55128  04 11 31.06   -00 58 34.4   22.5w 14YD100   F51  C~77rr      

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    -0.07       0.00    -0.05
     2   0.0000     -1.70    -0.21       0.02    -0.03
     3   0.0001     -2.91     0.14       0.13     0.06
     4   0.0657  -2218.16    -0.13     209.69     0.01
     5   0.0657  -2218.86     0.22     209.97     0.07
     6   0.0658  -2220.24    -0.11     210.02    -0.10
     7   0.0658  -2220.89     0.29     210.49     0.15
     8   0.1531  -3914.44    -0.15     997.97    -0.07
     9   0.1531  -3914.63    -0.03     998.43    -0.00
    10   0.1532  -3914.85     0.05     998.79    -0.03
    11   2.8206  33940.98    -0.04   -7351.76    -0.15
    12   2.8207  33940.28    -0.15   -7352.62    -0.24
    13   2.8207  33940.26     0.12   -7352.72     0.06
    14   2.8535  33401.68     0.05   -7874.59     0.02
    15   2.8535  33401.41     0.19   -7875.05    -0.14
    16   2.8536  33400.93     0.14   -7875.03     0.17
    17   2.8536  33400.21    -0.17   -7875.36     0.12
    18   2.9327  31124.70    -0.23   -8764.79     0.23
    19   2.9327  31122.46     0.03   -8765.46     0.05
    20   2.9328  31121.24     0.05   -8765.88    -0.12

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.

14YD100    quality flag:3

Type:           3:2E      3:2E      3:2E

axisobj        39.960    39.990    39.931
ecceobj         0.300     0.300     0.300
incobj         25.257    25.258    25.257
qmin           27.047    27.111    26.891
qmax           52.481    52.611    52.602
amean          39.454    39.454    39.453
amin           38.982    38.977    39.011
amax           40.042    40.047    39.979
emean           0.262     0.251     0.261
emin            0.190     0.184     0.192
emax            0.314     0.315     0.316
imean          25.936    26.389    25.887
imin           24.395    24.529    24.142
imax           27.841    28.208    27.675
excite_mean     0.511     0.512     0.510
fracstop        1.000     1.000     1.000
cjmean          2.749     2.747     2.750

libcent 0       178.8     179.7     180.9
libamp  0        97.9     113.5      85.8
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       273.7     270.9     273.5
kozaiamp         47.7      57.5      45.5