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: 03YS179
# Created Tue Apr 1 01:08:33 2025
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 38 observations of 38
# Arc: 18.19y
# First observation: 2003/12/24
# Last observation: 2022/03/02
# Chi-squared of fit: 30.35 DOF: 70 RMS: 0.16
# Min/Max residuals: -0.55 0.32
# Exact a, adot, b, bdot, g, gdot:
1.602668E-05 2.203698E-02 7.813649E-07 1.303808E-03 2.331189E-02 -3.662903E-04
# Covariance matrix:
1.5797E-13 -3.4083E-14 2.9461E-15 -1.6688E-15 2.9476E-14 -6.5392E-14
-3.4083E-14 1.9159E-14 -1.7378E-15 1.1167E-15 5.8006E-15 4.4079E-14
2.9461E-15 -1.7378E-15 1.0336E-13 -6.7226E-15 4.5343E-16 -4.1382E-15
-1.6688E-15 1.1167E-15 -6.7226E-15 7.1797E-16 3.1799E-16 2.6594E-15
2.9476E-14 5.8006E-15 4.5343E-16 3.1799E-16 1.0527E-13 1.3862E-14
-6.5392E-14 4.4079E-14 -4.1382E-15 2.6594E-15 1.3862E-14 1.0498E-13
# lat0 lon0 xBary yBary zBary JD0
1.569146 111.290366 0.324399 0.025410 -0.925082 2452997.964183
# Heliocentric elements and errors
Epoch: 2452998.5000 = 2003/12/25
Mean Anomaly: 273.01786 +/- 0.086
Argument of Peri: 114.27500 +/- 0.093
Long of Asc Node: 86.55602 +/- 0.001
Inclination: 3.72588 +/- 0.000
Eccentricity: 0.02558804 +/- 0.0000
Semi-Major Axis: 43.85712197 +/- 0.0024
Time of Perihelion: 2478630.7201 +/- 26.3
Perihelion: 42.73490430 +/- 0.0024
Aphelion: 44.97933963 +/- 0.0025
Period (y) 290.4480 +/- 0.02
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -15.60746057 +/- 0.0002
Ecliptic Y 40.93668230 +/- 0.0006
Ecliptic Z 1.17467553 +/- 0.0000
Ecliptic XDOT -0.00239860 +/- 0.0000
Ecliptic YDOT -0.00099003 +/- 0.0000
Ecliptic ZDOT 0.00015204 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 43.82677361 +/- 0.0005
Geocenter to KBO 42.89661399 +/- 0.0006
# Hcoef: 6.83
The following table shows the complete astrometric record for 03YS179. 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 (03YS179) followed by the observatory code and reference code for the source of the astrometry.
2003 12 24.46344 07 33 06.83 +23 18 15.5 23.4g 03YS179 568 Cq9908 2003 12 24.48664 07 33 06.72 +23 18 15.8 23.6g 03YS179 568 Cq9908 2003 12 24.50988 07 33 06.62 +23 18 16.2 23.8g 03YS179 568 Cq9908 2003 12 25.50403 07 33 01.82 +23 18 28.0 23.6g 03YS179 568 Cq9908 2004 04 15.16648 07 27 18.66 +23 29 45.4 03YS179 675 Cq9908 2004 04 15.21821 07 27 18.72 +23 29 45.3 03YS179 675 Cq9908 2004 04 16.20223 07 27 20.06 +23 29 41.0 03YS179 675 Cq9908 2005 01 08.35280 07 37 18.66 +23 13 42.2 23.0r 03YS179 568 Cq9908 2005 01 08.39064 07 37 18.47 +23 13 42.7 23.1r 03YS179 568 Cq9908 2005 01 08.42845 07 37 18.27 +23 13 43.2 23.1r 03YS179 568 Cq9908 2006 01 28.30717 07 41 08.06 +23 09 27.2 03YS179 675 Cq9908 2006 01 29.29718 07 41 03.19 +23 09 39.0 03YS179 675 Cq9908 2006 01 29.38287 07 41 02.77 +23 09 40.0 23. R 03YS179 675 Cq9908 2008 11 02.68638 08 02 41.87 +22 23 03.9 23.9R 03YS179 250 S~06Ah 2008 11 02.69333 08 02 41.87 +22 23 04.0 03YS179 250 S~06Ah 2008 11 02.70027 08 02 41.87 +22 23 04.0 03YS179 250 S~06Ah 2008 11 02.70652 08 02 41.87 +22 23 04.0 03YS179 250 S~06Ah 2013 03 13.16798 08 16 13.08 +22 01 39.1 22.7R 03YS179 695 C~0ud7 2013 03 14.15346 08 16 10.28 +22 01 46.4 03YS179 695 C~0ud7 2013 03 14.24296 08 16 10.03 +22 01 46.7 03YS179 695 C~0ud7 2020 01 04.363720 08 58 53.17 +19 53 29.1 23.0G 03YS179 705 C~3slk 2020 01 04.425180 08 58 52.93 +19 53 30.4 23.4G 03YS179 705 C~3slk 2020 01 04.531950 08 58 52.43 +19 53 32.2 23.3G 03YS179 705 C~3slk 2020 12 22.30170 09 04 56.432 +19 31 13.10 23.3r 03YS179 269 C~8iQM 2020 12 22.30484 09 04 56.424 +19 31 13.12 22.5z 03YS179 269 C~8iQM 2020 12 22.30751 09 04 56.415 +19 31 13.16 22.7z 03YS179 269 C~8iQM 2020 12 22.31123 09 04 56.400 +19 31 13.25 23.9g 03YS179 269 C~8iQM 2020 12 22.31507 09 04 56.388 +19 31 13.34 23.9g 03YS179 269 C~8iQM 2020 12 22.31886 09 04 56.374 +19 31 13.40 23.1r 03YS179 269 C~8iQM 2020 12 22.32198 09 04 56.367 +19 31 13.46 22.5z 03YS179 269 C~8iQM 2020 12 22.32465 09 04 56.357 +19 31 13.52 22.6z 03YS179 269 C~8iQM 2020 12 22.32733 09 04 56.345 +19 31 13.57 22.5z 03YS179 269 C~8iQM 2020 12 22.33050 09 04 56.333 +19 31 13.59 23.1r 03YS179 269 C~8iQM 2021 02 15.229500 09 00 50.792 +19 49 51.52 23.2G 03YS179 G37 C~4Yr4 2021 02 15.282210 09 00 50.524 +19 49 52.70 03YS179 G37 C~4Yr4 2022 03 02.134460 09 05 02.561 +19 35 39.11 23.5G 03YS179 G37 C~5Rkz 2022 03 02.172770 09 05 02.419 +19 35 40.05 03YS179 G37 C~5Rkz 2022 03 02.212990 09 05 02.242 +19 35 40.66 03YS179 G37 C~5Rkz
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 -0.24 0.00 0.06
2 0.0001 0.00 -0.19 0.00 0.08
3 0.0001 0.00 0.01 0.00 0.20
4 0.0028 0.00 -0.23 0.00 0.04
5 0.3086 0.00 0.20 0.00 -0.24
6 0.3087 0.00 0.12 0.00 -0.11
7 0.3114 0.00 -0.08 0.00 -0.19
8 1.0428 0.00 0.04 0.00 0.01
9 1.0429 0.00 0.14 0.00 0.02
10 1.0430 0.00 0.09 0.00 0.04
11 2.0968 0.00 0.01 0.00 -0.23
12 2.0995 0.00 -0.10 0.00 -0.06
13 2.0997 0.00 -0.01 0.00 -0.05
14 4.8603 0.00 0.05 0.00 0.15
15 4.8603 0.00 0.09 0.00 0.22
16 4.8603 0.00 0.13 0.00 0.19
17 4.8604 0.00 0.17 0.00 0.16
18 9.2175 0.00 0.04 0.00 0.03
19 9.2202 0.00 -0.17 0.00 0.32
20 9.2205 0.00 -0.08 0.00 -0.00
21 16.0298 0.00 -0.15 0.00 -0.32
22 16.0300 0.00 0.16 0.00 -0.24
23 16.0303 0.00 -0.55 0.00 -0.52
24 16.9961 0.00 0.03 0.00 0.10
25 16.9961 0.00 0.07 0.00 0.07
26 16.9962 0.00 0.07 0.00 0.06
27 16.9962 0.00 0.04 0.00 0.09
28 16.9962 0.00 0.05 0.00 0.11
29 16.9962 0.00 0.04 0.00 0.10
30 16.9962 0.00 0.09 0.00 0.11
31 16.9962 0.00 0.08 0.00 0.12
32 16.9962 0.00 0.04 0.00 0.12
33 16.9962 0.00 0.02 0.00 0.09
34 17.1465 0.00 0.11 0.00 -0.12
35 17.1467 0.00 -0.11 0.00 0.04
36 18.1866 0.00 -0.17 0.00 -0.23
37 18.1867 0.00 0.17 0.00 0.06
38 18.1869 0.00 0.11 0.00 0.00
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.
03YS179 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 43.736 43.736 43.736 ecceobj 0.021 0.021 0.021 incobj 3.722 3.722 3.722 qmin 41.973 41.973 41.967 qmax 45.471 45.476 45.478 amean 43.639 43.639 43.639 amin 43.307 43.307 43.308 amax 43.977 43.975 43.979 emean 0.019 0.019 0.019 emin 0.001 0.001 0.001 emax 0.034 0.035 0.034 imean 1.987 1.987 1.987 imin 1.237 1.237 1.237 imax 2.617 2.617 2.616 excite_mean 0.040 0.040 0.040 fracstop 1.000 1.000 1.000 cjmean 3.095 3.095 3.095 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 200.0 200.1 200.1 kozaiamp 179.8 180.0 179.9