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: 15KV175
# Created Fri Nov 22 02:10:24 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 35 observations of 35
# Arc: 6.95y
# First observation: 2014/05/29
# Last observation: 2021/05/12
# Chi-squared of fit: 2.27 DOF: 64 RMS: 0.04
# Min/Max residuals: -0.13 0.10
# Exact a, adot, b, bdot, g, gdot:
1.654205E-05 2.776269E-02 -5.499947E-06 -9.193605E-03 2.678098E-02 8.805773E-04
# Covariance matrix:
1.6495E-13 -1.3968E-13 -2.8032E-14 3.6421E-14 -6.6675E-15 -5.7386E-13
-1.3968E-13 1.7179E-13 3.6899E-14 -4.8507E-14 -1.3348E-14 7.6476E-13
-2.8032E-14 3.6899E-14 8.6952E-14 -3.7004E-14 1.8575E-15 1.8499E-13
3.6421E-14 -4.8507E-14 -3.7004E-14 3.3324E-14 1.2590E-15 -2.4205E-13
-6.6675E-15 -1.3348E-14 1.8575E-15 1.2590E-15 1.4439E-13 -2.2931E-14
-5.7386E-13 7.6476E-13 1.8499E-13 -2.4205E-13 -2.2931E-14 3.8153E-12
# lat0 lon0 xBary yBary zBary JD0
6.107465 -127.537266 -0.269062 0.104135 -0.972692 2456806.851688
# Heliocentric elements and errors
Epoch: 2456806.5000 = 2014/05/29
Mean Anomaly: 11.72726 +/- 0.016
Argument of Peri: 145.29060 +/- 0.024
Long of Asc Node: 70.19055 +/- 0.000
Inclination: 19.29255 +/- 0.000
Eccentricity: 0.16203545 +/- 0.0001
Semi-Major Axis: 45.46195159 +/- 0.0040
Time of Perihelion: 2453159.2584 +/- 5.1
Perihelion: 38.09550385 +/- 0.0047
Aphelion: 52.82839933 +/- 0.0057
Period (y) 306.5352 +/- 0.04
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -23.00526360 +/- 0.0003
Ecliptic Y -30.37912247 +/- 0.0004
Ecliptic Z 3.97258263 +/- 0.0001
Ecliptic XDOT 0.00212986 +/- 0.0000
Ecliptic YDOT -0.00188317 +/- 0.0000
Ecliptic ZDOT -0.00092484 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 38.31334883 +/- 0.0004
Geocenter to KBO 37.33994748 +/- 0.0005
# Hcoef: 7.01
The following table shows the complete astrometric record for 15KV175. 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 (15KV175) followed by the observatory code and reference code for the source of the astrometry.
2014 05 29.35091 15 26 35.916 -12 28 30.45 22.8r 15KV175 568 C~2nvi 2014 05 29.38978 15 26 35.715 -12 28 29.99 22.7r 15KV175 568 C~2nvi 2014 05 29.42862 15 26 35.517 -12 28 29.59 22.7r 15KV175 568 C~2nvi 2014 05 30.45852 15 26 30.283 -12 28 18.39 22.7r 15KV175 568 C~2nvi 2014 05 31.37479 15 26 25.660 -12 28 08.53 22.8r 15KV175 568 C~2nvi 2014 06 21.39293 15 24 49.053 -12 25 33.30 22.8r 15KV175 568 C~2nvi 2014 07 19.27038 15 23 25.700 -12 26 18.75 22.6r 15KV175 568 C~2nvi 2015 02 20.65667 15 38 02.837 -13 41 48.24 22.9r 15KV175 568 C~2nvi 2015 03 19.57074 15 37 38.157 -13 38 47.02 22.9r 15KV175 568 C~2nvi 2015 04 18.51079 15 35 53.149 -13 32 08.20 22.8r 15KV175 568 C~2nvi 2015 05 17.38343 15 33 27.493 -13 25 02.94 22.7r 15KV175 568 C~2nvi 2015 05 17.42514 15 33 27.264 -13 25 02.35 22.7r 15KV175 568 C~2nvi 2015 05 17.46733 15 33 27.033 -13 25 01.78 22.7r 15KV175 568 C~2nvi 2015 05 24.36911 15 32 50.588 -13 23 33.16 22.8r 15KV175 568 C~2nvi 2015 05 24.41533 15 32 50.340 -13 23 32.60 22.8r 15KV175 568 C~2nvi 2015 05 24.45620 15 32 50.120 -13 23 32.11 22.8r 15KV175 568 C~2nvi 2015 05 26.44379 15 32 39.733 -13 23 08.31 22.7r 15KV175 568 C~2nvi 2015 06 18.34328 15 30 48.624 -13 19 45.91 22.8r 15KV175 568 C~2nvi 2015 06 18.38434 15 30 48.442 -13 19 45.67 22.8r 15KV175 568 C~2nvi 2015 06 21.35896 15 30 35.794 -13 19 30.97 22.8r 15KV175 568 C~2nvi 2015 07 10.39102 15 29 29.261 -13 19 11.46 22.8r 15KV175 568 C~2nvi 2015 07 17.34619 15 29 12.190 -13 19 38.72 23.0r 15KV175 568 C~2nvi 2015 07 18.31678 15 29 10.155 -13 19 44.12 22.9r 15KV175 568 C~2nvi 2016 02 06.62508 15 43 25.205 -14 33 06.66 23.2w 15KV175 568 C~2nvi 2016 02 12.61062 15 43 36.442 -14 33 25.66 23.2w 15KV175 568 C~2nvi 2016 03 15.61859 15 43 31.192 -14 31 34.85 23.1w 15KV175 568 C~2nvi 2016 04 03.53855 15 42 39.905 -14 28 15.61 23.0w 15KV175 568 C~2nvi 2016 04 08.58811 15 42 21.162 -14 27 11.25 23.0w 15KV175 568 C~2nvi 2016 04 29.46970 15 40 47.012 -14 22 21.28 22.9w 15KV175 568 C~2nvi 2016 05 04.40478 15 40 21.949 -14 21 11.50 22.9w 15KV175 568 C~2nvi 2016 05 30.47820 15 38 04.679 -14 15 41.03 23.0w 15KV175 568 C~2nvi 2016 07 04.29009 15 35 31.537 -14 12 17.42 23.0w 15KV175 568 C~2nvi 2016 07 05.35837 15 35 28.024 -14 12 17.43 23.2w 15KV175 568 C~2nvi 2021 05 12.390800 16 09 23.769 -18 34 54.89 23.0G 15KV175 G37 C~4pVs 2021 05 12.422370 16 09 23.613 -18 34 54.35 15KV175 G37 C~4pVs
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 -0.03 0.00 0.02
2 0.0001 0.00 -0.02 0.00 0.05
3 0.0002 0.00 0.04 0.00 0.02
4 0.0030 0.00 0.04 0.00 -0.10
5 0.0055 0.00 0.01 0.00 -0.07
6 0.0631 0.00 0.06 0.00 0.00
7 0.1394 0.00 0.01 0.00 -0.00
8 0.7318 0.00 -0.04 0.00 -0.01
9 0.8055 0.00 -0.02 0.00 -0.01
10 0.8875 0.00 -0.03 0.00 0.01
11 0.9666 0.00 0.03 0.00 -0.03
12 0.9667 0.00 -0.03 0.00 -0.00
13 0.9668 0.00 -0.08 0.00 -0.00
14 0.9857 0.00 -0.05 0.00 0.02
15 0.9858 0.00 -0.07 0.00 0.01
16 0.9859 0.00 -0.09 0.00 0.00
17 0.9914 0.00 0.02 0.00 0.01
18 1.0541 0.00 0.00 0.00 0.01
19 1.0542 0.00 0.00 0.00 0.03
20 1.0623 0.00 0.01 0.00 -0.03
21 1.1144 0.00 -0.01 0.00 0.00
22 1.1335 0.00 0.02 0.00 0.05
23 1.1361 0.00 0.02 0.00 -0.00
24 1.6927 0.00 0.08 0.00 -0.00
25 1.7091 0.00 0.05 0.00 -0.04
26 1.7968 0.00 -0.02 0.00 0.03
27 1.8486 0.00 0.00 0.00 -0.01
28 1.8624 0.00 0.05 0.00 0.05
29 1.9196 0.00 0.01 0.00 0.05
30 1.9331 0.00 0.02 0.00 -0.02
31 2.0045 0.00 0.02 0.00 0.05
32 2.0998 0.00 0.02 0.00 0.04
33 2.1027 0.00 -0.01 0.00 -0.08
34 6.9543 0.00 -0.11 0.00 -0.13
35 6.9543 0.00 0.08 0.00 0.10
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.
15KV175 quality flag:3 Type: SCATEXTD SCATEXTD SCATEXTD axisobj 45.141 45.140 45.141 ecceobj 0.156 0.156 0.156 incobj 19.308 19.308 19.308 qmin 37.174 37.173 37.174 qmax 54.292 54.251 54.281 amean 45.532 45.532 45.532 amin 45.140 45.126 45.140 amax 45.968 45.968 45.968 emean 0.165 0.165 0.165 emin 0.150 0.150 0.150 emax 0.182 0.181 0.182 imean 17.732 17.732 17.732 imin 17.232 17.232 17.232 imax 18.277 18.271 18.270 excite_mean 0.346 0.346 0.346 fracstop 1.000 1.000 1.000 cjmean 2.971 2.971 2.971 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 181.2 181.1 181.2 kozaiamp 180.0 180.0 180.0