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: 14UV277 # Created Wed Apr 24 01:16:37 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 17 observations of 17 # Arc: 8.16y # First observation: 2014/10/29 # Last observation: 2022/12/26 # Chi-squared of fit: 12.09 DOF: 28 RMS: 0.15 # Min/Max residuals: -0.33 0.48 # Exact a, adot, b, bdot, g, gdot: 1.678544E-05 3.017719E-02 -7.921724E-06 -1.215423E-02 2.714721E-02 3.125911E-03 # Covariance matrix: 3.9554E-13 -1.9501E-13 -7.7767E-14 6.3610E-14 6.5783E-14 -6.9578E-13 -1.9501E-13 1.5533E-13 6.3738E-14 -5.7428E-14 3.1397E-14 6.0274E-13 -7.7767E-14 6.3738E-14 2.4166E-13 -7.1142E-14 -2.3106E-14 2.9239E-13 6.3610E-14 -5.7428E-14 -7.1142E-14 4.0844E-14 -8.2757E-15 -2.5203E-13 6.5783E-14 3.1397E-14 -2.3106E-14 -8.2757E-15 4.5753E-13 -4.0005E-14 -6.9578E-13 6.0274E-13 2.9239E-13 -2.5203E-13 -4.0005E-14 2.6950E-12 # lat0 lon0 xBary yBary zBary JD0 -26.632000 33.844495 -0.028181 -0.445582 -0.888987 2456959.824318 # Heliocentric elements and errors Epoch: 2456960.5000 = 2014/10/30 Mean Anomaly: 7.46330 +/- 0.004 Argument of Peri: 213.93146 +/- 0.009 Long of Asc Node: 166.64824 +/- 0.000 Inclination: 33.54146 +/- 0.000 Eccentricity: 0.39325326 +/- 0.0001 Semi-Major Axis: 61.27571212 +/- 0.0123 Time of Perihelion: 2453328.3865 +/- 2.2 Perihelion: 37.17883860 +/- 0.0101 Aphelion: 85.37258565 +/- 0.0185 Period (y) 479.6680 +/- 0.14 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 28.15562487 +/- 0.0007 Ecliptic Y 18.91780624 +/- 0.0005 Ecliptic Z -16.51245308 +/- 0.0004 Ecliptic XDOT -0.00192173 +/- 0.0000 Ecliptic YDOT 0.00237382 +/- 0.0000 Ecliptic ZDOT -0.00123694 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 37.72636947 +/- 0.0006 Geocenter to KBO 36.83616093 +/- 0.0009 # Hcoef: 7.84
The following table shows the complete astrometric record for 14UV277. 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 (14UV277) followed by the observatory code and reference code for the source of the astrometry.
2014 10 29.32354 02 42 10.471 -12 18 43.21 23.1r 14UV277 W84 C~55Sh 2014 10 31.30073 02 42 00.524 -12 19 44.53 23.3i 14UV277 W84 C~55Sh 2014 11 28.23917 02 39 43.208 -12 28 22.29 23.4r 14UV277 W84 C~55Sh 2015 12 17.17640 02 46 01.040 -12 31 54.84 23.6r 14UV277 W84 C~55Sh 2015 12 17.17778 02 46 01.034 -12 31 54.68 24.0g 14UV277 W84 C~55Sh 2016 09 24.31448 02 59 45.255 -12 01 28.55 23.8r 14UV277 W84 C~55Sh 2016 09 25.26060 02 59 42.222 -12 02 15.23 24.4g 14UV277 W84 C~55Sh 2016 11 22.21833 02 55 16.544 -12 35 04.33 23.7r 14UV277 W84 C~55Sh 2016 12 23.17124 02 53 07.838 -12 33 57.00 24.3g 14UV277 W84 C~55Sh 2017 10 29.33518 03 04 47.293 -12 28 23.78 23.0i 14UV277 W84 C~55Sh 2017 10 29.33656 03 04 47.293 -12 28 23.97 23.3r 14UV277 W84 C~55Sh 2017 10 29.33794 03 04 47.277 -12 28 24.23 24.1g 14UV277 W84 C~55Sh 2017 12 22.17446 03 00 37.876 -12 37 02.21 24.3r 14UV277 W84 C~55Sh 2017 12 23.17406 03 00 34.536 -12 36 47.30 24.2g 14UV277 W84 C~55Sh 2022 12 26.115840 03 36 47.698 -12 38 11.80 23.6G 14UV277 G37 C~69bM 2022 12 26.168850 03 36 47.548 -12 38 11.00 14UV277 G37 C~69bM 2022 12 26.230750 03 36 47.265 -12 38 09.99 14UV277 G37 C~69bM
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 0.10 0.00 0.22
2 0.0054 0.00 -0.03 0.00 -0.13
3 0.0819 0.00 0.04 0.00 -0.06
4 1.1331 0.00 -0.02 0.00 0.01
5 1.1331 0.00 -0.03 0.00 0.16
6 1.9055 0.00 0.04 0.00 -0.06
7 1.9081 0.00 -0.08 0.00 0.06
8 2.0668 0.00 -0.12 0.00 -0.14
9 2.1515 0.00 -0.05 0.00 -0.05
10 3.0007 0.00 0.02 0.00 0.14
11 3.0007 0.00 0.12 0.00 -0.00
12 3.0007 0.00 -0.01 0.00 -0.22
13 3.1481 0.00 -0.06 0.00 0.22
14 3.1509 0.00 0.20 0.00 -0.12
15 8.1582 0.00 -0.33 0.00 0.03
16 8.1584 0.00 0.48 0.00 -0.02
17 8.1585 0.00 -0.19 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.
14UV277 quality flag:3 Type: SCATNEAR SCATNEAR SCATNEAR axisobj 62.058 62.058 62.058 ecceobj 0.401 0.401 0.401 incobj 33.455 33.455 33.455 qmin 35.662 35.622 35.651 qmax 88.046 88.039 88.217 amean 61.272 61.245 61.274 amin 60.603 60.500 60.595 amax 62.167 62.169 62.218 emean 0.399 0.399 0.399 emin 0.380 0.380 0.381 emax 0.417 0.416 0.418 imean 32.473 32.464 32.472 imin 31.954 31.949 31.955 imax 33.159 33.146 33.132 excite_mean 0.669 0.669 0.669 fracstop 1.000 1.000 1.000 cjmean 2.698 2.698 2.698 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 179.9 180.1 179.9 kozaiamp 180.0 179.9 180.0