Orbit Fit and Astrometric record for 15RC281

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: 15RC281   
# Created Wed Dec 25 02:10:25 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     35 observations of     35
# Arc:   6.28y
# First observation: 2015/06/23
#  Last observation: 2021/10/03
# Chi-squared of fit:     7.12 DOF:     64 RMS:  0.08
# Min/Max residuals:    -0.19    0.20
# Exact a, adot, b, bdot, g, gdot:
  1.404614E-05  1.969227E-02  1.245293E-06  1.171698E-03  2.147474E-02  7.266441E-04
# Covariance matrix:
  1.3172E-13 -3.5748E-14 -1.9393E-15 -2.3076E-15  7.5202E-14 -2.3464E-13
 -3.5748E-14  1.8951E-13 -9.4685E-15  1.3877E-14  9.5605E-14  1.6498E-12
 -1.9393E-15 -9.4685E-15  5.8858E-14 -1.6380E-14 -8.8087E-15 -8.6967E-14
 -2.3076E-15  1.3877E-14 -1.6380E-14  1.4938E-14  6.6799E-15  1.3079E-13
  7.5202E-14  9.5605E-14 -8.8087E-15  6.6799E-15  1.5623E-13  8.4217E-13
 -2.3464E-13  1.6498E-12 -8.6967E-14  1.3079E-13  8.4217E-13  1.5523E-11
#      lat0       lon0       xBary       yBary       zBary        JD0
    2.684121   10.667696    1.004192   -0.007236    0.156422  2457197.102358
# Heliocentric elements and errors
Epoch:              2457196.5000  =  2015/06/23
Mean Anomaly:          127.49433 +/-     0.471
Argument of Peri:      268.73038 +/-     0.469
Long of Asc Node:      331.69277 +/-     0.003
Inclination:             4.39463 +/-     0.000
Eccentricity:         0.01773141 +/-    0.0001
Semi-Major Axis:     45.91288903 +/-    0.0029
Time of Perihelion: 2416953.6514 +/-     148.8
Perihelion:          45.09878867 +/-    0.0071
Aphelion:            46.72698938 +/-    0.0072
Period (y)              311.1073 +/-      0.03
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           45.73980618 +/-    0.0008
Ecliptic Y            7.59522284 +/-    0.0002
Ecliptic Z            2.18079612 +/-    0.0000
Ecliptic XDOT        -0.00038314 +/-    0.0000
Ecliptic YDOT         0.00247681 +/-    0.0000
Ecliptic ZDOT         0.00015362 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   46.41737047 +/-    0.0008
Geocenter to KBO     46.56632852 +/-    0.0009
# Hcoef:  7.28

The following table shows the complete astrometric record for 15RC281. 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 (15RC281) followed by the observatory code and reference code for the source of the astrometry.

2015 06  23.60158  00 34 59.106  +06 41 28.30  24.2r 15RC281   568  C~2nvs      
2015 07  14.55424  00 35 09.709  +06 44 11.29  23.7r 15RC281   568  C~2nvs      
2015 07  19.52115  00 35 07.214  +06 44 17.81  23.9r 15RC281   568  C~2nvs      
2015 08  13.49219  00 34 27.309  +06 41 47.66  23.7r 15RC281   568  C~2nvs      
2015 08  13.61738  00 34 26.988  +06 41 46.16  23.9r 15RC281   568  C~2nvs      
2015 08  19.55480  00 34 11.360  +06 40 28.26  24.0r 15RC281   568  C~2nvs      
2015 08  19.62493  00 34 11.160  +06 40 26.89  24.5r 15RC281   568  C~2nvs      
2015 08  20.43022  00 34 08.887  +06 40 15.41  23.6r 15RC281   568  C~2nvs      
2015 08  20.47949  00 34 08.738  +06 40 14.55  23.8r 15RC281   568  C~2nvs      
2015 09  07.57672  00 33 08.967  +06 34 46.85  24.2w 15RC281   568  C~2nvs      
2015 09  09.40442  00 33 02.179  +06 34 07.86  23.8r 15RC281   568  C~2nvs      
2015 09  09.44553  00 33 02.023  +06 34 06.97  23.7r 15RC281   568  C~2nvs      
2015 09  09.48644  00 33 01.867  +06 34 06.03  23.9r 15RC281   568  C~2nvs      
2015 09  10.51074  00 32 58.013  +06 33 43.78  24.0w 15RC281   568  C~2nvs      
2015 09  18.47260  00 32 27.010  +06 30 41.45  24.3w 15RC281   568  C~2nvs      
2015 10  08.36042  00 31 05.631  +06 22 21.68  24.1w 15RC281   568  C~2nvs      
2015 10  08.41303  00 31 05.415  +06 22 20.34  24.0w 15RC281   568  C~2nvs      
2015 10  09.33000  00 31 01.670  +06 21 56.47  24.3w 15RC281   568  C~2nvs      
2015 11  10.45634  00 29 03.824  +06 08 54.64  24.1w 15RC281   568  C~2nvs      
2015 12  08.25463  00 28 05.205  +06 01 29.02  24.4w 15RC281   568  C~2nvs      
2016 01  01.31705  00 28 02.272  +05 59 53.04  24.0w 15RC281   568  C~2nvs      
2016 01  02.26815  00 28 03.152  +05 59 55.46  24.2w 15RC281   568  C~2nvs      
2016 09  05.49045  00 37 23.163  +07 06 12.50  23.6w 15RC281   568  C~2nvs      
2016 09  06.44465  00 37 19.708  +07 05 52.78  24.4w 15RC281   568  C~2nvs      
2016 09  06.48592  00 37 19.559  +07 05 52.01  24.0w 15RC281   568  C~2nvs      
2016 09  26.44346  00 36 01.356  +06 58 12.32  24.2w 15RC281   568  C~2nvs      
2016 11  03.46810  00 33 32.211  +06 42 14.83  24.1w 15RC281   568  C~2nvs      
2016 12  25.26033  00 32 02.824  +06 30 24.22  24.0w 15RC281   568  C~2nvs      
2017 01  02.30275  00 32 07.595  +06 30 27.43  24.6w 15RC281   568  C~2nvs      
2017 01  30.23419  00 33 04.659  +06 35 03.54  24.5w 15RC281   568  C~2nvs      
2017 09  16.50931  00 40 52.360  +07 33 09.27  24.2w 15RC281   568  C~2nvs      
2017 09  22.46275  00 40 28.634  +07 30 49.81  24.2w 15RC281   568  C~2nvs      
2021 10  03.301800 00 56 31.623  +09 28 31.32  23.9G 15RC281   G37  C~55Wp      
2021 10  03.338380 00 56 31.473  +09 28 30.56        15RC281   G37  C~55Wp      
2021 10  03.375160 00 56 31.311  +09 28 29.57        15RC281   G37  C~55Wp      

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     0.12       0.00    -0.04
     2   0.0574      0.00     0.05       0.00    -0.08
     3   0.0710      0.00     0.02       0.00    -0.07
     4   0.1393      0.00     0.08       0.00    -0.08
     5   0.1397      0.00     0.00       0.00    -0.09
     6   0.1559      0.00     0.09       0.00     0.17
     7   0.1561      0.00     0.12       0.00    -0.19
     8   0.1583      0.00     0.05       0.00     0.10
     9   0.1585      0.00    -0.03       0.00    -0.04
    10   0.2080      0.00    -0.07       0.00    -0.01
    11   0.2130      0.00    -0.16       0.00     0.03
    12   0.2131      0.00    -0.14       0.00     0.02
    13   0.2132      0.00    -0.13       0.00    -0.03
    14   0.2160      0.00    -0.02       0.00     0.02
    15   0.2378      0.00     0.00       0.00    -0.13
    16   0.2923      0.00    -0.02       0.00     0.03
    17   0.2924      0.00     0.03       0.00     0.06
    18   0.2949      0.00     0.11       0.00    -0.04
    19   0.3829      0.00     0.07       0.00    -0.01
    20   0.4590      0.00     0.05       0.00     0.09
    21   0.5249      0.00    -0.08       0.00     0.11
    22   0.5275      0.00     0.05       0.00     0.06
    23   1.2044      0.00     0.09       0.00     0.20
    24   1.2070      0.00     0.04       0.00    -0.04
    25   1.2071      0.00     0.11       0.00     0.04
    26   1.2617      0.00    -0.03       0.00    -0.00
    27   1.3658      0.00    -0.10       0.00    -0.03
    28   1.5076      0.00    -0.01       0.00     0.04
    29   1.5296      0.00    -0.04       0.00     0.05
    30   1.6061      0.00     0.12       0.00    -0.10
    31   2.2338      0.00    -0.04       0.00     0.05
    32   2.2501      0.00    -0.12       0.00     0.07
    33   6.2798      0.00    -0.00       0.00    -0.09
    34   6.2799      0.00     0.06       0.00     0.05
    35   6.2800      0.00    -0.04       0.00    -0.04

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.

15RC281    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        46.380    46.380    46.380
ecceobj         0.015     0.015     0.015
incobj          4.379     4.379     4.379
qmin           44.709    44.708    44.713
qmax           47.701    47.701    47.695
amean          46.129    46.130    46.129
amin           45.773    45.773    45.772
amax           46.493    46.494    46.491
emean           0.015     0.015     0.015
emin            0.003     0.003     0.003
emax            0.026     0.026     0.026
imean           5.506     5.506     5.506
imin            5.166     5.166     5.166
imax            5.829     5.829     5.829
excite_mean     0.097     0.097     0.097
fracstop        1.000     1.000     1.000
cjmean          3.116     3.116     3.116

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       178.5     178.5     178.7
kozaiamp        180.0     180.0     180.0