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Table 3
Asteroid masses obtained with INPOP13a, significantly different from values found in INPOP10e, and inducing a change in the Earth-planets distances smaller than 5 meters over the fitting interval.
IAU designation | INPOP13a | INPOP10e | Konopliv et al. (2011) | ||
number | 1012 × M⊙ | 1012 × M⊙ | 1012 × M⊙ | ||
|
|||||
1 | 468.430 ± 1.184 | 467.267 ± 1.855 | 467.90 ± 3.25 | ||
2 | 103.843 ± 0.982 | 102.654 ± 1.600 | 103.44 ± 2.55 | ||
9 | 3.637 ± 0.400 | 4.202 ± 0.670 | 3.28 ± 1.08 | ||
15 | 14.163 ± 0.555 | 15.839 ± 0.950 | 14.18 ±1.49 | ||
16 | 11.212 ± 1.373 | 12.613 ± 2.208 | 12.41 ± 3.44 | ||
19 | 5.182 ± 0.342 | 4.892 ± 0.513 | 3.20 ± 0.53 | ||
46 | 3.076 ± 0.446 | 3.525 ± 0.743 | – | ||
51 | 3.287 ± 0.485 | 0.009 ± 0.004 | – | ||
65 | 8.789 ± 2.266 | 4.210 ± 0.863 | – | ||
78 | 1.486 ± 0.504 | 2.562 ± 0.574 | – | ||
105 | 2.070 ± 0.365 | 3.046 ± 0.635 | – | ||
106 | 3.369 ± 0.408 | 3.870 ± 0.411 | – | ||
134 | 3.451 ± 0.595 | 1.014 ± 0.368 | – | ||
194 | 4.872 ± 0.452 | 5.601 ± 0.636 | – | ||
324 | 5.087 ± 0.189 | 4.769 ± 0.435 | 5.34 ± 0.99 |
Notes. The uncertainties are given at 1 published sigma and compared with Konopliv et al. (2011).
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