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Table 2
Orbital parameters of 10 solutions derived by Genoid with the keplerian model for the outer moon of (3749) Balam with a similar fp.
| fp | Semi-major axis | Period | Eccentricity | Mass | Density | |
| (mas) | (km) | (days) | (1014 kg) | (g/cm3) | ||
|
|
||||||
| Sol 1 | 12.66 | 194.74 | 54.41 | 0.768 | 1.98 | 3.7 |
| Sol 2 | 13.80 | 189.10 | 61.39 | 0.670 | 1.42 | 2.6 |
| Sol 3 | 12.65 | 196.18 | 69.45 | 0.596 | 1.24 | 2.3 |
| Sol 4 | 12.36 | 203.42 | 81.43 | 0.573 | 1.01 | 1.9 |
| Sol 5 | 12.58 | 237.71 | 91.36 | 0.349 | 1.28 | 2.4 |
| Sol 6 | 12.94 | 219.23 | 97.42 | 0.543 | 0.88 | 1.6 |
| Sol 7 | 12.48 | 260.06 | 109.54 | 0.365 | 1.16 | 2.2 |
| Sol 8 | 13.28 | 256.28 | 122.51 | 0.512 | 0.89 | 1.7 |
| Sol 9 | 13.17 | 297.73 | 136.68 | 0.386 | 1.12 | 2.1 |
| Sol 10 | 13.88 | 285.74 | 162.46 | 0.625 | 0.70 | 1.3 |
Notes. The best fitted solution for (3749) Balam is given in Table 1. The density is derived by using the radiometric size Deq = 4.68 ± 0.54 km derived from Spitzer/IRS observations.
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