Table 4
Two submoons at hydrostatic equilibrium.
| Name | m1 | m2 | a1 | a2 | e1 | e2 | I1 | I2 |
|---|---|---|---|---|---|---|---|---|
| 500b073S | 0.625 | ... | 9.516 | ... | 0.5828 | ... | 0.32° | ... |
| 500b075S | 0.944 | 0.035 | 7.663 | 3.314 | 0.0269 | 0.042 | 1.84° | 0.56° |
| half-Earth | 1.219 | 0.069 | 8.623 | 3.677 | 0.0052 | 0.062 | 3.13° | 12.0° |
| random | 0.644 | 0.002 | 8.587 | 3.188 | 0.3675 | 0.150 | 0.51° | 0.29° |
Notes. Characteristics of the two submoons massive enough to be at hydrostatic equilibrium (more massive than Mimas) 11 000 years after the giant impact for simulations of Table 1. Masses are in Lunar masses and semi-major axes are in Earth radii. The inclinations are with respect to the equatorial plane. Clicking on the simulation’s name redirects to a log of all collisions.
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