Table 3
State of the system 11 000 years after the giant impact.
| Name | Mc (M⊕) | 2π/Ω(hr) | Ns | Mdisk(M☾) | mf(M☾) |
|---|---|---|---|---|---|
| 500b073S | 1.001784 | 5.9167 | 1 | 0.6379 | 0.01295 |
| 500b075S | 0.999374 | 5.6802 | 2 | 0.9892 | 0.01081 |
| half-Earth | 1.075642 | 4.0277 | 2 | 1.3045 | 0.01616 |
| random | 1.000164 | 5.2217 | 2 | 0.6761 | 0.03041 |
Notes. Clicking on the simulation’s name redirects to a log of the simulation (use wget in terminal to download it). Mc and Ω are the mass and sidereal rotation of Earth. Ns is the number of significant submoons (massive enough to be at hydrostatic equilibrium). Mdisk and mf are the total mass in orbit and the mass of the inner fluid disk.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.