Free Access
Table 1.
Initial conditions.
| Planet | a (AU) | e | I (deg) | ω, Ω, λ (deg) |
|---|---|---|---|---|
| J1 | 3.0000 | 0.05 | 1° | Random ∼U[0−360 ° ) |
| J2 | 4.6765 | 0.05 | 1° | Random ∼U[0−360 ° ) |
| J3 | 7.2899 | 0.05 | 1° | Random ∼U[0−360 ° ) |
Notes. We ran 500 N-body simulations. Each simulation had three Jupiter-like planets separated by five mutual Hill radii. The eccentricity and inclination were fixed, and the other orbital angles (longitude of periastron, longitude of ascending node, mean longitude) were randomised.
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.