Free Access

Table 3

Distribution of trapping in a 1:1 resonance, collisions, crossings, and trappings that are MMRs or gap trappings due to the equality between the gas disk and pebble angular velocities.

Mass ratio Collision radius Co-orbitals Collisions Crossings Trappings

μ2 = 10-4 0.005 RHill <1% 36% 62% 2%
(b = 0.1) 0.05 RHill <1% 38% 60% 2%
μ2 = 3 × 10-4 0.005 RHill 47% 4% 49%
(b = 0.25) 0.05 RHill 48% 3% 49%
μ2 = 3 × 10-4 0.005 RHill 68% 3% 29%
(b = 0.3) 0.05 RHill 69% 2% 29%
μ2 = 6 × 10-4 0.005 RHill 60% 2% 38%
(b = 0.5) 0.05 RHill 61% 1% 38%
μ2 = 6 × 10-4 0.005 RHill 37% 1% 62%
(b = 0.6) 0.05 RHill 38% <1% 62%
μ2 = 10-3 0.005 RHill 13% 1% 86%
(b = 0.9) 0.05 RHill 14% <1% 86%
μ2 = 10-3 0.005 RHill 17% 2% 81%
(b = 0.99) 0.05 RHill 18% 1% 81%

Notes.The range of the planet eccentricity is 0.07 < e2 ≤ 0.105.

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.