Table 3: Fate of the disk mass at the end of each run.
Scenario I II III IV V
Total Initial Solids $({M}_{\oplus})$ 24.81 24.81 24.81 24.81 24.81
Total Surviving Solids $({M}_{\oplus})$ 16.60 (67%) 16.69 (67%) 17.40 (70%) 21.23 (86%) 20.22 (81%)
Interior Surviving Solids $({M}_{\oplus})$ 0.88 (4%) 0.65 (2%) 1.00 (4%) 0.84 (3%) 0.31 (1%)
$N, f_{{\rm proto}}$ 0, 0 0, 0 0, 0 0, 0 0, 0
Exterior Surviving Solids $({M}_{\oplus})$ 15.72 (63%) 16.04 (65%) 16.40 (66%) 20.39 (82%) 19.90 (80%)
$N, f_{{\rm proto}}$ 39, 0.27 29, 0.28 33, 0.42 31, 0.63 23, 0.66
Accreted by Star $({M}_{\oplus})$ 0.01 (0.04%) 0.01 (0.04%) 0.11 (0.4%) 0.0 (0%) 0.0 (0%)
Accreted by Giant $({M}_{\oplus})$ 8.20 (33%) 7.85 (32%) 6.77 (27%) 3.41 (14%) 4.59 (19%)
Ejected $({M}_{\oplus})$ 0.00 (0%) 0.26 (1%) 0.51 (2%) 0.17 (1%) 0.0 (0%)


Source LaTeX | All tables | In the text