Table 3: Fate of the disk mass at 170 000 years.
Scenario I II III IV V

Total Initial Solids $({M}_{\oplus})$ 24.39 23.68 22.89 20.61 14.59

Total Surviving Solids $({M}_{\oplus})$ 22.06 (90%) 21.04 (89%) 12.05 (53%) 14.75 (70%) 9.91 (68%)

Interior Surviving Solids $({M}_{\oplus})$ 15.65 (64%) 14.60 (62%) 4.96 (22%) 2.86 (14%) 0.00 (0%)

$N, f_{{\rm proto}}$ 1, 1 3, 1 1, 0.99 1, 1 0, 0

Exterior Surviving Solids $({M}_{\oplus})$ 6.41 (26%) 6.44 (27%) 7.09 (31%) 11.59 (56%) 9.91 (68%)

$N, f_{{\rm proto}}$ 32, 0.66 32, 0.63 25, 0.65 23, 0.93 16, 0.89

Accreted by Star $({M}_{\oplus})$ 1.05 (4%) 0.74 (3%) 9.60 (42%) 5.81 (28%) 3.03 (21%)

Accreted by Giant $({M}_{\oplus})$ 1.19 (5%) 1.88 (8%) 1.24 (5%) 0.34 (2%) 1.65 (11%)

Ejected $({M}_{\oplus})$ 0.00 (0%) 0.025 (0.1%) 0.00 (0%) 0.025 (0.1%) 0.00 (0%)

**Table 3:** Fate of the disk mass at 170 000 years.
Scenario	I	II	III	IV	V
Total Initial Solids $({M}_{\oplus})$	24.39	23.68	22.89	20.61	14.59
Total Surviving Solids $({M}_{\oplus})$	22.06 (90%)	21.04 (89%)	12.05 (53%)	14.75 (70%)	9.91 (68%)
Interior Surviving Solids $({M}_{\oplus})$	15.65 (64%)	14.60 (62%)	4.96 (22%)	2.86 (14%)	0.00 (0%)
$N, f_{{\rm proto}}$	1, 1	3, 1	1, 0.99	1, 1	0, 0
Exterior Surviving Solids $({M}_{\oplus})$	6.41 (26%)	6.44 (27%)	7.09 (31%)	11.59 (56%)	9.91 (68%)
$N, f_{{\rm proto}}$	32, 0.66	32, 0.63	25, 0.65	23, 0.93	16, 0.89
Accreted by Star $({M}_{\oplus})$	1.05 (4%)	0.74 (3%)	9.60 (42%)	5.81 (28%)	3.03 (21%)
Accreted by Giant $({M}_{\oplus})$	1.19 (5%)	1.88 (8%)	1.24 (5%)	0.34 (2%)	1.65 (11%)
Ejected $({M}_{\oplus})$	0.00 (0%)	0.025 (0.1%)	0.00 (0%)	0.025 (0.1%)	0.00 (0%)

Source LaTeX | All tables | In the text

	1 Introduction.
	2 Description of the model
	3 Results
	4 Caveats and future model improvements
	5 Conclusions
	References