Consequences of the simultaneous formation of giant planets by the core accretion mechanism

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Table 2:

Isolated formation of Jupiter and Saturn for a disk with surfaces densities of solids and gas ${\propto }a^{-3/2}$ .
MM		Jupiter				Saturn
SN
	$\Sigma_{\rm s}$	$\rho_{\rm g}$	$M_{\rm c}$	$t_{\rm f}$	$\Sigma_{\rm s}$	$\rho_{\rm g}$	$M_{\rm c}$	$t_{\rm f}$
4	10.12	2.54	21.31	5.34	--	--	--	--
5	12.65	3.17	26.61	2.86	--	--	--	--
6	15.18	3.81	31.35	1.76	6.14	0.73	17.07	9.62
7	17.71	4.45	36.32	1.09	7.17	0.85	20.83	4.89
8	20.24	5.08	41.48	0.62	8.19	0.97	23.76	2.85
9	22.77	5.72	45.39	0.33	9.22	1.09	26.38	1.75
10	25.30	6.35	46.09	0.16	10.24	1.21	28.72	1.08

Notes. ^(*) $\Sigma_{\rm s}~[{\rm g~cm}^{-2}]$ and $\rho_{\rm g}~[10^{-11}~{\rm g~cm}^{-3}]$ are the initial surface density of solids and the initial volumetric density of gas at the disk mid-plane at the position of Jupiter and Saturn, respectively. $M_{\rm c}~[M_{\oplus}]$ is the final core mass and $t_{\rm f}~[{\rm Myr}]$ is the formation time.

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