Table 1.

Integral parameters for Mars model atmospheres models with dust depletion factors f of 0.1, 0.01, and 0.001 and for accretion rates ${\dot{M}}_{\mathrm{acc}}$ between $1\times {10}^{-6}$ and $1\times {10}^{-9}$ Earth masses per year. L is the luminosity resulting from the accretion of planetesimals; $M_{\mathrm{atm}}$ is the atmospheric mass up to the Bondi radius; and surface pressure and temperature on the surface are denoted as $P_{\mathrm{s}}$ and $T_{\mathrm{s}}$, respectively.

${\dot{M}}_{\mathrm{acc}}$ ($M_{\mathrm{Mars}}/\mathrm{yr}$)	$f_{\mathrm{dust}}$	L (erg/s)	$M_{\mathrm{atm}}$ (g)	$P_{\mathrm{s}}$ (bar)	$T_{\mathrm{s}}$ (K)
$9.35\times {10}^{-9}$	0.001	$2.39\times {10}^{22}$	$6.58\times {10}^{22}$	7.81	600
$9.35\times {10}^{-9}$	0.01	$2.39\times {10}^{22}$	$3.21\times {10}^{22}$	3.38	639
$9.35\times {10}^{-9}$	0.1	$2.39\times {10}^{22}$	$1.00\times {10}^{22}$	8.08	690
$9.35\times {10}^{-8}$	0.001	$2.38\times {10}^{23}$	$2.66\times {10}^{22}$	2.58	693
$9.35\times {10}^{-8}$	0.01	$2.38\times {10}^{23}$	$9.76\times {10}^{21}$	0.763	724
$9.35\times {10}^{-8}$	0.1	$2.38\times {10}^{23}$	$2.86\times {10}^{21}$	0.155	754
$9.35\times {10}^{-7}$	0.001	$2.38\times {10}^{24}$	$8.81\times {10}^{21}$	0.628	795
$9.35\times {10}^{-7}$	0.01	$2.38\times {10}^{24}$	$2.84\times {10}^{21}$	0.151	784
$9.35\times {10}^{-7}$	0.1	$2.38\times {10}^{24}$	$5.25\times {10}^{20}$	0.028	841
$9.35\times {10}^{-6}$	0.001	$2.38\times {10}^{25}$	$2.70\times {10}^{21}$	0.132	885
$9.35\times {10}^{-6}$	0.01	$2.38\times {10}^{25}$	$5.14\times {10}^{20}$	0.028	862
$9.35\times {10}^{-6}$	0.1	$2.38\times {10}^{25}$	$3.21\times {10}^{19}$	0.005	960