**Table 2:** Typical dust volume composition $V_{\rm s}/V_{\rm tot}$ , mass composition $M_{\rm s}/M_{\rm tot}$ , and mean particles sizes $\langle a\rangle~[\mu$ m] as a function of local temperature for models as depicted in Fig. 2. ( $\nearrow$ ) - increasing in T-interval; ( $\searrow$ ) - decreasing in T-interval.
T	$V_{\rm s}/V_{\rm tot}$	$M_{\rm s}/M_{\rm tot}$	$\langle a\rangle$
$\rm [K]$			$\rm [\mu$ m]
700	24% MgSiO₃, 20% Mg₂SiO₄	1. MgSiO₃	10^-3
.	12% SiO₂, 10% SiO, 9% FeS	2. Mg₂SiO₄	.
.	{MgO, FeO, Fe₂O₃} <9%	3. FeS, Fe₂O₃, FeO	.
.	{Fe, Al₂O₃}<5%	4. SiO₂, MgO, Fe	.
950	{TiO₂, CaTiO₃} <1%	5. SiO	10^-2
950			10^-2
.	strongly changing		.
1200			10^-0.5
1200	35% Mg₂SiO₄, 23% SiO₂	1. Fe	10^-0.5
.	<20% MgSiO₃ ( $\searrow$ )	2. Mg₂SiO₄	.
.	15% Fe, 5% MgO	3. SiO₂/MgSiO₃	.
1700	everything else <5%	4. MgO	10
1700			10
.	strongly changing		.
1900	(SiO, MgO peaking but low %)		10²
1900	72% Fe ( $\searrow$ )	1. Fe	10²
.	20% Al₂O₃ ( $\nearrow$ ), <5% TiO₂	2. Al₂O₃ ( $\nearrow$ )	$(\star)$
2100	10% CaTiO₃ (at 2100 K)	3. CaTiO₃	0

$(\star)$ Mean grain sizes $\langle a\rangle$ can reach up to 10^3.5 in lower gravity
atmospheres like giant-gas planets (compare Fig. 4).

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