A chemical perspective on planet formation in reduced systems

Open Access

Table 2

Condensation temperatures, $T_{c}^{50 %}$ $Mathematical equation: $\[T_{c}^{50 \%}\]$$ (K) for elements in solar-like (Lodders03; C/O= 0.50), transitional (HD 94151; C/O= 0.89), and reduced (HD 24633; C/O= 0.95) systems at three different disk pressures.

Star	Pressure	Al	Ca	Cr	Fe	Mg	Na	Ni	S	Si	Ti
Lodders03 (C/O = 0.50)	10⁻² bar	1795	1645	1500	1530	1485	1180	1555	645	1455	1765
	10⁻⁴ bar	1655	1475	1310	1330	1335	1045	1355	645	1320	1595
	10⁻⁶ bar	1530	1345	1160	1180	1220	940	1200	645	1205	1460
HD 94151 (C/O = 0.89)	10⁻² bar	1620	1525	1515	1545	1240	1090	1570	635	1315	1660
	10⁻⁴ bar	1505	1390	1320	1345	1060	935	1365	1055	1170	1505
	10⁻⁶ bar	1390	1270	1170	1190	945	830	1210	940	1055	1375
HD 24633 (C/O = 0.95)	10⁻² bar	1490	1455	1435	1540	1220	1040	1555	1205	1315	1850
	10⁻⁴ bar	1325	1285	1245	1340	1060	935	1345	1065	1155	1645
	10⁻⁶ bar	1190	1145	1105	1195	940	830	1180	945	1040	1470

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