HPx-eos: igneous sets

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Multiple sets of x-eos for magmatic systems have been published. As of December 2024, the sets recommended for use are:

We have removed the following sets of x-eos from this site, after discovering an algebraic error in the formulation of the melt x-eos:

See also: which x-eos for phases in each set?

Calculations in anhydrous subalkaline to alkaline systems

The W24 igneous set.

Citation: Weller, OM, Holland, TJB, Soderman, CR, Green, ECR, Powell, R, Beard, CD & Riel, N (2024). New Thermodynamic Models for Anhydrous Alkaline-Silicate Magmatic Systems. Journal of Petrology 65 egae098. For calculations in anhydrous subalkaline to alkaline magmatic systems.

As of December 2024, these x-eos can be used in MAGEMin (Riel et al, 2022), or in THERMOCALC version 3.51 and later. Download input files for THERMOCALC here:

For calculations in hydrous or anhydrous subalkaline systems

The G25 igneous set.

Citation: Green, ECR, Holland, TJB, Powell, R, Weller, OM, & Riel, N (2025). Corrigendum to: Melting of peridotites through to granites: a simple thermodynamic model in the system KNCFMASHTOCr, and, A thermodynamic model for the subsolidus evolution and melting of peridotite. Journal of Petrology, XXXXX

As of December 2024, these x-eos can be used in MAGEMin (Riel et al, 2022), or in THERMOCALC version 3.51 and later. Download input files for THERMOCALC here:

Which x-eos for which set?

The four sets of x-eos for magmatic systems listed above use various versions of x-eos for specific phases, some of which were published prior to H18. They also use different versions of the Holland & Powell (2011) internally-consistent dataset of end-member thermodynamic data. The following table summarizes the x-eos for individual phases and the dataset versions used in the four sets:

PhasesG25W24T21*H18*
silicate meltliq_G25wliq_W24dliq_T21dliq_H18w
aqueous fluidfl_G25fl_H18
olivineol_H18ol_H18ol_H18ol_H18
garnetg_W24g_W24g_T21g_H18
spinel-groupspl_T21spl_T21spl_T21spl_H18
feldsparsfsp_H22fsp_H22fsp_T21fsp_H03
clinopyroxenecpx_W24cpx_W24cpx_T21cpx_H18
orthopyroxeneopx_W24opx_W24opx_T21opt_h18
ilmenite/hematiteilm_W24ilm_W24ilm_W00
biotitebi_G25bi_H18
muscovitemu_W14mu_W14
clinoamphiboleamp_G16amp_G16
epidoteep_H11ep_H11
cordieritecd_G25cd_H18
nephelinenph_W24
kalsilitekals_W24
leucitelct_W24
melilitemel_W24
Dataset version6.366.366.346.33

*should not be used due to algebraic mistake in melt x-eos.

The codes used in the x-eos names refer to the following studies, in addition to the four referenced above:

H22 – Holland, TJB, Green, ECR & Powell, R (2022). A thermodynamic model for feldspars in KAlSi3O8-NaAlSi3O8-CaAl2Si2O8 for mineral equilibrium calculations. Journal of Metamorphic Geology 40 587-600

G16 – The “metabasite” set. Green, ECR, White, RW, Diener, JFA, Powell, R, Holland, TJB &
Palin, RM (2016). Activity-composition relations for the calculation of partial melting equilibria in metabasic rocks. Journal of Metamorphic Geology 34 845-869

W14 – The “metapelite” set. New mineral activity-composition relations for thermodynamic calculations in metapelitic systems. Journal of Metamorphic Geology 32 261-286

H11 – Holland, TJB & Powell, R (2011). An improved and extended internally consistent thermodynamic dataset for phases of petrological interest, involving a new equation of state for solids. Journal of Metamorphic Geology 29 333-383

H03 – Holland, TJB & Powell, R (2003). Activity-composition relations for phases in petrological calculations: an asymmetric multicomponent formulation. Contributions to Mineralogy and Petrology 145 492-501

W00 – White, RW, Powell, R, Holland, TJB & Worley, B (2000). The effect of TiO2 and Fe2O3 on metapelitic assemblages at greenschist and amphibolite facies conditions: mineral equilibria calculations in the system K2O-FeO-MgO-Al2O3-SiO2-H2O-TiO2-Fe2O3. Journal of Metamorphic Geology 18 497-511

Contact us

Please contact us if you find problems with the Weller et al (2024) or Green et al (2025) x-eos, or if you think there is other information we should include on this page.