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Determination of pre-eruptive conditions of phonolitic magmas using experimental petrology Second year progress report

General Objetives. Objective 3: To demonstrate the utility of experimental petrology in volcanic risk assessment. Objective 1: To determine the pre-eruptive conditions (P, T, volatile content) of phonolitic magmas from Teide and Vesuvius by using experimental petrology. Objective 2: To constrain mineral-melt partitioning of various components (especially volatile species, which largely determine the explosivity potential of eruptions.

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Determination of pre-eruptive conditions of phonolitic magmas using experimental petrology Second year progress report

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    1. Determination of pre-eruptive conditions of phonolitic magmas using experimental petrology (Second year progress report) Group of Volcanology, CSIC, Barcelona, Spain

    3. Working plan 1) Determination of the pre-eruptive conditions ( T, P, f H2O, fO2) of two selected samples from T-PV complex: MB subplinian eruption deposit (2 ka; Ablay et al., 1995) and Lavas Negras (1.2-0.8? ka; Ablay et al., 1998); and one sample from the El Abrigo deposit: (pre-Teide, caldera-forming eruption, 179ka, Martí et al., 1994) 2) Constraining the present state of the Teide volcano 3) Comparison between the eruption dynamics of Teide (effusive) and Las Cañadas (explosive). 4) Comparison between Teide and Vesuvius phonolites

    4. Experiments planning El Abrigo pumice (pre- Teide phonolite)

    5. Experiments planning Montaña Blanca obsidian (Teide phonolite)

    6. RESULTS EA Experimental mineral phases: sanidine/anorthoclase+biotite+magnetite+clinopyroxene+sphene+apatite+nepheline

    8. Preliminary results

    9. El Abrigo experiments: General observations ? ?O2 ? increase stability of mgn ? H2O ? 50ºC increase of the liquidus T of mineral phases, ?px stability, ? tit stability, nepheline is stable at higher P, ? crystallinity at higher T. Presence of magnetite but NOT illmenite Variation on P,T, H2O ? variation on mineral and glass composition, degree of crystallization

    10. EA experimental mineral phases

    11. EA experimental glasses (sat experiments) SiO2: A T=cte, ?P ? ?[SiO2], Non-T effect Al2O3:A T=cte, ?P ? ?[Al2O3], Non-T effect MgO: A P=cte, ?T ? ?[MgO], ?P ? ?[MgO] CaO: A T=cte, ?P ? ?[CaO];?T ? ?[CaO]; crystal. Titanite. MnO and FeO: non-observed trend; affected by magnetite, biotite and pyroxene crystallization. Na2O: T=cte, ?P ? ?[Na2O]; Non-T effect K2O: Non-observed trend TiO2: A P=cte, ?T ? [TiO2]?

    12. EA experimental glasses (non-sat experiments) SiO2: A T=cte, ?P ? ?[SiO2], ?T ? ?[SiO2], Al2O3:not clear influence of T/P MgO: ?T ? ?[MgO], ?P ? ?[MgO] CaO: A T=cte, ?P ? ?[CaO];?T ? ?[CaO]; crystal. Titanite and clpx. MnO and FeO: ?P ? ?[MnO-FeO] Na2O: A T=cte, ?P ? ?[Na2O], Non T effect K2O: Non-observed trend TiO2: A P=cte, ?T ? [TiO2]?

    13. Conclusions Comparing previous petrological data with the new experimental results, we can conclude that the pre-eruptive conditions of El Abrigo pumice (pre- Teide phonolite) were: T: 750ºC-800ºC P:1100 bars ?O2 :NNO-NNO+1. %H2O:3-5%. The presence haüyne, sodalite and apatite at natural assemblage ? S, Cl i F.

    14. Results MB Montaña Blanca obsidian: NNO+1 Water sat-experiments (top) Non-sat-experiments (bottom)

    15. Results MB

    16. MB experiments: general observations

    17. MB experimental mineral phases Experimental phases:anor+bt+clpx+ill+mgn+tit+ap. Biotites:annite-phlogopite: Ti rich biotites ? T ? ?XMg at NNO+1; ? ?O2,? ?XMg DMg linear relationship with P Feldspars: Ab 56-66.5,Or:30-43.; ? T,?PH2O, ? fO2,? ? Or Or nat duplicated T<800ºC,fO2 FQM-PH2O?1kbar Oxides: ? ?O2? ? illmenite (solidus at ?T) - ?Magnetite stability. Mgn: ?T ? ?Mg, on influence of fO2, ? ?O2 ? ?[Fe3+]; ? T ? ?XMg at NNO+1 Clpx: En10-27 Fs22-37 Wo38-43 Ac 7-15(FQM), NNO+1(small crystal size) ? T ? ?XMg at NNO+1 ;? P ? ? Na, ?Fe3+, ? fO2 ? ?XMg

    18. MB experimental glasses Glasses: peralkaline phonolites SiO2:?T ? ?SiO2 at all ?O2. MgO: compatible trend at all ?O2 ?crystallisation of Mg bearing phases NaO: incompatible trend at 1Kbar/compatible trend at 2kbar CaO: low content ?clpx-tit crystallisation

    19. Conclusions Combining previous petrological data with the new experimental data we can conclude that the Montaña Blanca magma chamber contained two phonolitic liquids: Pre-eruptive conditions of the uppermost phonolitic layer were : T:755-800ºC,P:1500bars, ?O2 :FQM-1, 3-4.5%H2O. while those of the lower layer were: 877ºC, water contents<3%.

    20. Experimental Problems Under Mike Carroll’s supervision we have detected the following problems: Furnaces: thermocouple calibration, ?O2 Experiments: variation of water activity ? does not allow to compare data between samples; studies of sample crystalinity (constraining pressure and water activity) Microprobe analysis: problems with mineral analysis (stechyometric and standard deviation checking), Na-loss in glass analysis, problems with microprobe standards

    21. Problem solutions Furnaces: thermocouple calibration ? gold point, ? correction experiments T; ?O2 ? future calculations. Experiments: variation of water activity ? same water activity for all P; studies of sample crystalinity are in progress. Microprobe analysis: problems with mineral analysis ? (stechyometric and standard deviation checking), Na-loss in glass analysis ? create own standards for analyzing and correct Na-loss, problems with microprobe standards ? find new standards

    22. Future work (3rd year) Correction of El Abrigo experimental data. Reversal experiments: checking mineral equilibrium ?Pre-eruptive parameters for EA and MB Experiments for Lavas Negras Experiments for MB (varying water activity) Experiments for Vesuvius

    23. The End

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