Determination of preeruptive conditions of phonolitic magmas using experimental petrology Second yea - PowerPoint PPT Presentation

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Determination of preeruptive conditions of phonolitic magmas using experimental petrology Second yea

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Title: Determination of preeruptive conditions of phonolitic magmas using experimental petrology Second yea


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

Joan Andújar Fabio Teixidó Joan Martí
2
General Objetives
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
Objective 3 To demonstrate the utility of
experimental petrology in volcanic risk assessment
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/anorthoclasebiotitemagnetiteclinopyrox
    enespheneapatitenepheline

7
Preliminary results
El Abrigo pumice (pre- Teide phonolite)
water-sat exp.
8
Preliminary results
El Abrigo pumice (pre- Teide phonolite) non-sat
exp
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
  • Experimental phasessan/anorbttitpxap(neph)
  • Biotites -phlogopite-annite(XMg vs. Al)
  • - XMg Fe/Mg nat are between
    NNO-NNO1??O2 ? ?XMg
  • - TinatgtTiexp
  • - Pcte linear relationship of XMg
    vs.T ?
  • formation T 763ºC (sat) and
    765ºC (non-sat)
  • - Tcte linear relationship between
    DMg vs.P ?
  • formation P 1270(sat) and 1100 (non-sat)
  • Feldspars sanidine-anorthoclase,
    Orexp29.6-55.6, Abexp77.4-45,
    Anexp0.52-5.73
  • Ornat(34.5-40.3) is duplicated at 750ºC and
    1000 bars, and NNO,H2O3-5. ?H2O
    experiments ? ? Or
  • Oxides titanomagnetites.(no illmenite). ?no nat
    data.
  • Titanite very frequent at NNO1 and water
    saturated, low compositional variation with P T
    changes.
  • Apatite small crystal size ? analysis errors
  • Pyroxene small crystal size at water-sat
    conditions water non-sat Exp. Pyr
    En4.64-14 Wo31.9-64.8 Fs 0.56-42.7
  • Nepheline small crystal size ? analysis errors

11
EA experimental glasses (sat experiments)
  • SiO2 A Tcte, ?P ? ?SiO2, Non-T effect
  • Al2O3A Tcte, ?P ? ?Al2O3, Non-T effect
  • MgO A Pcte, ?T ? ?MgO, ?P ? ?MgO
  • CaO A Tcte, ?P ? ?CaO?T ? ?CaO crystal.
    Titanite.
  • MnO and FeO non-observed trend affected by
    magnetite, biotite and pyroxene crystallization.
  • Na2O Tcte, ?P ? ?Na2O Non-T effect
  • K2O Non-observed trend
  • TiO2 A Pcte, ?T ? TiO2?

12
EA experimental glasses (non-sat experiments)
  • SiO2 A Tcte, ?P ? ?SiO2, ?T ? ?SiO2,
  • Al2O3not clear influence of T/P
  • MgO ?T ? ?MgO, ?P ? ?MgO
  • CaO A Tcte, ?P ? ?CaO?T ? ?CaO crystal.
    Titanite and clpx.
  • MnO and FeO ?P ? ?MnO-FeO
  • Na2O A Tcte, ?P ? ?Na2O, Non T effect
  • K2O Non-observed trend
  • TiO2 A Pcte, ?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
  • P1100 bars
  • ?O2 NNO-NNO1.
  • H2O3-5.
  • The presence haüyne, sodalite and apatite at
    natural assemblage ? S, Cl i F.

14
Results MB
  • Montaña Blanca obsidian NNO1
  • Water sat-experiments (top)
  • Non-sat-experiments (bottom)

15
Results MB
Montaña Blanca obsidian FMQ Water
sat-experiments (left) Non-sat-experiments
(right)
16
MB experiments general observations
  • ?H2O (NNO1) ?solidus T of feldspars, biotite
    about 50ºC illmenite ? solidus T about 25ºC and
    reduce its stability
  • ?H2O (FMQ) ?solidus T of feldspars about 30ºC
    disappearance of titanite.
  • ? ?O2 Increase on illmenite stability to higher
    T low decrease on solidus T of pyroxene, apatite
    and titanite at water saturated conditions
    disappearance of titanite.
  • Variation on P,T, H2O ? variation on mineral,
    glass composition, degree of crystallization

17
MB experimental mineral phases
  • Experimental phasesanorbtclpxillmgntitap.
  • Biotitesannite-phlogopite
  • Ti rich biotites
  • ? T ? ?XMg at NNO1 ? ?O2,? ?XMg
  • DMg linear relationship with P
  • Feldspars Ab 56-66.5,Or30-43.
  • ? T,?PH2O, ? fO2,? ? Or
  • Or nat duplicated Tlt800ºC,fO2
    FQM-PH2O?1kbar
  • Oxides ? ?O2? ? illmenite (solidus at ?T) -
    ?Magnetite stability.
  • Mgn ?T ? ?Mg, on influence of fO2, ? ?O2
    ? ?Fe3 ? T ? ?XMg at NNO1
  • Clpx En10-27 Fs22-37 Wo38-43 Ac 7-15(FQM),
    NNO1(small crystal size)
  • ? T ? ?XMg at NNO1 ? 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
  • T755-800ºC,P1500bars, ?O2 FQM-1,
    3-4.5H2O.
  • while those of the lower layer were
  • 877ºC, water contentslt3.

20
Experimental Problems
  • Under Mike Carrolls 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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