Trachybasalt scoria from a cinder cone near the Mexican volcanic front contain phenocrysts of olivine with chromite inclu-sions, apatite, augite and hornblende, with microphenocrysts of plagioclase. The water-saturated phase relations reproduce the phenocryst assemblage between 1040C and 970C with water contents of between 25 and 45%(50---150MPa).The absence of biotite phenocrysts in the scoria places a tight constraint on the pressure---temperature conditions of phenocryst equilibration, as there is only a small zone where biotite does not accompany hornblende in the experiments. Diluting the fluid phase with CO2 changes the composition of the olivine, indicating that CO2 was only a minor component of the fluid of the scoria. Horn-blende is stable to 1040C at oxygen fugacities of NNO 2 (where NNO is the nickel---nickel oxide buffer), but at lower oxygen fugacities, the upper limit is 990C. There is a progress-ive increase in crystallinity in experimental runs as both pressure and temperature decrease. Isobaric plots of crystallinity show that the onset of hornblende crystallization involves a reaction relation, and also results in a marked 15---40 vol. % increase in crystallinity. Ascending hydrous magmas intersecting the cooler crust could be trapped there by the large increase in crystallinity accompanying the isobaric crystallization of hornblende.
No takes yet. Share an insight, caveat, or question.
Jenni Barclay (2004) studied this question.
Synapse has enriched 5 related papers. Consider them for comparative context: