Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
6438947 | Geochimica et Cosmochimica Acta | 2013 | 11 Pages |
Abstract
This result appears inconsistent with the shallow depth of origin (â¼<2 m) assumed for MIL 03346, further supporting the discrepancy between MIL 03346 textural and petrologic evidence of fast cooling and the abovementioned Tc results obtained for augite. Therefore, a tentative scenario is that, soon after eruption and initial quench and while still at relatively high-T (â¼600 °C), MIL 03346 was blanketed with subsequent lava flows that slowed down the cooling rate and allowed the augite Fe2+-Mg exchange reaction to proceed.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geochemistry and Petrology
Authors
M.C. Domeneghetti, A.M. Fioretti, F. Cámara, C. McCammon, M. Alvaro,