Hostname: page-component-78c5997874-xbtfd Total loading time: 0 Render date: 2024-11-10T14:38:28.893Z Has data issue: false hasContentIssue false

Amethyst-bearing lava flows in the Paraná Basin (Rio Grande do Sul, Brazil): cooling, vesiculation and formation of the geodic cavities

Published online by Cambridge University Press:  19 October 2006

DOMINIQUE PROUST
Affiliation:
UMR 6532 CNRS, HydrASA, Faculté des Sciences, 40 Avenue du recteur Pineau, 86022 Poitiers cedex, France
CLAUDE FONTAINE
Affiliation:
UMR 6532 CNRS, HydrASA, Faculté des Sciences, 40 Avenue du recteur Pineau, 86022 Poitiers cedex, France

Abstract

Size distribution data obtained from detailed field study of bubbles and amethyst-geodes in the basaltic lava flows of the Serra Geral Formation (Ametista do Sul, Rio Grande do Sul, Brazil) are used in cooling and vesiculation models to infer the origin and the formation processes of the geodic cavities. Coupled field observations and modelling results emphasize that (1) the formation of geodes in the studied lava flow can be explained, qualitatively and quantitatively, by the exsolution of magmatic gas from the supersaturated melt with no need for external surface water supply; (2) the vertically elongated habits of the geodes result from higher cooling rate of the magma in contact with the accumulating bubbles; and (3) the abnormal metre-sized geodes with their branching habits result not only from the diffusive/decompressive bubble growth but also from the coalescence of inwards-progressing tubular cavities.

Type
Original Article
Copyright
© 2006 Cambridge University Press

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)