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Using pyroxene microphenocrysts to determine cosmogenic 3He concentrations in old volcanic rocks: an example of landscape development in central Gran Canaria
Determinations of cosmogenic 3He exposure ages and erosion rates in volcanic rocks older than a few hundred thousand years are complicated by the presence of radiogenic He in addition to the magmatic and cosmogenic He, in phenocryst minerals. However, by analysing microphenocrysts (that crystallised...
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Published in: | Quaternary science reviews 2005, Vol.24 (1), p.211-222 |
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Main Authors: | , , , |
Format: | Article |
Language: | English |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | Determinations of cosmogenic
3He exposure ages and erosion rates in volcanic rocks older than a few hundred thousand years are complicated by the presence of radiogenic He in addition to the magmatic and cosmogenic He, in phenocryst minerals. However, by analysing microphenocrysts (that crystallised on or immediately prior to eruption) that have not trapped magmatic He, the three-component problem can be eliminated and accurate determinations of cosmogenic
3He made. In this study, we perform three experiments using pyroxene microphenocrysts in basaltic clasts in the Pliocene Ayacata Formation breccias, Gran Canaria, that demonstrate they are free of magmatic He. Exposure ages and erosion rates calculated from the cosmogenic
3He concentrations are combined with a geomorphological study, to produce a tentative interpretation of landscape evolution in the mountainous interior of Gran Canaria. Long-term steady-state erosion rates of 14–24
mm
ka
−1 are recorded from bedrock erosional surfaces on a high plateau. Headwall retreat rates for a major drainage system of 1.6
m
ka
−1 have been constrained from the ca 225
ka exposure age of a boulder emplaced on slopes beneath the headwall. Strath terraces and boulders in a small canyon system yield much younger exposure ages of 47–43
ka. |
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ISSN: | 0277-3791 1873-457X |
DOI: | 10.1016/j.quascirev.2004.07.004 |