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Journal of Volcanology and Geothermal Research
Volume 172, Issues 1-2, 10 May 2008, Pages 38-60
Physical Volcanology of Large Igneous Provinces
 
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doi:10.1016/j.jvolgeores.2005.11.011    
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Copyright © 2007 Elsevier B.V. All rights reserved.

Geological evolution of the Coombs–Allan Hills area, Ferrar large igneous province, Antarctica: Debris avalanches, mafic pyroclastic density currents, phreatocauldrons

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Pierre-Simon RossCorresponding Author Contact Information, a, E-mail The Corresponding Author, James D.L. Whitea and Murray McClintocka

aDepartment of Geology, University of Otago, PO Box 56, Dunedin, New Zealand


Received 5 April 2005; 
accepted 12 November 2005. 
Available online 12 November 2007.

Abstract

The Jurassic Ferrar large igneous province of Antarctica comprises igneous intrusions, flood lavas, and mafic volcaniclastic deposits (now lithified). The latter rocks are particularly diverse and well-exposed in the Coombs–Allan Hills area of South Victoria Land, where they are assigned to the Mawson Formation. In this paper we use these rocks in conjunction with the pre-Ferrar sedimentary rocks (Beacon Supergroup) and the lavas themselves (Kirkpatrick Basalt) to reconstruct the geomorphological and geological evolution of the landscape. In the Early Jurassic, the surface of the region was an alluvial plain, with perhaps 1 km of mostly continental siliciclastic sediments underlying it. After the fall of silicic ash from an unknown but probably distal source, mafic magmatism of the Ferrar province began. The oldest record of this event at Allan Hills is a ≤ 180 m-thick debris-avalanche deposit (member m1 of the Mawson Formation) which contains globular domains of mafic igneous rock. These domains are inferred to represent dismembered Ferrar intrusions emplaced in the source area of the debris avalanche; shallow emplacement of Ferrar magmas caused a slope failure that mobilized the uppermost Beacon Supergroup, and the silicic ash deposits, into a pre-existing valley or basin.

The period which followed (‘Mawson time’) was the main stage for explosive eruptions in the Ferrar province, and several cubic kilometres of both new magma and sedimentary rock were fragmented over many years. Phreatomagmatic explosions were the dominant fragmentation mechanism, with magma–water interaction taking place in both sedimentary aquifers and existing vents filled by volcaniclastic debris. At Coombs Hills, a vent complex or ‘phreatocauldron’ was formed by coalescence of diatreme-like structures; at Allan Hills, member m2 of the Mawson Formation consists mostly of thick, coarse-grained, poorly sorted layers inferred to represent the lithified deposits of pyroclastic density currents. Meanwhile at Carapace Nunatak, mafic clasts were mixed with detrital material to form the Carapace Sandstone in alluvial and eventually lacustrine environments.

Eruptions then became largely effusive, producing hundreds of metres of flood lavas that covered the landscape (‘Kirkpatrick time’). In places, lava flowed into ephemeral lakes to form pillow-palagonite breccias (base of sequence, Carapace Nunatak) or pillow lavas (top of sequence, Coombs Hills). Several generations of Ferrar intrusions were emplaced during the course of these events; at least three can be distinguished based on field relations. New geochemical data indicates that for the Ferrar province, magma involved in the explosive eruptions had the same major element composition as that which produced shallow intrusions and lavas. We also note the possibility that flood lavas were fed by plugs cross-cutting the Mawson Formation at Coombs Hills, rather than by major dikes extending to the surface. Finally, we infer that eruption plumes were limited to the troposphere and that direct environmental impacts were thus likely restricted to the southern hemisphere.

Keywords: large igneous province; Ferrar; Antarctica; Mawson Formation; Kirkpatrick Basalt; Coombs Hills; Allan Hills

Article Outline

1. Introduction
1.1. A word on stratigraphy, nomenclature and samples
2. Coombs Hills
2.1. The Coombs Hills vent complex
2.2. Bedded volcaniclastic deposits
2.2.1. The Pyramid
2.2.2. The East Ridge
2.3. Kirkpatrick lavas (Mt Brooke)
3. Allan Hills
3.1. Southern Allan Hills
3.2. Central Allan Hills
4. Carapace Nunatak
4.1. Carapace Sandstone
4.2. Kirkpatrick lavas
4.3. Volcaniclastic intervals
5. Preliminary geochemistry
5.1. Established chemical types
5.2. New data
6. Environmental impacts of Mawson-forming eruptions
7. Geomorphological and geological evolution of the Coombs–Allan Hills area
7.1. Setting the stage
7.2. Initiation of Ferrar magmatism: debris avalanches and topographic relief
7.3. Main explosive stage (‘Mawson time’)
7.4. Effusive stage (‘Kirkpatrick time’)
7.5. Clastic and igneous intrusions
8. Summary and conclusions
Acknowledgements
References