Flood lavas on Earth, Io and Mars

Flood lavas are major geological features on all the major rocky planetary bodies. They provide important insight into the dynamics and chemistry of the interior of these bodies. On the Earth, they appear to be associated with major and mass extinction events. It is therefore not surprising that the...

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Published in:Journal of the Geological Society
Main Authors: Keszthelyi, L., Self, S., Thordarson, T.
Format: Article in Journal/Newspaper
Language:unknown
Published: 2006
Subjects:
Online Access:https://zenodo.org/record/1236152
https://doi.org/10.1144/0016-764904-503
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spelling ftzenodo:oai:zenodo.org:1236152 2023-05-15T16:52:52+02:00 Flood lavas on Earth, Io and Mars Keszthelyi, L. Self, S. Thordarson, T. 2006-03-01 https://zenodo.org/record/1236152 https://doi.org/10.1144/0016-764904-503 unknown https://zenodo.org/record/1236152 https://doi.org/10.1144/0016-764904-503 oai:zenodo.org:1236152 info:eu-repo/semantics/openAccess https://creativecommons.org/publicdomain/zero/1.0/legalcode info:eu-repo/semantics/article publication-article 2006 ftzenodo https://doi.org/10.1144/0016-764904-503 2023-03-11T02:34:17Z Flood lavas are major geological features on all the major rocky planetary bodies. They provide important insight into the dynamics and chemistry of the interior of these bodies. On the Earth, they appear to be associated with major and mass extinction events. It is therefore not surprising that there has been significant research on flood lavas in recent years. Initial models suggested eruption durations of days and volumetric fluxes of order 107 m3 s−1 with flows moving as turbulent floods. However, our understanding of how lava flows can be emplaced under an insulating crust was revolutionized by the observations of actively inflating pahoehoe flows in Hawaii. These new ideas led to the hypothesis that flood lavas were emplaced over many years with eruption rates of the order of 104 m3 s−1. The field evidence indicates that flood lava flows in the Columbia River Basalts, Deccan Traps, Etendeka lavas, and the Kerguelen Plateau were emplaced as inflated pahoehoe sheet flows. This was reinforced by the observation of active lava flows of ≥100 km length on Io being formed as tube-fed flows fed by moderate eruption rates (102–103 m3 s−1). More recently it has been found that some flood lavas are also emplaced in a more rapid manner. New high-resolution images from Mars revealed 'platy–ridged' flood lava flows, named after the large rafted plates and ridges formed by compression of the flow top. A search for appropriate terrestrial analogues found an excellent example in Iceland: the 1783–1784 Laki Flow Field. The brecciated Laki flow top consists of pieces of pahoehoe, not aa clinker, leading us to call this 'rubbly pahoehoe'. Similar flows have been found in the Columbia River Basalts and the Kerguelen Plateau. We hypothesize that these flows form with a thick, insulating, but mobile crust, which is disrupted when surges in the erupted flux are too large to maintain the normal pahoehoe mode of emplacement. Flood lavas emplaced in this manner could have (intermittently) reached effusion rates of the order of 106 ... Article in Journal/Newspaper Iceland Zenodo Kerguelen Laki ENVELOPE(-18.237,-18.237,64.070,64.070) Journal of the Geological Society 163 2 253 264
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description Flood lavas are major geological features on all the major rocky planetary bodies. They provide important insight into the dynamics and chemistry of the interior of these bodies. On the Earth, they appear to be associated with major and mass extinction events. It is therefore not surprising that there has been significant research on flood lavas in recent years. Initial models suggested eruption durations of days and volumetric fluxes of order 107 m3 s−1 with flows moving as turbulent floods. However, our understanding of how lava flows can be emplaced under an insulating crust was revolutionized by the observations of actively inflating pahoehoe flows in Hawaii. These new ideas led to the hypothesis that flood lavas were emplaced over many years with eruption rates of the order of 104 m3 s−1. The field evidence indicates that flood lava flows in the Columbia River Basalts, Deccan Traps, Etendeka lavas, and the Kerguelen Plateau were emplaced as inflated pahoehoe sheet flows. This was reinforced by the observation of active lava flows of ≥100 km length on Io being formed as tube-fed flows fed by moderate eruption rates (102–103 m3 s−1). More recently it has been found that some flood lavas are also emplaced in a more rapid manner. New high-resolution images from Mars revealed 'platy–ridged' flood lava flows, named after the large rafted plates and ridges formed by compression of the flow top. A search for appropriate terrestrial analogues found an excellent example in Iceland: the 1783–1784 Laki Flow Field. The brecciated Laki flow top consists of pieces of pahoehoe, not aa clinker, leading us to call this 'rubbly pahoehoe'. Similar flows have been found in the Columbia River Basalts and the Kerguelen Plateau. We hypothesize that these flows form with a thick, insulating, but mobile crust, which is disrupted when surges in the erupted flux are too large to maintain the normal pahoehoe mode of emplacement. Flood lavas emplaced in this manner could have (intermittently) reached effusion rates of the order of 106 ...
format Article in Journal/Newspaper
author Keszthelyi, L.
Self, S.
Thordarson, T.
spellingShingle Keszthelyi, L.
Self, S.
Thordarson, T.
Flood lavas on Earth, Io and Mars
author_facet Keszthelyi, L.
Self, S.
Thordarson, T.
author_sort Keszthelyi, L.
title Flood lavas on Earth, Io and Mars
title_short Flood lavas on Earth, Io and Mars
title_full Flood lavas on Earth, Io and Mars
title_fullStr Flood lavas on Earth, Io and Mars
title_full_unstemmed Flood lavas on Earth, Io and Mars
title_sort flood lavas on earth, io and mars
publishDate 2006
url https://zenodo.org/record/1236152
https://doi.org/10.1144/0016-764904-503
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geographic Kerguelen
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