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- W1993849611 abstract "Volcanism on Mars is dominated by mafic or ultramafic products. On Earth, mafic volcanics are typically emplaced through small-scale pyroclastic activity such as lava fountaining or Strombolian eruptions, resulting in lava flows. Tyrrhena and Hadriaca Paterae, large, central-vent volcanoes on Mars, however, appear to be primarily constructed of mafic pyroclastic deposits (probably pyroclastic flows), and magma–water (or ice) interactions were not necessarily the cause of these explosive eruptions. The volcanotectonic conditions which generated highly explosive basaltic eruptions on Mars may exist on Earth as well: Masaya Caldera Complex, Nicaragua, has produced large-volume, basaltic ignimbrite, Plinian ash-fall and surge deposits, without overt magma–water interactions. Basaltic magma apparently originated ∼100 km beneath Masaya, and ascended faster than ∼100 cm s−1through an established conduit, allowing the magma and exsolved volatiles to reach the surface simultaneously. The combination of deep-sourced magma and rapid rise rate may have also generated ignimbrite-like basaltic pyroclastic deposits at Zavaritski Volcano, Russia, and Ambrym, Vanuatu. Examination of these terrestrial volcanoes may further our understanding of large-scale mafic pyroclastic activity on Mars." @default.
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- W1993849611 date "1996-08-01" @default.
- W1993849611 modified "2023-10-14" @default.
- W1993849611 title "Explosive Mafic Volcanoes on Mars and Earth: Deep Magma Sources and Rapid Rise Rate" @default.
- W1993849611 doi "https://doi.org/10.1006/icar.1996.0132" @default.
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