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• W1997330816 abstract "Tyrrhena Patera (22°S, 104°E), Mars, is a low-relief (1800 m maximum relief), central-vent volcano whose flanks are dissected with broad (∼5 km wide), flat-floored channels. The easily eroded nature of the shield materials, combined with extremely low flank slopes (≤ 2.0°), suggest that Tyrrhena Patera is composed of pyroclastic materials. These shield deposits are observed to crop out ≥ 600 km from the volcano's summit with measured thicknesses of 100–150 m at these distances. Such dimensions strongly suggest emplacement via pyroclastic flows. Currently available data indicate that these deposits have a mafic composition. Application of models derived for terrestrial pyroclastic flow emplacement reveals that, aside from environmental parameters (atmospheric density, gravity), if all else is held equal, a pyroclastic flow should travel a factor of 3 to 4 times farther on Mars than on Earth. The observed Tyrrhena Patera deposits extend even farther, suggesting that some emplacement mechanism may be enhancing pyroclastic flow runout distances on Mars." @default.
• W1997330816 created "2016-06-24" @default.
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• W1997330816 date "2006-07-01" @default.
• W1997330816 modified "2023-10-04" @default.
• W1997330816 title "Mafic pyroclastic flows at Tyrrhena Patera, Mars: Constraints from observations and models" @default.
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• W1997330816 doi "https://doi.org/10.1016/j.jvolgeores.2006.02.008" @default.
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