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• W2073804711 abstract "A vast area of smooth plains in southeastern Elysium, here referred to as the “Cerberus Formation,” is interpreted to be of volcanic origin. Surface morphology, lobate edges of the unit, the identification of vents (low shields), and the embayment relation of the unit with adjacent older units all suggest a volcanic origin. The plains were formed by the eruption of low-viscosity lavas that filled a topographic depression in southeast Elysium and then flowed into western Amazonis Planitia. Flow into western Amazonis was facilitated by a series of channels, carved by an earlier fluvial episode, which were exploited by lavas as they moved down slope. Crater frequencies and stratigraphic relations indicate that the unit is very young—Upper Amazonian. The presence of such young flood lavas indicates; (1) late in Martian history, large-scale eruptions of low-viscosity lava was still possible; (b) sufficient heat remained in the mantle to mobilize large quantities of magma; and (c) flood volcanism either continued or resumed in Elysium after activity of the large central volcanoes had ceased. Each of these points are important considerations in understanding the Martian thermal and volcanic history." @default.
• W2073804711 created "2016-06-24" @default.
• W2073804711 creator A5046133757 @default.
• W2073804711 date "1990-12-01" @default.
• W2073804711 modified "2023-10-02" @default.
• W2073804711 title "Recent flood lavas in the Elysium region of Mars" @default.
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• W2073804711 doi "https://doi.org/10.1016/0019-1035(90)90095-q" @default.
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