Tropical Mountain Glaciers on Mars: Volcano-Ice Interactions and Influences on Glacial Evolution

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Tropical Mountain Glaciers on Mars: Volcano-Ice Interactions and Influences on Glacial Evolution Seventh International Conference on Mars 3123.pdf TROPICAL MOUNTAIN GLACIERS ON MARS: VOLCANO-ICE INTERACTIONS AND INFLUENCES ON GLACIAL EVOLUTION. L. Wilson1 and J. W. Head2; 1Environmental Science Dept., Lancaster University, Lancaster LA1 4YQ, UK ([email protected]); 2Dept. Geological Sciences, Brown University, Providence, RI 02912, USA ([email protected]). Introduction: Late Amazonian fan-shaped the Arsia deposit and are separated by about 25-30 km. deposits on the northwest flanks of the Tharsis Graben, pits and moberg-like ridges characterize the Montes volcanoes are interpreted to have formed as a eastern ridge. The western structure contains a lobe- result of cold-based tropical mountain glaciation [1- shaped plateau and crater near the edge of the hummocky 6] (Figs. 1, 2). Deposits and landforms interpreted to facies, and forms subaerial cones along its northern have formed during subglacial eruptions have been extension, between the inner and outer ridged facies, and documented beneath and within these deposits [4, 7- again outside the glacial deposits to the north. The lobe- 8]. These include low ridges interpreted to be dikes, shaped plateau (~9 km long and 6 km wide) extends lobate deposits interpreted to be steep-sided flows, downslope and the adjacent crater is ~4 km wide and linear mounds and low ridges interpreted to be ~100 m deep. The plateau is ~130-150 m high and moberg-like ridges and cones, and elongated extends from the base of a ridge that is ~350 m high. We depressions and trough-like features interpreted to be interpret the ridge, located along the strike of the linear the result of subglacial and englacial trend, to be a sub-glacial moberg-like ridge, and the phreatomagmatic eruptions. Phreatomagmatic elongate plateau to be a subglacial, sill-like lava flow eruptions could produce enough tephra and country extending from the vent. Superposed on the lobate rock to alter the behavior of the glacier through direct plateau, and extending downslope and out onto the melting, albedo-induced effects, surface insulation, subjacent lava flows, is a sinuous ridge that is generally and influences on the rheology of ice. In some continuous for ~14 km; we interpret this to be an esker places, sufficient meltwater appears to have been draining subglacial eruption-induced meltwater. generated during the intrusion of steep-sided sill-like Adjacent to and downslope from the ridge/lobate plateau subglacial flows to produce subglacial lakes. The the configuration of the drop moraines bows outward for presence of subglacial lakes could have led to local a distance of ~5-10 km. The most prominent drop wet-based conditions, local tongue-like wet based moraine occurs at the distal (downslope) edge of this glacial surges, and to the release of meltwater from inner set of drop moraines and several fluvial channels the margin of the glacier in fluvial drainage channels emerge from its base and extend at least 5-7 km into the or jokulhlaups. In this contribution we examine surrounding terrain. several of these factors from an observational and We interpret this configuration to be the result of modeling point of view. subglacial volcanism and volcanically induced meltwater Arsia Mons Cold-Based Tropical Mountain generation and drainage. Sufficient meltwater appears to Glacier: Subglacial Eruptions, Polythermal have been generated to cause a local transition from Glaciation, and Distal Drainage of Meltwater: At cold-based to wet-based conditions, producing local wet- Arsia Mons, the tropical mountain glacier deposits based surging of a 30-40 km wide portion of the contain features and structures interpreted to otherwise cold-based glacier. In addition, drainage of the represent subglacial and englacial eruptions. Here we meltwater from beneath the glacier out into the describe a series of features that together are surrounding terrain formed local fluvial channels at the interpreted to represent a linear subglacial eruption glacier margin. that caused the production of sufficient meltwater to Subglacial Eruptions and Polythermal Glaciation form eskers, a local wet-based glacial surge that on Mars: The Pavonis Mons Tropical Mountain formed anomalously lobate moraines, and a distal Glacier Steep-Sided Subglacial Flows: Subglacial and series of channels emerging from the edge of the englacial magma in contact with glacial ice can cause glacial deposit and flowing downslope into the melting and produce meltwater. Here we examine the surrounding terrain that is interpreted to represent heating associated with specific features interpreted to be subglacial drainage following the eruption. subglacial eruptions [4,7-8] (Fig. 2) in order to assess A series of NW-trending preglacial lava flows their relative ability to melt glacial ice and to produce extend down the flanks of Arsia and the fan-shaped sufficient meltwater to potentially cause a transition from glacial deposits are superposed. Facies in the NW cold-based to wet-based glacial conditions. We find that part of the Arsia deposit include concentric ridged among the range of subglacial eruption features, steep- deposits interpreted to be drop moraines and sided subglacial lava flows are the most efficient in hummocky deposits interpreted to be sublimation producing meltwater. Due to their sill-like nature and tills. Two generally parallel graben-ridge systems the continuing supply of overlying ice replacing draining trend for several hundred km across the NW part of meltwater, water volumes of up to 450 km3 can be Seventh International Conference on Mars 3123.pdf generated from a typical 100 km long, 15 km wide, sources of sediment include global airborne dust, 500 m thick subglacial flow emplaced at a plausible volcano summit and flank explosive tephra-forming effusion rate of ~10,000 m3/s over a 2.5 year period. eruptions, country rocks from phreatomagmatic This volume of meltwater is equivalent to a layer eruptions, and rocky debris derived from alcoves and averaging 4.5 m deep below an area equivalent to the scarps near the accumulation area. Abundant evidence maximum extent of the Pavonis tropical mountain suggests that the glaciers were cold-based and thus glacier but more importantly is equivalent to an incorporation of subglacial debris into the glacial ice was average water layer thickness of 45 m beneath the minimal. specific zone between the flows and the distal part of Subglacial volcanic eruptions occurring during the the lobe. time of the presence of the glaciers show evidence for This analysis suggests that there may have been dike, sill, subglacial flow, moberg ridge, and cone-like some predictable influences from the generation of activity. Cone-like activity may represent eruptions that this volume of meltwater. First, thermal calculations produce local to regional tephra blankets that could be a show that a transient subglacial lake should form substantial source of glacial debris and serve as agents of down-slope of the advancing lava flow. Shallow direct heating and melting (hot airfall deposits) or lakes would rapidly refreeze, but the volumes albedo-induced melting (blanketing dark tephra). We generated here could lead to additional consequences. model a hypothetical set of cones based on composite For example, volumetrically significant local observations. We locate the cones along a 40 km long subglacial magmatic melting (such as calculated ridge beneath the Tharsis Montes tropical mountain here) could produce sufficient meltwater to cause a glacier ridged facies, interpreted to be drop moraines at local transition from cold-based to wet-based the outer, thinner part of the glacial system. The ridge is conditions, producing local wet-based surging of a interpreted to be the subglacial manifestation of a dike; portion of the otherwise cold-based glacier. the cones are interpreted to represent eruptive centers Evidence for such activity might be manifested in forming along wide places in the dike. We model the anomalous arcuate lobes of moraines downslope of cones as occupying a 6 km long segment of the ridge and the subglacial flows. In addition, drainage of the ranging from 600-1200 m in width, 600-1800 m in meltwater from beneath the glacier out into the length, and 150-280 m in height. Such cones are surrounding terrain could form local fluvial zones interpreted to represent eruptions into a melted cavity in ranging in scale from small channels up to the scale the ice or onto the glacier surface. Widths of such cones of jokulhlaups. Rapid drainage would be consistent are related to the ranges of ejected pyroclasts and imply with the survival of the released water against rapid explosive eruption speeds of ~ 40 m/s and magma water freezing in the low-temperature, low-atmospheric contents of ~0.1 wt %. If they were emplaced from dikes pressure martian environment. releasing magma at 1-10 cubic meters per second per In summary, we find that local sill-like subglacial meter along strike (a common rate on Earth), eruptions can produce sufficient meltwater to cause emplacement times would have been a few hours to 1-2 localized transitions from cold-based to wet-based days. Away from the cones, the ridge is modeled as ~ 60 glacial behavior, and produce related, and perhaps m high and ~250 m wide; here effusion rates would be catastrophic, drainage of meltwater. Studies are much smaller, ~0.004 cubic meters per second per meter underway to assess the relationships between the from a dike ~0.1 m wide. These values and this specific steep-sided
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