Cratered cones in Southern Cerberus Palus, Mars: Evidence for phreatovolcanism associated with interactions between Amazonian aged lavas and the Medusae Fossae Formation
Abstract
Abundant cratered cones have been identified in Southern Cerberus Palus where young, Cerberus Fossae-derived lavas interact with Medusae Fossae Formation (MFF) materials from Aeolis Planum and Zephyria Planum. These regions contain cones analogous to Icelandic pseudocraters, but the cones display characteristics that differentiate them from others that have been previously described elsewhere on Mars. The cones in this study are found abutting the MFF border, where yardang fleets are embayed by Cerberus lavas, and within flood lavas that overlie MFF deposits west of Zephyria Planum. Rootless cones have formerly been observed in areas of Athabasca Valles, Amazonis Planitia, Elysium Planitia, and Marte Valles. Using HiRISE and CTX imagery from the Mars Reconnaissance Orbiter, Southern Cerberus Palus cones are observed to preferentially form along the tops of partially and fully embayed yardangs. In addition, the cones often form in circular groups atop impact crater rims, and occasionally have large cracks along their flanks. Some cones are also found in linear chains along fissures of obscured origins. Several of these attributes have been noted in previous studies of Martian cratered cones and interpreted as a result of unusual contact geometries with the substrate and a tendency to form at topographic highs, where overburden pressures are minimal (Jaeger et al 2007). Surrounding many cones are areas of light colored, smooth material with lobate margins, below the level of the neighboring rubbly lava. The surface texture of this material is similar to the smooth, polygonally fractured material often found in rifts between Cerberus lava plates, but do not appear to result from tearing in the surrounding lava surface, as they have no preferred size or direction. Due to their overall morphology and distribution, the cones in this study are interpreted to most likely be rootless, hydrovolcanic features formed by explosive interactions between lava flows and H2O present in MFF substrate. The form and quantity of this water is currently unknown; possible hypotheses include sequences of ice deposits, interstitial regolith ice, or possibly hydrated minerals. Spatial distributions of the cones indicate that the conditions required for their formation are not present everywhere the MFF encounters the Cerberus flows.
- Publication:
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AGU Fall Meeting Abstracts
- Pub Date:
- December 2017
- Bibcode:
- 2017AGUFM.P33B2879S
- Keywords:
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- 0450 Hydrothermal systems;
- BIOGEOSCIENCES;
- 5220 Hydrothermal systems and weathering on other planets;
- PLANETARY SCIENCES: ASTROBIOLOGY;
- 5419 Hydrology and fluvial processes;
- PLANETARY SCIENCES: SOLID SURFACE PLANETS;
- 8424 Hydrothermal systems;
- VOLCANOLOGY