Structural modeling of lobate scarps in the NW margin of Argyre impact basin, Mars

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URI: http://hdl.handle.net/10498/32079
DOI: 10.1016/J.ICARUS.2018.09.027
ISSN: 1090-2643
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2019Department
Física AplicadaSource
Herrero-Gil, A., Egea-González, I., Ruiz, J., & Romeo, I. (2019). Structural modeling of lobate scarps in the NW margin of Argyre impact basin, Mars. Icarus, 319, 367-380. https://doi.org/10.1016/J.ICARUS.2018.09.027Abstract
Martian lobate scarps are prominent tectonic structures interpreted to be the topographic expression of large
thrust faults generated under compression. Here, we present a structural modeling performed on three large
lobate scarps (Ogygis Rupes, Bosporos Rupes and Phrixi Rupes) located in the heavily cratered highlands of
Mars, specifically in Aonia Terra, between Thaumasia Montes and Argyre impact basin. These lobate scarps,
formed in the Late Noachian/Early Hesperian, strike parallel to the edge of the Thaumasia Montes, and were
generated by ESE-vergent thrust faults. Structural analysis of craters deformed by these lobate scarps gives
minimum estimates for the faults slip of ∼1700–3100 m. We applied two structural methods in order to constrain the geometry of these thrust faults at depth, area balanced cross sections and forward mechanical dislocation modeling, obtaining a depth of faulting in this area between ∼18 and ∼45 km, and dip angles between
23° and 35°. These results are consistent with previous studies of lobate scarps on Mars. The depth of faulting
gives an estimation of the depth of the brittle-ductile transition at the time of its formation giving a range of
depth in which the state of the lithosphere change from brittle to ductile-dominated deformation. The heat flow
values calculated from the obtained depths of the brittle–ductile transition range from 25 to 51 mW m−2. We
show that the brittle-ductile transition depth in Aonia Terra is set in 18–27 km at a larger distance from the basin
center, while it is deeper closer to the Argyre rim (∼33–45 km). This difference seems to indicate a thickening of
the brittle domain under Argyre main rim with respect to the external area but, attending to regional geology
and heat flow values calculated, this high value (∼33–45 km) might be an overestimation of the depth of
faulting caused by the presence of the crater rim elevation before the formation of the lobate scarps.
Subjects
Lobate scarp; Mars; Thrust Faults; Depth of faulting; Heat flowCollections
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