Data di Pubblicazione:
2021
Abstract:
Chaotic terrains are broad regions on Mars characterized by the disruption of the basaltic
bedrock into polygonal blocks separated by deep fractures. To date, the proposed genetic scenarios often
involve the occurrence of subsurface ice or liquid H2O. Nevertheless, similar features also occur within
some craters on the Moon, namely floor-fractured craters (FFCs), where water ice reservoirs are not
present. We propose a new formation mechanism for Martian chaotic terrains as well as for lunar and
Martian FFCs. The proposed mechanism does not require a major role of water but multiple cycles of
inflation and deflation of a buried magma chamber. This process results in a particular type of caldera
collapse, called the piecemeal (or chaotic) caldera collapse. A series of analog experiments show both
geometrical and quantitative correspondence with natural case studies: Arsinoes Chaos (Mars), an
unnamed FFC (Mars), and Komarov crater (FFC on the Moon).
Tipologia CRIS:
01.01 Articolo in rivista
Keywords:
Craters; Moon; Mars
Elenco autori:
Maestrelli, Daniele; Corti, Giacomo
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