Data di Pubblicazione:
2000
Abstract:
One of main objectives of Mars exploration in the 21st century is to search for evidence of present or ancient life. Sedimentary
processes are important on the Martian surface. However, styles of Martian sedimentation can be dierent from its terrestrial counterpart
in some aspects because of the relatively stable Martian crust and the lack of a continuous and active surface hydrological cycle. Certain
types of sedimentary deposits on Earth are closely linked to biological activities, and searching for such deposits on Mars can potentially
enhance the chance of nding life or evidence of ancient life on the planet. A wide range of hypothesized siliciclastic and non-siliciclastic
sedimentary deposits on Mars are of particular interest for the future exobiological exploration. Searching the substrate of sedimentary
deposits is the preferred strategy because it is dicult to preserve organic matter or geochemical evidence of biological activity in the
photochemically active and oxidizing surface environment of Mars.
processes are important on the Martian surface. However, styles of Martian sedimentation can be dierent from its terrestrial counterpart
in some aspects because of the relatively stable Martian crust and the lack of a continuous and active surface hydrological cycle. Certain
types of sedimentary deposits on Earth are closely linked to biological activities, and searching for such deposits on Mars can potentially
enhance the chance of nding life or evidence of ancient life on the planet. A wide range of hypothesized siliciclastic and non-siliciclastic
sedimentary deposits on Mars are of particular interest for the future exobiological exploration. Searching the substrate of sedimentary
deposits is the preferred strategy because it is dicult to preserve organic matter or geochemical evidence of biological activity in the
photochemically active and oxidizing surface environment of Mars.
Tipologia CRIS:
1.1 Articolo in rivista
Elenco autori:
Komatsu, Goro; Ori, Gian Gabriele
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