401 比較惑星河川学V(セッション4)

概要

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The objective of this study is to examine whether Martian valley networks are formed by fluvial valleys as has been widely accepted so far. Although morphology of the Martian valley networks is similar to that of terrestrial valley networks, it does not necessarily mean that the Martian valley networks are landforms eroded by liquid-water flow. The landforms eroded by flows driven by gravity are controlled by viscosity of fluid, gravity, discharge of the flow, inclination, and others. In this study, we will attempt to assess what parameter is the most important for fluvial landforms on the Earth.
日本惑星科学会の論文
1995-11-13