Morphologic, stratigraphic and morphometric investigations of valley networks in eastern Libya Montes, Mars: Implications for the Noachian/Hesperian climate change

Abstract

“Dendritic valley networks” and broad “longitudinal valleys” are widespread within the eastern Libya Montes region. The morphologic characteristics of the studied dendritic valleys, especially their occurrence at local summits, provide evidence for the initial formation by surface runoff due to atmospheric precipitation whereas the longitudinal valley systems are thought to have been formed and modified by groundwater-induced processes. Our crater counts and model ages show, that the dendritic valley networks (average age ∼ 4.0 Ga) formed earlier than the longitudinal valley systems (average age ∼ 3.7 Ga). Both fluvial forms indicate a temporal change of the erosive environment at the Noachian/Hesperian transition at ∼ 3.8 Ga. Our results suggest that the fluvial activity within our investigation area lasted for ∼ 800 My, from ∼ 4.1 Ga to ∼ 3.3 Ga. The dendritic valleys show valley densities between 0.12 km − 1 and 0.57 km − 1 , indicative of highly mature and integrated valley systems that we interpret to be characteristic of warmer and wetter conditions on Mars.