Present-day Mars is cold and dry, but mineralogical and morphological evidence shows that liquid-water existed on the surface of ancient Mars. In order to explain this evidence and assess ancient Mars

DataCite Commons2023-09-15 更新40

Supporting information for “Late Amazonian ice survival in Kasei Valles, Mars”

火星冰川地貌

行星地质建模

SuppMat: Late Amazonian ice survival in Kasei Valles, MarsContact: adh28@aber.ac.ukThis repository contains the supplementary material associated with Hepburn et al. (2020) Contained within: Table_1_G

Figshare2020-10-29 更新00

Supporting information for_Extensive glaciation in the Erebus Montes region of Mars

火星冰川地貌

行星地质制图

Supporting information for Extensive glaciation in the Erebus Montes region of Mars - shapefiles for craters counts, shapefiles for morphological mapping, and list of datasets used in the study

Figshare2020-11-26 更新40

Distribution and Surface Morphology of Debris-Covered Glaciers and the Latitude Dependent Mantle (LDM) in Phlegra Montes, Mars

火星冰川地貌

行星地表过程

This dataset supports the 2024 study titled "Distribution and Surface Morphology of Debris-Covered Glaciers and the Latitude Dependent Mantle (LDM) in Phlegra Montes, Mars" by C.N. Andres et al. The s

NIAID Data Ecosystem00

Data for: Glacial landscape and paleoglaciation in Terra Sabaea: Evidence for a 3.6 Ga polythermal plateau ice cap.

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