The Bagnold dune field, Gale crater
A series introducing aeolian processes and deposition, comparing the conditions on Earth and Mars. Mars’ landscaping over the past three […]
A series introducing aeolian processes and deposition, comparing the conditions on Earth and Mars. Mars’ landscaping over the past three […]
An Introduction to aeolian processes and deposition, comparing the conditions on Earth and Mars. Mars current climate is basically a
An Introduction to wind-blown, aeolian deposition, comparing the conditions on Earth, Mars, Venus, and Titan. Modern sand dunes cover extensive
The experiment at the Experimental EarthScape facility focused on evaluating sequence stratigraphic discordances in a scale-independent sedimentary basin model. Key findings included significant stratigraphic surfaces like downlap and onlap, generated during base level changes. The results align well with natural stratigraphic systems, showcasing the importance of base level dynamics in sedimentary processes.
This post discusses an experimental stratigraphic modeling process conducted at Minnesota University’s Experimental EarthScape facility. It highlights the methods, boundary conditions, and variable base levels used to analyze sedimentary systems and stratigraphic responses, building on previous research by Martin et al. and emphasizing the importance of controlling various factors.
This post is part of a series on Mars geology that focuses on sedimentary processes and systems. Why focus on
The rocky planets – Mercury, Venus, Earth (its Moon), and Mars Our knowledge and understanding of the Solar System and
Martian stratigraphy – lessons from the Moon The universality of fundamental laws is firmly embedded in the scientific milieu; viz.
This brief article about Mary Mantell is part of the series Pioneering Women in Earth Sciences – the link will
The rheology of soft sediment and weak rock. This post is part of the Lithofacies Series. See the companion post