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The Geology of Mars

Our knowledge and understanding of the Solar System and its manifold flotsam and jetsam, from specks of dust to our average-sized Sun, has increased to the point that travel by spacecraft and rovers to far-flung lands is not only achievable, it allows us to contemplate our own sojourns – to Mars or back to the Moon. I marvel at the bewildering differences among our planets – the rocky planets and gas giants and their tidally-trapped partners; Io, Enceladus, Titan, the Moon. My own visits to any of these will only ever be imagined. I have never worked on planetary geology. So, the posts that follow will probably be as close as I get.

The red planet has for centuries figured in our imagination. Did Giovanni Schiaparelli anticipate the levels of excitement and speculation when he produced his wonderful map of canali (1888) – features he rendered as channels. Misinterpretation of his term as canals, with its anthropomorphic connotations, whether by omission or commission, let imaginations go wild, creating whole new worlds of ancient Martian civilizations that had structured their existence around complex drainage systems. H.G. Wells made good use of these imaginative scenarios in his War of the Worlds (1898). Orson Welles took these visions to a whole new level of hysteria with his 1938 dramatization that created panic in the unwitting, anger in the duped (especially some broadcasters), and amusement in everyone else.

The new era of Mars science probably began with the Mariner Mission flybys between 1965 and 1971, followed by the Viking 1 and 2 missions that also landed on the surface. These early missions finally gave us imagery and data on which planetary scientists were able to generate sensible hypotheses. Our ideas about Mars evolution – its atmosphere, hydrosphere, and lithosphere have increased in sophistication concomitant with the increasing ingenuity of exploration missions since the mid 1970s. There is now a wealth of information – images, data – and yet the question was there life on Mars remains allusive.

The posts deal primarily with Mars sedimentology and stratigraphy. They are not encyclopedic, but hopefully will serve as a useful introduction

.

Mars sedimentology and stratigraphy

Martian Stratigraphy – The Framework

Stratigraphy of the rocky planets

Evidence for sedimentary rocks on Mars

Mars orbiter and lander missions

A few older posts

Sand dunes but no beach; A Martian breeze

A watery Mars: Canals, a duped radio audience, and geological excursions

Life on Mars; what are we searching for?

Visualizing Mars landscape in 3 dimensions; stunning images from HiRISE

Marsquakes: The InSight experiment

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Categories
dip and strike compass
Measuring dip and strike
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Classification of sandstones
Calcite cemented subarkose, Proterozoic Altyn Fm. southern Alberta
Sandstones in thin section
poles to bedding great circles
Stereographic projection – poles to planes
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Fluid flow: Froude and Reynolds numbers
Stokes Law for particle settling in a schematic context of other fluid flow functions
Fluid flow: Stokes Law and particle settling
sedimentary-basins-distribution-1-768x711
Classification of sedimentary basins
Model are representational descriptions are written in different languages - diagrammatic, descriptive, mathematical, and conceptual. They commonly contain variables and dimensionless quantities that permit quantitative analysis of the physical systems the models represent.
Geological models
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