Lectures 12-14 Flashcards
Hemispheric Dichotomy
Elevation difference separates the northern lowlands from southern highlands
L-sub-S
Solar longitude. The main way of measuring the time of year on Mars, since the Mars year is longer than an Earth year
Patterned ground
Distinctive geometric patterns caused by freeze-thaw processes. Evidence for ground ice on Mars
Eolian features observed on Mars today
Dust storms, yardangs, dunes, and dust devils
Yardangs
Linear ridges formed by eolian erosion of intervening valleys
Mass Movement
Gravity-driven downhill movement of unconsolidated material.
Large-scale: enlargement canyons, development of chaotic terrain
Small-scale: gullies (aka streak slopes), Recurring Slope Lineae (RSL)
Three main lines of evidence that the SNC meteorites are from Mars
- trapped atmospheric gases
- young crystallization ages
- oxygen isotopes
What is Olympus Mons and where is it?
The largest volcano in the Solar System. Found on Mars in the Tharsis region
Geophysics of Mars
The density of Mars suggests that the core contains significant amounts of sulfur
Rampart craters
Are formed by impact on Mars, where there was ground ice present
Formation model for Valles Marineris
Radial fracturing from the Tharsis uplift, followed by widening due to mass movement