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Martian Volcanism
Ian Marrs
Our Future
Where do we go?
Comparison
A Wandering Companion
A Wandering Companion
Moons
• Phobos
• Diameter
• 22.2 km
• 13.8 mi
• Mass
• 1.08*10^16 kg
• Deimos
• Diameter
• 12.6 km
• 7.8 mi
• Mass
• 2*10^15 kg
Moons
Moons
• Deimos
• Phobos
• Our moon
Moons
Impact
Impact
Impact
History
Core Hypothesis
The Martian Dichotomy
Ancient Oceans
Where are we?
Gusev crater
Gusev crater TAS
TAS comparison
Titanium
Potassium
Indicative elements
• Manganese
• Nickel
Meteorite Hand Sample
Shergotty thin
section
• Pigeonite
• Pig
• Glass
• mk
Y000749
Hypothesized
cooling
Valles Marineris
• One of the largest canyons in the
solar system
• 4000 km long
• 200 km wide
• 7 km deep
Valley v. United States
Olympus Mons
• Shield Volcano
• Basaltic lava
• Similar to Hawaiian Islands
Olympus Mons
Meteor thin sections
• B
• Adjacent olivine and pyroxene recrystallized in
a melt pocket
• C
• Opaque melt engulfing phosphate grains
• D
• Shock melt pocket
Meteor thin
sections
• A
• Deformed pyroxene
• B
• Deformed olivine
• D
• Melt pocket of olivine
• F
• Brecciation in ALH84001
Robotics
Pollution
Protection
The Future of
Exploration
Inspiration
References
Bertaux, J.-L., Leblanc, F., Witasse, O., Quemerais, E., Lilensten, J., Stern, S.A., Sandel, B., and Korablev, O., 2005, Discovery of an aurora on Mars:
Nature, v. 435, p. 790–794, doi: 10.1038/nature03603.
Bridges, J., and Warren, P., 2006, The SNC meteorites: basaltic igneous processes on Mars: Journal of the Geological Society, v. 163, p. 229–251, doi:
10.1144/0016-764904-501.
Carr, M.H., and Head, J.W., 2005, Geologic history of Mars: Earth and Planetary Science Letters, p. 185–203, doi: 10.1016/j.epsl.2009.06.042.
Fritz, Jӧrg, et al. “Ejection of Martian Meteorites.” Meteoritics & Planetary Science, vol. 40, no. 9-10, 2005, pp. 1393–1411., doi:10.1111/j.1945-
5100.2005.tb00409.x.
Leone, G., Tackley, P.J., Gerya, T.V., May, D.A., and Zhu, G., 2014, Three-dimensional simulations of the southern polar giant impact hypothesis for
the origin of the Martian dichotomy: Geophysical Research Letters, v. 41, p. 8736–8743, doi: 10.1002/2014gl062261.
Mcsween, H. Y. “Basaltic Rocks Analyzed by the Spirit Rover in Gusev Crater.” Science, vol. 305, no. 5685, 2004, pp. 842–845.,
doi:10.1126/science.1099851.
Mcsween, H. Y., et al. “Elemental Composition of the Martian Crust.” Science, vol. 324, no. 5928, 2009, pp. 736–739., doi:10.1126/science.1165871.
Solomon, S.C., Head, J.W., 2007. If the late heavy bombardment on the Moon was a terminal cataclysm, what are some implications for Mars? Lunar
Planet. Sci. 38, 1636 abstract.
Voosen, P., 2018, By listening for quakes on Mars, NASA lander will probe Red Planet’s interior: Science, doi: 10.1126/science.aat9232.
Yant*, Marcella, et al. “Visible, near-Infrared, and Mid-Infrared Spectral Characterization of Hawaiian Fumarolic Alteration near Kilauea's December
1974 Flow: Implications for Spectral Discrimination of Alteration Environments on Mars.” American Mineralogist, vol. 103, no. 1, 2018, pp. 11–25.,
doi:10.2138/am-2018-6116.

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Martian volcanism