PG_logo Bridge to Mars:
Planetary Geophysics Group

Colorado School of Mines
Department of Geophysics
Jeff Andrews-Hanna
Assistant Professor
Dept of Geophysics
Green Center, Rm 280K

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I use of a combination of numerical modeling, analysis of gravity and topography, and geomorphology to understand the interaction of a variety of processes responsible for shaping the surfaces and interiors of Mars and the terrestrial planets. I’m particularly interested in the interaction of geodynamic, tectonic, volcanic, climatic, and hydrologic processes at a variety of scales. Much of my research is focused in two main areas: processes involving liquid water on and beneath the surface of Mars, and the tectonic and geodynamic evolution of Mars.

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A brief discussion of some of my individual research projects follows.

**click on the images for more information on individual projects
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dichotomy Martian hemispheric dichotomy: I am investigating the possibility that the dichotomy between the southern highlands and northern lowlands may have been the result of a giant impact.
strikeslip Strike-slip faults on Mars: I have mapped a new population of ancient strike-slip faults on Mars and used them to shed light on the thermal and tectonic evolution of the planet.
Meridiani Meridiani Planum: The MER Opportunity rover has found evidence for evaporites at Meridiani. I am using global scale hydrological models to understand the origin of these deposits and their implications for the history of water and climate on Mars.
South Pole Mars south polar cap density: I am using a combination of MOLA topography, gravity data from the MRO spacecraft, and radar sounding from MARSIS to calculate the density of the south polar layered deposits on Mars.
Hellas Giant impact basins: The surfaces of Mars and the Moon are marred by several giant impact basins, including Hellas, Utopia, and the South Pole-Aitken basin. I am trying to understand why these basins appear the way they do.
chaos Martian outflow channel floods: Many of the martian outflow channels originate in regions of disrupted ground called "chaos regions". I have used numerical modeling to show that these floods would likely have been periodic.
Mangala Earthquake-triggered floods on Mars: Several Martian outflow channels originate within tectonic features (including Mangala and Athabasca Valles). I have demonstrated that the tectonism itself could have pressurized the aquifers and directly caused the flooding.
graph Climate change and hydrology: It has been suggested that dramatic changes in the Martian climate could have triggered the outflow channel floods. In modeling this process I have found that the required pore pressures and flood volumes could not likely be produced by this mechanism alone.

Publications and Presentations

Peer-reviewed

Presentations and abstracts