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- Publications
- Influence
Primary centers and secondary concentrations of tectonic activity through time in the western hemisphere of Mars
- R. Anderson, J. Dohm, +5 authors B. Peer
- Geology
- 25 September 2001
Five main stages of radial and concentric structures formed around Tharsis from the Noachian through the Amazonian as determined by geologic mapping of 24,452 structures within the stratigraphic… Expand
Astrobiology through the ages of Mars: the study of terrestrial analogues to understand the habitability of Mars.
- A. Fairén, A. Davila, +10 authors C. McKay
- Environmental Science, Medicine
- Astrobiology
- 18 November 2010
Mars has undergone three main climatic stages throughout its geological history, beginning with a water-rich epoch, followed by a cold and semi-arid era, and transitioning into present-day arid and… Expand
Geology of the Thaumasia region, Mars: plateau development, valley origins, and magmatic evolution
Abstract We have constructed the complex geologic history of the Thaumasia region of Mars on the basis of detailed geologic mapping and relative-age dating of rock units and structure. The Thaumasia… Expand
Environmental Studies with the Sensor Web: Principles and Practice
- K. Delin, S. Jackson, +8 authors V. Baker
- Computer Science
- Sensors (Basel, Switzerland)
- 1 February 2005
TLDR
Episodic flood inundations of the northern plains of Mars
- A. G. Fairén, A. G. Fairén, +6 authors R. Anderson
- Geology
- 1 September 2003
Throughout the recorded history of Mars, liquid water has distinctly shaped its landscape, including the prominent circum-Chryse and the
northwestern slope valleys outflow channel systems, and the… Expand
Evidence for Hesperian impact-induced hydrothermalism on Mars
- G. Marzo, A. Davila, +8 authors C. P. McKay
- Geology
- 1 August 2010
Abstract Several hydrated silicate deposits on Mars are observed within craters and are interpreted as excavated Noachian material. Toro crater (71.8°E, 17.0°N), located on the northern edge of the… Expand
Exploration of hydrothermal targets on Mars
- D. Schulze-Makuch, J. Dohm, +5 authors Wolfgang Fink
- Geology
- 1 August 2007
Based on various lines of geologic, geomorphic, topographic, geophysical, spectral, and elemental evidence, we conclude that hydrothermal environments have certainly existed on Mars and are likely to… Expand
Ancient drainage basin of the Tharsis region, Mars: Potential source for outflow channel systems and putative oceans or paleolakes
- J. Dohm, J. Ferris, +8 authors D. H. Scott
- Geology
- 25 December 2001
Paleotopographic reconstructions based on a synthesis of published geologic information and high-resolution topography, including topographic profiles, reveal the potential existence of an enormous… Expand
Evolution of water reservoirs on Mars: Constraints from hydrogen isotopes in martian meteorites
- H. Kurokawa, M. Sato, +4 authors T. Usui
- Geology, Physics
- 17 March 2014
Abstract Martian surface morphology implies that Mars was once warm enough to maintain persistent liquid water on its surface. While the high D/H ratios (∼6 times the Earth's ocean water) of the… Expand