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Geologic map of the eastern equatorial region of Mars

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The article was published on 1987-01-01 and is currently open access. It has received 497 citations till now. The article focuses on the topics: Mars Exploration Program & Geologic map.

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Orbital Identification of Carbonate-Bearing Rocks on Mars

TL;DR: The presence of carbonate as well as accompanying clays suggests that waters were neutral to alkaline at the time of its formation and that acidic weathering, proposed to be characteristic of Hesperian Mars, did not destroy these carbonates and thus did not dominate all aqueous environments.
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The Evolution of the Martian Hydrosphere: Implications for the Fate of a Primordial Ocean and the Current State of the Northern Plains

TL;DR: In this article, the authors consider the hydraulic and thermal conditions that gave rise to the elevated source regions of the Late Hesperian outflow channels and explore their implications for the evolution of the Martian hydrosphere.
References
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ReportDOI

Geologic map of the western equatorial region of mars

TL;DR: Lowland terrains as mentioned in this paper consist of all plains-forming units between the highland-lowland boundary scarp and the north edge of the map area, exclusive of materials of the western volcanic assemblage on the Tharsis swell.
Journal ArticleDOI

Thermal and albedo mapping of Mars during the Viking primary mission

TL;DR: The behavior of Mars as observed by the Viking infrared thermal mapper (IRTM) is considered in this article, where the IRTM is a 28-channel, 4-telescope radiometer that operated in six spectral bands.
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Mars: Fretted and chaotic terrains

TL;DR: Fretted and chaotic terrains are members of a larger family of lowland terrains on the Martian surface as discussed by the authors, characterized by extensive, smooth, lowland plains separated from the old cratered upland by an abrupt escarpment of highly irregular planimetric configuration.
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Preliminary mariner 9 report on the geology of Mars

TL;DR: In this article, the equatorial region between 30 deg N and 30 deg S latitude is depicted in four geologic sketch maps, and seventeen geologic units are defined on the basis of their textural characteristics.
Journal ArticleDOI

The martian hemispheric dichotomy may be due to a giant impact

TL;DR: In this article, the authors proposed that the large expanse of lowlands of Mars is substantially due to the formation of a large impact basin early in the planet's history, which has markedly influenced the character of the Martian surface.
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