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Journal ArticleDOI

The Global Topography of Mars and Implications for Surface Evolution

TLDR
Elevations measured by the Mars Orbiter Laser Altimeter have yielded a high-accuracy global map of the topography of Mars, which includes the low northern hemisphere, the Tharsis province, and the Hellas impact basin.
Abstract
Elevations measured by the Mars Orbiter Laser Altimeter have yielded a high-accuracy global map of the topography of Mars. Dominant features include the low northern hemisphere, the Tharsis province, and the Hellas impact basin. The northern hemisphere depression is primarily a long-wavelength effect that has been shaped by an internal mechanism. The topography of Tharsis consists of two broad rises. Material excavated from Hellas contributes to the high elevation of the southern hemisphere and to the scarp along the hemispheric boundary. The present topography has three major drainage centers, with the northern lowlands being the largest. The two polar cap volumes yield an upper limit of the present surface water inventory of 3.2 to 4.7 million cubic kilometers.

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Book ChapterDOI

Composition of the Continental Crust

TL;DR: In this paper, the present-day composition of the continental crust, the methods employed to derive these estimates, and the implications of continental crust composition for the formation of the continents, Earth differentiation, and its geochemical inventories are discussed.
Journal ArticleDOI

The Generic Mapping Tools Version 6

TL;DR: GMT 6 defaults to classic mode and thus is a recommended upgrade for all GMT 5 users, and new users should take advantage of modern mode to make shorter scripts, quickly access commonly used global data sets, and take full advantage of the new tools to draw subplots, place insets, and create animations.

Water on Mars

TL;DR: In this paper, the amount of water outgassed from Mars by impact erosion and hydrodynamic escape is estimated to be between 6 to 160 m. The two sets of estimates may be reconciled if early in its history, Mars lost part of its atmosphere.
References
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Water on Mars

TL;DR: In this paper, the amount of water outgassed from Mars by impact erosion and hydrodynamic escape is estimated to be between 6 to 160 m. The two sets of estimates may be reconciled if early in its history, Mars lost part of its atmosphere.
Journal ArticleDOI

A model for the hydrologic and climatic behavior of water on Mars

TL;DR: In this paper, an analysis of the hydrologic response of a water-rich Mars to climate change and to the physical and thermal evolution of its crust is carried out, with particular attention given to the potential role of the subsurface transport, assuming that the current models of insolation-driven change describe reasonably the atmospheric leg of the planet's long-term hydrological cycle.
Journal ArticleDOI

Ancient oceans, ice sheets and the hydrological cycle on Mars

TL;DR: The formation of valley networks early in Mars' history is evidence for a long-term hydrological cycle, which may have been associated with the existence of a persistent ocean as mentioned in this paper.
Journal ArticleDOI

The Mars Observer laser altimeter investigation

TL;DR: The Mars Observer laser altimeter (MOLA) was used to determine globally the topography of Mars at a level suitable for addressing problems in geology and geophysics as mentioned in this paper.
Book

The Surface of Mars

TL;DR: In this article, a systematic summary of what we have learnt about the geological evolution of Mars as a result of these missions is presented, including the diverse Martian surface features and summarizes current ideas as to how, when and under what conditions they formed, and explores how Earth and Mars differ and why the two planets evolved so differently.
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