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N. A. Cabrol

Researcher at Ames Research Center

Publications -  32
Citations -  4570

N. A. Cabrol is an academic researcher from Ames Research Center. The author has contributed to research in topics: Mars Exploration Program & Impact crater. The author has an hindex of 18, co-authored 21 publications receiving 4293 citations. Previous affiliations of N. A. Cabrol include Search for extraterrestrial intelligence.

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Overview of the Spirit Mars Exploration Rover Mission to Gusev Crater: Landing site to Backstay Rock in the Columbia Hills

Raymond E. Arvidson, +62 more
TL;DR: In this paper, the authors show that the surface enrichment is the result of a minor amount of transport and deposition by aqueous processes on the surface of olivine-bearing basalts.
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The Opportunity Rover's Athena science investigation at Meridiani Planum, Mars.

Steven W. Squyres, +49 more
- 03 Dec 2004 - 
TL;DR: The Mars Exploration Rover Opportunity has investigated the landing site in Eagle crater and the nearby plains within Meridiani Planum, and the rocks are interpreted to be a mixture of chemical and siliciclastic sediments formed by episodic inundation by shallow surface water, followed by evaporation, exposure, and desiccation.
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The Spirit Rover's Athena Science Investigation at Gusev Crater, Mars

Steven W. Squyres, +49 more
- 06 Aug 2004 - 
TL;DR: The Mars Exploration Rover Spirit and its Athena science payload have been used to investigate a landing site in Gusev crater, but no clear evidence for lacustrine sedimentation has been found to date as discussed by the authors.
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Distribution, Classification, and Ages of Martian Impact Crater Lakes

TL;DR: Paleolakes in impact craters on Mars were characterized at global scale using the Viking Orbiter data as discussed by the authors, and 179 paleolakes were identified in impact structures formed by the influx of water and sediment derived from valley networks and channels that can be classified into three different fluviolacustrine systems: closed, open and lake-chain systems.
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On the possibility of liquid water on present‐day Mars

TL;DR: In this article, a validated general circulation model was used to determine where and for how long the surface pressure and surface temperature on Mars meet the minimum requirements for the existence of liquid water in the present climate system: pressures and temperatures above the triple point of water but below the boiling point.