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Restio vallis-simius

Known as: Restio vallis simius 
 
National Institutes of Health

Papers overview

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2020
2020
Mawrth Vallis, Mars: A Fascinating Place for Future In Situ Exploration.
After the successful landing of the Mars Science Laboratory rover, both NASA and ESA initiated a selection process for potential… Expand
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2019
2019
Discovery of recurring slope lineae candidates in Mawrth Vallis, Mars
Several interpretations of recurring slope lineae (RSL) have related RSL to the potential presence of transient liquid water on… Expand
Highly Cited
2013
Highly Cited
2013
What the ancient phyllosilicates at Mawrth Vallis can tell us about possible habitability on early Mars
Abstract Phyllosilicate deposits on Mars provide an opportunity to evaluate aqueous activity and the possibility that habitable… Expand
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2013
2013
3D Reconstruction of the Source and Scale of Buried Young Flood Channels on Mars
Seeing Below the Surface Marte Vallis represents the largest of the young outflow channels on Mars. Thought to be the result of… Expand
Highly Cited
2008
Highly Cited
2008
Columbia Hills, Mars: Aeolian features seen from the ground and orbit
[1] Abundant wind-related features occur along Spirit's traverse into the Columbia Hills over the basaltic plains of Gusev Crater… Expand
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2007
2007
THE LIGHT-TONED SEDIMENTS IN AND NEAR LOWER MAWRTH VALLIS MAY BE A DRAPE
Introduction: Marwth Vallis and the phyllosilicaterich deposits in and near its lower terminus constitute one of the most… Expand
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Highly Cited
2005
Highly Cited
2005
Groundwater‐controlled valley networks and the decline of surface runoff on early Mars
[1] Fluvial erosion on early Mars was dominated by valley networks created through a combination of groundwater processes and… Expand
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Highly Cited
2004
Highly Cited
2004
Geomorphology of Ma'adim Vallis, Mars, and associated paleolake basins
[1] Ma'adim Vallis, one of the largest valleys in the Martian highlands, appears to have originated by catastrophic overflow of a… Expand
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2004
2004
Geomorphology and Hydraulics of Ma'adim Vallis, Mars, During a Noachian/Hesperian Boundary Paleoflood
HESPERIAN BOUNDARY PALEOFLOOD. R. P. Irwin III, A. D. Howard, and T. A. Maxwell, Center for Earth and Planetary Studies, National… Expand
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2001
2001
Eruption Constraints for a Young Channelized Lava Flow, Marte Vallis, Mars
This study constrains flow rates for a specific channelized lava flow in Marte Vallis, Mars. We measured slope-gradient, channel… Expand
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