Evidence for recent groundwater seepage and surface runoff on Mars.
By Michael C. Malin, K. Edgett. Science, 2000
1,060 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atmospheric Science, Soil Science
View Paper: https://www.semanticscholar.org/paper/3fb45e6845ab43478058523f9e3d4bb897886106
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
- Michael D. Smith
- S. Byrne
- A. S. McEwen
- Michael J. Wolff
- Nicolas Gonzalez Thomas
- Hirise Team
- B. Cantor
- R. Haberle
In Atmospheric Science
- A. S. McEwen
- Nicolas Gonzalez Thomas
- Hirise Team
- S. Byrne
- M. Hecht
- Alan D. Howard
- Michael J. Wolff
- R. Craddock
In Soil Science
- A. S. McEwen
- Nicolas Gonzalez Thomas
- Hirise Team
- S. Byrne
- M. Hecht
- Alan D. Howard
- K. Edgett
- Michael C. Malin
Citations in the corpus
- Granular and particle-laden flows: from laboratory experiments to field observations (2017, background): “This has strong implication for planetary science and in particular on Mars (e.g. Mangold et al 2003, 2010) where the levee-channel landslide morphologies were first interpreted as indicating the presence of water during emplacement (Malin and Edgett 2000).”
- Hydrogen in the Deep Earth (2001, background): “A backdrop to these terrestrial issues is the evidence of significant water abundances elsewhere in the solar system, including polar caps and channels on Mars as well as the recent observational evidence of large subsurface quantities of water on Mars (Malin & Edgett 2000, Zuber et al 2000).”
- Planetary habitability: lessons learned from terrestrial analogues (2014, neutral): “Evidence of past water action is present as landforms that look like artefacts of fl uvial action (e.g. Malin & Edgett 2000) and to some extent even mineral deposits that require water for their formation.”
- Have olivine, will gas: Serpentinization and the abiogenic production of methane on Mars (2005, background): “Additionally, rock stratification would permit lateral movement of H2O or melted permafrost from its source manifesting as liquid flows at cliff faces [Malin and Edgett, 2000].”
- A chronology of early Mars climatic evolution from impact crater degradation (2012, background): “…networks are present mainly to the east of the area, e.g., Loire Vallis and Samara Vallis, but valleys also exist in the western area, sometimes with depositional fans, for example, in and around Holden and Eberswalde craters [Grant et al., 2008; Malin and Edgett, 2003; Pondrelli et al., 2008].”
- Modelling the surface and subsurface Martian radiation environment: Implications for astrobiology (2007, background): “Intriguingly, the gullies and seeps seen at high latitude suggest the recent transient presence of liquid water [Malin and Edgett, 2000].”