Updated global map of Martian valley networks and implications for climate and hydrologic processes
By B. Hynek, M. Beach, M. Hoke. 2010
414 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atmospheric Science
View Paper: https://www.semanticscholar.org/paper/7bbcb01e49b756d6e84c01c93a2f87daf6907107
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
- E. Kite
- R. Wordsworth
- James W. Head III
- Ernst Hauber
- B. Hynek
- Caleb I. Fassett
- Harald Hiesinger
- Greg Michael
In Atmospheric Science
- E. Kite
- Ernst Hauber
- R. Wordsworth
- Caleb I. Fassett
- James W. Head III
- Greg Michael
- B. Hynek
- D. Loizeau
Citations in the corpus
- Formation timescales of large Martian valley networks (2011, background): “…Noachian and Early Hesperian (~3.5–3.8 Ga) (Fassett and Head, 2008b; Hoke and Hynek, 2009), consistent with their formation during a period of enhanced fluvial erosion and incision on Mars (e.g. Craddock and Howard, 2002; Howard et al., 2005; Hynek and Phillips, 2001, 2003; Hynek et al., 2010).”
- Sequence and timing of conditions on early Mars (2011, background): “The characteristics of valley networks thus seem to require, at minimum, time periods when precipitation on the surface was possible, water was cycled through the early Mars atmosphere, and water was stable or metastable at the martian surface (Craddock and Howard, 2002; Hynek et al., 2010).”
- The geological and climatological case for a warmer and wetter early Mars (2018, neutral): “International Journal of Climatology, 26(15), 2181-2198 (2006).”
- The High Resolution Stereo Camera (HRSC) of Mars Express and its approach to science analysis and mapping for Mars and its satellites (2016, background): “This appears relatively low in comparison to the highest Strahler order (i.e. 7) found by Hynek et al. (2010) from a combination of MOLA and IR THEMIS data.”
- Transient reducing greenhouse warming on early Mars (2016, positive): “This evidence includes dendritic valley networks distributed over large regions of the equatorial and southern Noachian highlands, fluvial conglomerates, open-basin lakes, and fluvolacustrine deposits [ Fassett and Head , 2008a; Hynek et al. , 2010; Grotzinger et al. , 2015].”
- Geologic Constraints on Early Mars Climate (2018, methodology): “Most large gaps in the latitude-longitude distribution of valley networks in THEMIS and MOLA databases (Hynek et al. 2010, Luo et al. 2017) correspond to post-fluvial resurfacing (i.e., Amazonian lava or Amazonian ice-rich mantling deposits).”