Extensive Hesperian-aged south polar ice sheet on Mars: Evidence for massive melting and retreat, and lateral flow and ponding of meltwater
By James W. Head III, S. Pratt. 2001
184 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atmospheric Science
View Paper: https://www.semanticscholar.org/paper/31eea6fceb8db9ebfbf8f2d8452c478f0768c7ce
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
- R. Wordsworth
- Mark A. Wieczorek
- James W. Head III
- Maria T. Zuber
- G. Neumann
- Francois Forget
- M. Carr
- S. Byrne
In Atmospheric Science
- R. Wordsworth
- Francois Forget
- S. Byrne
- M. Carr
- R. Pierrehumbert
- L. Kerber
- Doris Breuer
- Maria T. Zuber
Citations in the corpus
- Outgassing History and Escape of the Martian Atmosphere and Water Inventory (2015, background): “2001), and the ice deposits sequestered in the Dorsa Argentea Formation (DAF), near the south polar cap, could have represented ∼15 m in the past (Head and Pratt 2001).”
- Geologic history of Mars (2010, background): “, Clifford, 1987, 1993) or one of the major sinks for water emplaced in the northern lowlands during the Noachian and Hesperian (Head and Pratt, 2001).”
- Oceans on Mars: An assessment of the observational evidence and possible fate (2002, background): “Other suggested reservoirs for such water include volatiles in units such as the Hesperian-aged Dorsa Argentea Formation (possibly as much as 20 m GEL) [Head and Pratt, 2001], and as a water/ice component in the Amazonian-aged Medusae Fossae Formation [Head, 2001], whose total volume is $1.4 Â 10 6 ”
- Crustal structure of Mars from gravity and topography (2004, background): “[38] The southern layered terrains grade downhill, merging into the surrounding cratered highlands, but appear to have been emplaced on a 1–2 km high plain marked by Schmidt Valley, Prometheus Basin, and the Dorsa Argentia formation [Head and Pratt, 2001; Fishbaugh and Head, 2001].”
- The Polar Deposits of Mars (2009, background): “Analysis of MGS imaging and topography data suggests that this deposit may be the devolatilized remnant of an ancient polar ice sheet (Head & Pratt 2001).”
- Comparison of “warm and wet” and “cold and icy” scenarios for early Mars in a 3‐D climate model (2015, background): “[2013], and may be linked to the late Noachian to early Hesperian era Dorsa Argentea Formation [Head and Pratt, 2001; Kress and Head, 2015].”