Ancient ocean on Mars supported by global distribution of deltas and valleys
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The quantity of surface water sufficient to fill a northern ocean to the di Achille & Hynek (2010) shoreline implies a GEL of around 550 m.
“The quantity of surface water sufficient to fill a northern ocean to the di Achille & Hynek (2010) shoreline implies a GEL of around 550 m, so in the immediate post-warm-and-wet phase these ice sheets could be several kilometers thick.”
From The Climate of Early Mars (2016) · cites this paper as di Achille & Hynek 2010
Even with a northern ocean at the di Achille & Hynek (2010) shoreline, Mars would possess a far higher land to ocean ratio than Earth does, making the physics of a snowball transition quite different.
“Even with a northern ocean at the di Achille & Hynek (2010) shoreline, Mars would possess a far higher land to ocean ratio than Earth does, making the physics of a snowball transition quite different.”
From The Climate of Early Mars (2016) · cites this paper as di Achille & Hynek 2010
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“Even with a northern ocean at the di Achille & Hynek (2010) shoreline, Mars would possess a far higher land to ocean ratio than Earth does, making the physics of a snowball transition quite different.”
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- Authors
- Di Achille, G., & Hynek, B. M.
- Affiliations
- University of Colorado Boulder (US)
- ORCID
- Hynek, Brian M.
- Venue
- Nature Geoscience
- Published
- 2010-06-13
- Volume
- 3
- Issue
- 7
- Pages
- 459-463
- ISSN
- 1752-0894 (ISSN-L)
- 1752-0908
- OpenAlex
- W2023934786
- Cited by
- 417
- References
- 33
- Citations by year
- 2026: 28 · 2025: 25 · 2024: 26 · 2023: 32 · 2022: 46 · 2021: 39 · 2020: 30 · 2019: 20 · 2018: 38 · 2017: 21 · 2016: 28 · 2015: 14 · 2014: 15 · 2013: 11 · 2012: 19
- FWCI
- 16.61
- Type
- journal article
- Language
- en
- Open access
- closed
- Licence
- www.springer.com/tdm (tdm)
- Locations
- Nature Geoscience (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Planetary Science and Exploration
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
- Physical Sciences › Earth and Planetary Sciences › Earth-Surface Processes › Geological formations and processes
- Keywords
- early Mars climate, valley networks, equipotential surfaces, northern lowlands, paleoshorelines, Mars topography, hydrological systems
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