The early martian evolution—Constraints from basin formation ages
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The presence of these carbonates in Huygens rim rocks suggests that they predate Huygens itself, an Early Noachian basin dated to ~3.98 Ga.
“Indeed, the presence of these carbonates in Huygens rim rocks suggests that they predate Huygens itself, an Early Noachian basin dated to ~3.98 Ga [Werner, 2008]”
From Orbital evidence for more widespread carbonate-bearing rocks on Mars (2016) · cites this paper as Werner, 2008
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- Authors
- Werner, S. C.
- Affiliations
- Geological Survey of Norway (NO)
- Corresponding author
- Werner, S.C.
- ORCID
- Werner, S.C.
- Venue
- Icarus
- Publisher
- Elsevier BV
- Published
- 2008-05
- Volume
- 195
- Issue
- 1
- Pages
- 45-60
- ISSN
- 0019-1035 (ISSN-L)
- OpenAlex
- W2042371405
- Cited by
- 185
- References
- 45
- Citations by year
- 2026: 10 · 2025: 13 · 2024: 7 · 2023: 9 · 2022: 16 · 2021: 12 · 2020: 11 · 2019: 16 · 2018: 12 · 2017: 10 · 2016: 8 · 2015: 8 · 2014: 10 · 2013: 8 · 2012: 16
- FWCI
- 3.69
- Type
- journal article
- Language
- en
- Open access
- closed
- Licence
- Locations
- Icarus (publishedVersion)
- Funders
- Deutsche Forschungsgemeinschaft
- 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 › Geophysics › Geological and Geochemical Analysis
- Keywords
- early Mars, Hellas basin, Isidis basin, Argyre basin, heavy bombardment, crustal thickness, impactor population
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