Cited by 160Planetary Science and ExplorationAstro and Planetary ScienceGeochemistry and Elemental Analysis

Juvenile chemical sediments and the long term persistence of water at the surface of Mars

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Tosca, Nicholas J., Knoll, Andrew H.·2009·Earth and Planetary Science Letters

Integrity signals

Registry

Crossref · 10.1016/j.epsl.2009.07.004

Cites

4 of 4 references verified0 citation errors · 0 not checkable

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  • Global analysis of aqueous alteration products on the Martian surface suggests a predominance of juvenile or weakly modified minerals.

    “Indeed, global analysis of aqueous alteration products on the Martian surface suggests a predominance of juvenile or weakly modified minerals (Tosca & Knoll 2009).”

    From The Climate of Early Mars (2016) · cites this paper as Tosca & Knoll 2009

  • The flows responsible for eroding the late Noachian and Hesperian surface were relatively short-lived.

    “This suggests that the flows responsible for eroding the late Noachian and Hesperian surface were relatively short-lived.”

    From The Climate of Early Mars (2016) · cites this paper as Tosca & Knoll 2009

  • A successful theory for surface warming must yield valley network erosion rates consistent with the geologic evidence but avoid extensive surface carbonate formation and aqueous alteration of sediments.

    “A successful theory for surface warming must yield valley network erosion rates consistent with the geologic evidence (Hoke, Hynek & Tucker 2011) but avoid extensive surface carbonate formation and aqueous alteration of sediments (Tosca & Knoll 2009; Ehlmann et al. 2011).”

    From The Climate of Early Mars (2016) · cites this paper as Tosca & Knoll 2009

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Authors
Tosca, N. J., & Knoll, A. H.
Affiliations
Harvard University (US)
Corresponding author
Tosca, Nicholas J.
Venue
Earth and Planetary Science Letters
Publisher
Elsevier BV
Published
2009-09
Volume
286
Issue
3-4
Pages
379-386
ISSN
0012-821X (ISSN-L)
OpenAlex
W2012354505
Cited by
160
References
4
Citations by year
2026: 7 · 2025: 7 · 2024: 11 · 2023: 4 · 2022: 6 · 2021: 11 · 2020: 15 · 2019: 10 · 2018: 8 · 2017: 11 · 2016: 7 · 2015: 8 · 2014: 8 · 2013: 12 · 2012: 17
FWCI
5.88
Type
journal article
Language
en
Open access
Locations
  • Earth and Planetary Science Letters (publishedVersion)
  • Department of Earth Sciences EPrints Repository (acceptedVersion)
  • Digital Access to Scholarship at Harvard (DASH) (Harvard University) (submittedVersion, cc-by)
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 › Geochemistry and Petrology › Geochemistry and Elemental Analysis
Keywords
Mars, aqueous alteration, chemical sediments, diagenesis, smectite, iron sulfate, volcanic rock, valley formation, habitability

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Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.

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