Provenance and diagenesis of the evaporite-bearing Burns formation, Meridiani Planum, Mars

@article{McLennan2005ProvenanceAD,
  title={Provenance and diagenesis of the evaporite-bearing Burns formation, Meridiani Planum, Mars},
  author={Scott M. McLennan and James F. Bell and Wendy M. Calvin and Philip R. Christensen and Benton C. Clark and Paulo A. de Souza and Jack D. Farmer and William H. Farrand and David A. Fike and Ralf Gellert and A. Ghosh and Timothy D. Glotch and John P. Grotzinger and Brian C. Hahn and Kenneth E. Herkenhoff and Joel A. Hurowitz and Jeffrey R. Johnson and Sarah Stewart Johnson and Bradley L. Jolliff and G{\"o}star Klingelh{\"o}fer and Andrew H. Knoll and Z. A. Learner and Michael C. Malin and Harry Y. McSween and J. M. Pocock and Steven W. Ruff and Laurence A. Soderblom and Steven W. Squyres and Nicholas J. Tosca and Wesley Andr{\'e}s Watters and Michael Bruce Wyatt and Albert S. Yen},
  journal={Earth and Planetary Science Letters},
  year={2005},
  volume={240},
  pages={95-121}
}

Elemental Geochemistry of Sedimentary Rocks at Yellowknife Bay, Gale Crater, Mars

The absence of predicted geochemical variations indicates that magnetite and phyllosilicates formed by diagenesis under low-temperature, circumneutral pH, rock-dominated aqueous conditions during the early history of Mars.

Evidence for Water at Meridiani

The Mars Exploration Rover Opportunity has examined sedimentary structures in the Burns formation at Meridiani Planum. The materials in this formation reflect, in part, subaqueous deposition of
...

References

SHOWING 1-10 OF 76 REFERENCES

Dissolution-collapse breccias and paleokarst resulting from dissolution of evaporite rocks, especially sulfates

The lithological trinity of dolostone, limestone, and sulfates (anhydrite and/or gypsum) is subject to rapid dissolution of the sulfates and leads to the development of dissolution-collapse breccias

Geologic setting and origin of Terra Meridiani hematite deposit on Mars

[1] We have completed a regional analysis of the hematite deposit in Terra Meridiani and conclude that the unit is in the midst of a 600-m-thick stack of friable layered materials superposed on

Early Post-Depositional Modification of Aeolian Dune Sands

  • K. Pye
  • Geology, Environmental Science
  • 1983

Petrography and geochemistry of feldspathic and mafic sediments of the northeastern Pacific margin

  • P. KampB. Leake
  • Geology
    Transactions of the Royal Society of Edinburgh: Earth Sciences
  • 1985
ABSTRACT This study attempts to ascertain whether the differing provenance sources and plate tectonic settings of deposition of clastic sediments and rocks can be identified by chemical means, thus

Formation of the hematite-bearing unit in Meridiani Planum: Evidence for deposition in standing water

[1] The most plausible models for the origin and evolution of a unique geologic unit in Meridiani Planum, Mars, are low-temperature precipitation of Fe oxides/oxyhydroxides from standing water,

Deposition and early alteration of evaporites

The depositional settings for primary and early diagenetic evaporite deposits generally fall into three categories: marginal (mixed shallow‐subaqueous and subaerial), shallow and deep subaqueous.

In Situ Evidence for an Ancient Aqueous Environment at Meridiani Planum, Mars

The geologic record at Meridiani Planum suggests that conditions were suitable for biological activity for a period of time in martian history.

Diagenetically Enhanced Bedding in Argillaceous Platform Limestones: Stratified Cementation and Selective Compaction

A field and petrographic study has been made of 34 massive beds in argillaceous limestones of open marine platform facies in the U.K. Lithologies include grainstones, packstones, wackestones and lime
...