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STRATI 2013 pp 337-341 | Cite as

Stratigraphic Analysis of the Depositional Sequence in Danielson Crater, Mars

  • Alessio MuranaEmail author
  • Thomas Kneissl
Conference paper
Part of the Springer Geology book series (SPRINGERGEOL)

Abstract

Danielson Crater is a complex impact structure with a diameter of about 60 km and is located between North Sinus Meridiani and West Arabia Terra, on Mars. The crater is characterized by deposits showing alternations of bright material, apparently hard and massive, and dark material, less resistant than the former. Recent data from the Mars Reconnaissance Orbiter mission have allowed a detailed analysis to be made of the depositional sequence, a stratigraphic column to be constructed (in progress), and several interesting surface features to be identified. The basis of our stratigraphic study was the analysis of a US Geological Survey HiRISE DTM covering our investigation area as well as the use of a software tool that allows layer attitudes (dip and strike angles) to be computed from remote-sensing data. Our observations, combined with larger-scale investigations conducted by other authors, allow us to constrain the possible formation mechanisms of these layered deposits and to relate them to past changes in Martian climate.

Keywords

Mars Stratigraphy Climate change HiRISE MRO Danielson Crater 

References

  1. Andrews-Hanna, J. C., Zuber, M. T,, Arvidson, R. E., & Wiseman, S. M. (2010). Early Mars hydrology: Meridiani playa deposits and the sedimentary record of Arabia Terra. Journal of Geophysical Research Planets115, 1−22.Google Scholar
  2. Cadieux, S. B. (2011). Constraining Martian Sedimentation Via Analysis of Stratal Packaging, Intracrater Layered Deposits, Arabia Terra, Mars (p. 101). Master Thesis, University of Tennessee.Google Scholar
  3. Chavdarian, G. V., & Sumner, D. Y. (2011). Origin and evolution of polygonal cracks in hydrous sulphate sands. White Sands National Monument, New Mexico, Sedimentology,58(2), 407–423.Google Scholar
  4. Edgett, K. S. (2005). The sedimentary rocks of sinus meridiani: Five key observations from data acquired by the Mars global surveyor and Mars Odyssey orbiters. Mars,1, 5–58.CrossRefGoogle Scholar
  5. Kneissl, T., van Gasselt, S., & Neukum, G. (2010). Measurement of Strike and Dip of Geologic Layers from Remote Sensing Data—New Software Tool for ArcGIS. Lunar and Planetary Institute Science Conference Abstracts (p. 1640). The Woodlands: 41.Google Scholar
  6. Laskar, J., Correia, A. C. M., Gastineau, M., Joutel, F., Levrard, B., & Robutel, P. (2004). Long term evolution and chaotic diffusion of the insolation quantities of Mars. Icarus,170(2), 343–364.CrossRefGoogle Scholar
  7. Malin, M.C., & Edgett, K.S. (2000). Sedimentary rocks of early Mars, Science290(5498), 1927–1937.CrossRefGoogle Scholar
  8. Sgavetti, M. (1992). Criteria for stratigraphic correlation using aerial photographs—examples from the south-central Pyrenees. AAPG Bulletin-American Association of Petroleum Geologists,76(5), 708–730.Google Scholar
  9. Squyres, S. W., & Knoll, A. H. (2005). Sedimentary rocks at meridiani planum: Origin, diagenesis, and implications for life on Mars. Earth and Planetary Science Letters,240(1), 1–10.CrossRefGoogle Scholar
  10. Wiseman, S. M, Arvidson, R. E., Morris, R. V, Poulet, F., Andrews-Hanna, J. C., & Bishop, J. L. et al. (2010). Spectral and stratigraphic mapping of hydrated sulfate and phyllosilicate-bearing deposits in northern Sinus Meridiani, Mars, Geophysical Research Planets 115, 1−31.Google Scholar

Copyright information

© Springer-Verlag Berlin Heidelberg 2014

Authors and Affiliations

  1. 1.International Research School of Planetary SciencesUniversità “G. D’Annunzio”PescaraItaly
  2. 2.Institute of Geological Sciences, Planetary Sciences and Remote SensingFreie Universitaet BerlinBerlinGermany

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