Chemically striking regions on Mars and Stealth revisited

The Mars Odyssey Gamma Ray Spectrometer Suite has yielded global chemical information for Mars. In this work, we establish regions of unusual chemical composition relative to average Mars primarily on the basis of Ca, Cl, Fe, H, K, Si, and Th. Using data from Mars Odyssey; the Mars Exploration Rover...

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Published inJournal of Geophysical Research. B. Solid Earth Vol. 114; no. E12
Main Authors Karunatillake, Suniti, Wray, James J., Squyres, Steven W., Taylor, G. Jeffrey, Gasnault, Olivier, McLennan, Scott M., Boynton, William, El Maarry, M. R., Dohm, James M.
Format Journal Article
LanguageEnglish
Published Washington, DC Blackwell Publishing Ltd 01.12.2009
American Geophysical Union
Subjects
chemically striking regions
Dust
Earth sciences
Earth, ocean, space
Exact sciences and technology
Fog
Gamma rays
Low temperature
Mars
Planetology
Planets
Radar
Remote sensing
Scientific apparatus & instruments
stealth
Sulfates
Volcanoes
gamma rays
global
air
Snowfall
sulfates
Earth
Mars
brines
acids
ground ice
dust
MRO space probe
Fog
exploration
salt
Regional scope
volcanoes
transport
low temperature
chemically precipitated rocks
evaporites
in situ
sedimentary rocks
depth
Radar observation
chemical composition
radar methods
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Abstract The Mars Odyssey Gamma Ray Spectrometer Suite has yielded global chemical information for Mars. In this work, we establish regions of unusual chemical composition relative to average Mars primarily on the basis of Ca, Cl, Fe, H, K, Si, and Th. Using data from Mars Odyssey; the Mars Exploration Rovers; the Mars Reconnaissance Orbiter Imaging; and 3.5 cm and 1.35 cm radar observations from Earth, we examine a chemically striking ≈2.E6 km2 region and find it to overlap significantly with a radar Stealth region on Mars. It is remarkably enriched in Cl and depleted in Fe and Si (along with minor variations in H, K, and Th) relative to average Mars. Surface dust observed at the two rover sites mixed with and indurated by Ca/Mg‐bearing sulfate salts would be a reasonable chemical and physical analog to meter‐scale depths. We describe potential scenarios that may have contributed to the unique properties of this region. The bulk dust component may be an air fall deposit of compositionally uniform dust as observed in situ. Hydrothermal acid fog reactions on the flanks of nearby volcanoes may have generated sulfates with subsequent deflation and transport. Alternatively, sulfates may have been produced by low‐temperature, regional‐scale activity of ground ice–driven brine and/or regional‐scale deposition of acidified H2O snowfall.
AbstractList The Mars Odyssey Gamma Ray Spectrometer Suite has yielded global chemical information for Mars. In this work, we establish regions of unusual chemical composition relative to average Mars primarily on the basis of Ca, Cl, Fe, H, K, Si, and Th. Using data from Mars Odyssey; the Mars Exploration Rovers; the Mars Reconnaissance Orbiter Imaging; and 3.5 cm and 1.35 cm radar observations from Earth, we examine a chemically striking [asymptotic to]2.E6 km2 region and find it to overlap significantly with a radar Stealth region on Mars. It is remarkably enriched in Cl and depleted in Fe and Si (along with minor variations in H, K, and Th) relative to average Mars. Surface dust observed at the two rover sites mixed with and indurated by Ca/Mg-bearing sulfate salts would be a reasonable chemical and physical analog to meter-scale depths. We describe potential scenarios that may have contributed to the unique properties of this region. The bulk dust component may be an air fall deposit of compositionally uniform dust as observed in situ. Hydrothermal acid fog reactions on the flanks of nearby volcanoes may have generated sulfates with subsequent deflation and transport. Alternatively, sulfates may have been produced by low-temperature, regional-scale activity of ground ice-driven brine and/or regional-scale deposition of acidified H2O snowfall.
The Mars Odyssey Gamma Ray Spectrometer Suite has yielded global chemical information for Mars. In this work, we establish regions of unusual chemical composition relative to average Mars primarily on the basis of Ca, Cl, Fe, H, K, Si, and Th. Using data from Mars Odyssey; the Mars Exploration Rovers; the Mars Reconnaissance Orbiter Imaging; and 3.5 cm and 1.35 cm radar observations from Earth, we examine a chemically striking -2.E6 km2 region and find it to overlap significantly with a radar Stealth region on Mars. It is remarkably enriched in Cl and depleted in Fe and Si (along with minor variations in H, K, and Th) relative to average Mars. Surface dust observed at the two rover sites mixed with and indurated by Ca/Mg-bearing sulfate salts would be a reasonable chemical and physical analog to meter-scale depths. We describe potential scenarios that may have contributed to the unique properties of this region. The bulk dust component may be an air fall deposit of compositionally uniform dust as observed in situ. Hydrothermal acid fog reactions on the flanks of nearby volcanoes may have generated sulfates with subsequent deflation and transport. Alternatively, sulfates may have been produced by low-temperature, regional-scale activity of ground ice-driven brine and/or regional-scale deposition of acidified H2O snowfall.
The Mars Odyssey Gamma Ray Spectrometer Suite has yielded global chemical information for Mars. In this work, we establish regions of unusual chemical composition relative to average Mars primarily on the basis of Ca, Cl, Fe, H, K, Si, and Th. Using data from Mars Odyssey; the Mars Exploration Rovers; the Mars Reconnaissance Orbiter Imaging; and 3.5 cm and 1.35 cm radar observations from Earth, we examine a chemically striking ≈2.E6 km 2 region and find it to overlap significantly with a radar Stealth region on Mars. It is remarkably enriched in Cl and depleted in Fe and Si (along with minor variations in H, K, and Th) relative to average Mars. Surface dust observed at the two rover sites mixed with and indurated by Ca/Mg‐bearing sulfate salts would be a reasonable chemical and physical analog to meter‐scale depths. We describe potential scenarios that may have contributed to the unique properties of this region. The bulk dust component may be an air fall deposit of compositionally uniform dust as observed in situ. Hydrothermal acid fog reactions on the flanks of nearby volcanoes may have generated sulfates with subsequent deflation and transport. Alternatively, sulfates may have been produced by low‐temperature, regional‐scale activity of ground ice–driven brine and/or regional‐scale deposition of acidified H 2 O snowfall.
The Mars Odyssey Gamma Ray Spectrometer Suite has yielded global chemical information for Mars. In this work, we establish regions of unusual chemical composition relative to average Mars primarily on the basis of Ca, Cl, Fe, H, K, Si, and Th. Using data from Mars Odyssey; the Mars Exploration Rovers; the Mars Reconnaissance Orbiter Imaging; and 3.5 cm and 1.35 cm radar observations from Earth, we examine a chemically striking ≈2.E6 km2 region and find it to overlap significantly with a radar Stealth region on Mars. It is remarkably enriched in Cl and depleted in Fe and Si (along with minor variations in H, K, and Th) relative to average Mars. Surface dust observed at the two rover sites mixed with and indurated by Ca/Mg‐bearing sulfate salts would be a reasonable chemical and physical analog to meter‐scale depths. We describe potential scenarios that may have contributed to the unique properties of this region. The bulk dust component may be an air fall deposit of compositionally uniform dust as observed in situ. Hydrothermal acid fog reactions on the flanks of nearby volcanoes may have generated sulfates with subsequent deflation and transport. Alternatively, sulfates may have been produced by low‐temperature, regional‐scale activity of ground ice–driven brine and/or regional‐scale deposition of acidified H2O snowfall.
The Mars Odyssey Gamma Ray Spectrometer Suite has yielded global chemical information for Mars. In this work, we establish regions of unusual chemical composition relative to average Mars primarily on the basis of Ca, Cl, Fe, H, K, Si, and Th. Using data from Mars Odyssey; the Mars Exploration Rovers; the Mars Reconnaissance Orbiter Imaging; and 3.5 cm and 1.35 cm radar observations from Earth, we examine a chemically striking 2.E6 km2 region and find it to overlap significantly with a radar Stealth region on Mars. It is remarkably enriched in Cl and depleted in Fe and Si (along with minor variations in H, K, and Th) relative to average Mars. Surface dust observed at the two rover sites mixed with and indurated by Ca/Mg-bearing sulfate salts would be a reasonable chemical and physical analog to meter-scale depths. We describe potential scenarios that may have contributed to the unique properties of this region. The bulk dust component may be an air fall deposit of compositionally uniform dust as observed in situ. Hydrothermal acid fog reactions on the flanks of nearby volcanoes may have generated sulfates with subsequent deflation and transport. Alternatively, sulfates may have been produced by low-temperature, regional-scale activity of ground icedriven brine and/or regional-scale deposition of acidified H2O snowfall.
Author Boynton, William
Gasnault, Olivier
Wray, James J.
El Maarry, M. R.
Karunatillake, Suniti
Dohm, James M.
McLennan, Scott M.
Squyres, Steven W.
Taylor, G. Jeffrey
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  givenname: Suniti
  surname: Karunatillake
  fullname: Karunatillake, Suniti
  email: wk43@cornell.edu
  organization: Department of Geosciences, State University of New York at Stony Brook, Stony Brook, New York, USA
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  givenname: James J.
  surname: Wray
  fullname: Wray, James J.
  organization: Department of Astronomy, Cornell University, New York, Ithaca, USA
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  givenname: Steven W.
  surname: Squyres
  fullname: Squyres, Steven W.
  organization: Department of Astronomy, Cornell University, New York, Ithaca, USA
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  givenname: G. Jeffrey
  surname: Taylor
  fullname: Taylor, G. Jeffrey
  organization: Hawaii Institute of Geophysics and Planetology, University of Hawai'i at Manoa, Hawaii, Honolulu, USA
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  fullname: Gasnault, Olivier
  organization: Université Paul Sabatier, Toulouse III, France
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  organization: Department of Geosciences, State University of New York at Stony Brook, New York, Stony Brook, USA
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  givenname: William
  surname: Boynton
  fullname: Boynton, William
  organization: Lunar and Planetary Laboratory, University of Arizona, Arizona, Tucson, USA
– sequence: 8
  givenname: M. R.
  surname: El Maarry
  fullname: El Maarry, M. R.
  organization: Max-Planck Institut fur Sonnensystemforschung, Katlenberg-Lindau, Germany
– sequence: 9
  givenname: James M.
  surname: Dohm
  fullname: Dohm, James M.
  organization: Department of Hydrology and Water Resources, University of Arizona, Arizona, Tucson, USA
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Issue E12
Keywords gamma rays
global
air
Snowfall
sulfates
Earth
Mars
brines
acids
ground ice
dust
MRO space probe
Fog
exploration
salt
Regional scope
volcanoes
transport
low temperature
chemically precipitated rocks
evaporites
in situ
sedimentary rocks
depth
Radar observation
chemical composition
radar methods
Language English
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PublicationTitle Journal of Geophysical Research. B. Solid Earth
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American Geophysical Union
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– name: American Geophysical Union
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Snippet The Mars Odyssey Gamma Ray Spectrometer Suite has yielded global chemical information for Mars. In this work, we establish regions of unusual chemical...
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SubjectTerms chemically striking regions
Dust
Earth sciences
Earth, ocean, space
Exact sciences and technology
Fog
Gamma rays
Low temperature
Mars
Planetology
Planets
Radar
Remote sensing
Scientific apparatus & instruments
stealth
Sulfates
Volcanoes
Title Chemically striking regions on Mars and Stealth revisited
URI https://api.istex.fr/ark:/67375/WNG-K4DZ6QRL-X/fulltext.pdf
https://onlinelibrary.wiley.com/doi/abs/10.1029%2F2008JE003303
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https://search.proquest.com/docview/21316567
https://search.proquest.com/docview/36362239
https://search.proquest.com/docview/787068458
Volume 114
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