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Nitrogen Incorporation in Potassic and Micro- and Meso-Porous Minerals: Potential Biogeochemical Records and Targets for Mars Sampling.
Nikitczuk, Matthew P; Bebout, Gray E; Geiger, Charles A; Ota, Tsutomu; Kunihiro, Takuya; Mustard, John F; Halldórsson, Sæmundur A; Nakamura, Eizo.
Afiliación
  • Nikitczuk MP; Department of Earth and Environmental Sciences, Lehigh University, Bethlehem, Pennsylvania, USA.
  • Bebout GE; Department of Earth and Environmental Sciences, Lehigh University, Bethlehem, Pennsylvania, USA.
  • Geiger CA; Pheasant Memorial Laboratory for Geochemistry and Cosmochemistry, Institute for Planetary Materials, Okayama University, Misasa, Japan.
  • Ota T; Universität Salzburg, Fachbereich Chemie und Physik der Materialien, Salzburg, Austria.
  • Kunihiro T; Pheasant Memorial Laboratory for Geochemistry and Cosmochemistry, Institute for Planetary Materials, Okayama University, Misasa, Japan.
  • Mustard JF; Pheasant Memorial Laboratory for Geochemistry and Cosmochemistry, Institute for Planetary Materials, Okayama University, Misasa, Japan.
  • Halldórsson SA; Department of Earth, Environmental and Planetary Sciences, Brown University, Providence, Rhode Island, USA.
  • Nakamura E; Nordic Volcanological Center, Institute of Earth Sciences, University of Iceland, Reykjavík, Iceland.
Astrobiology ; 22(11): 1293-1309, 2022 11.
Article en En | MEDLINE | ID: mdl-36074082
ABSTRACT
We measured the N concentrations and isotopic compositions of 44 samples of terrestrial potassic and micro- and meso-porous minerals and a small number of whole-rocks to determine the extent to which N is incorporated and stored during weathering and low-temperature hydrothermal alteration in Mars surface/near-surface environments. The selection of these minerals and other materials was partly guided by the study of altered volcanic glass from Antarctica and Iceland, in which the incorporation of N as NH4+ in phyllosilicates is indicated by correlated concentrations of N and the LILEs (i.e., K, Ba, Rb, Cs), with scatter likely related to the presence of exchanged, occluded/trapped, or encapsulated organic/inorganic N occurring within structural cavities (e.g., in zeolites). The phyllosilicates, zeolites, and sulfates analyzed in this study contain between 0 and 99,120 ppm N and have δ15Nair values of -34‰ to +65‰. Most of these minerals, and the few siliceous hydrothermal deposits that were analyzed, have δ15N consistent with the incorporation of biologically processed N during low-temperature hydrothermal or weathering processes. Secondary ion mass spectrometry on altered hyaloclastites demonstrates the residency of N in smectites and zeolites, and silica. We suggest that geological materials known on Earth to incorporate and store N and known to be abundant at, or near, the surface of Mars should be considered targets for upcoming Mars sample return with the intent to identify any signs of ancient or modern life.
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Texto completo: 1 Bases de datos: MEDLINE Asunto principal: Zeolitas / Marte Idioma: En Revista: Astrobiology Asunto de la revista: BIOLOGIA Año: 2022 Tipo del documento: Article País de afiliación: Estados Unidos

Texto completo: 1 Bases de datos: MEDLINE Asunto principal: Zeolitas / Marte Idioma: En Revista: Astrobiology Asunto de la revista: BIOLOGIA Año: 2022 Tipo del documento: Article País de afiliación: Estados Unidos