TY - JOUR
T1 - Nitrogenous Altered Volcanic Glasses as Targets for Mars Sample Return
T2 - Examples From Antarctica and Iceland
AU - Nikitczuk, M. P.
AU - Edward Bebout, Gray
AU - Ota, T.
AU - Kunihiro, T.
AU - Mustard, J. F.
AU - Flemming, R. L.
AU - Tanaka, R.
AU - Halldórsson, S. A.
AU - Nakamura, E.
N1 - Funding Information:
M. P. Nikitczuk acknowledges support of the N isotope work from the National Science Foundation (grant EAR‐1624092 to G. E. Bebout), of the micro‐analytical and geochemical work by the Pheasant Memorial Laboratory (Institute for Planetary Materials), and of the micro‐XRD analyses by The University of Western Ontario (NSERC Discovery Grant RGPIN‐2016‐06048 to R. L. Flemming). Funding for the work at the IPM was from grants from the 21st Century Center of Excellence, Japanese Ministry of Education, Science, Sports, and Culture (to E. Nakamura). Additional funding for geochemical and mineralogical analyses, was provided by the Lehigh University Department of Earth and Environmental Sciences, Office of International Students and Scholars (OISS), and College of Arts and Sciences (CAS). The authors thank Bruce Idleman for ongoing technical support in the stable isotope geochemistry laboratory at the Lehigh University.
Publisher Copyright:
© 2022 The Authors.
PY - 2022/2
Y1 - 2022/2
N2 - Mars exploration is focused on seeking evidence of habitable environments and microbial life. Terrestrial glassy basalts may be the closest Mars-surface weathering analog and observations increasingly indicate their potential to preserve biogeochemical records. The textures, major and trace element geochemistry, and N concentrations and isotopic compositions of subaerial, subglacial and continental lacustrine hyaloclastites from Antarctica, Iceland, and Oregon, respectively, were studied using micro-imaging and chemical methods, including gas-source mass spectrometry. Alteration by meteoric-sourced waters occurred in circum-neutral, increasingly alkaline low-temperature conditions of ∼60°C–100°C (Iceland) and ∼60°C–170°C (Antarctica). Incompatible large ion lithophile element (LILE) enrichments compared to mid-ocean ridge basalt (MORB) are consistent with more advanced alteration in Antarctic breccias consisting of heulandite-clinoptilolite, calcite, erionite, quartz, and fluorapophyllite. Granular and tubular alteration textures and radial apatite represent possible microbial traces. Most samples contain more N than fresh MORB or ocean island basalt reflecting enrichment beyond concentrations attributable to igneous processes. Antarctic samples contain 52–1,143 ppm N and have δ15Νair values of −20.8‰ to −7.1‰. Iceland-Oregon basalts contain 1.6–172 ppm N with δ15Ν of −6.7‰ to +7.3‰. Correlations between alteration extents, N concentrations, and concentrations of K2O, other LILEs, and Li and B, reflect the siting of secondary N likely as NH4+ replacing K+ and potentially as N2 in phyllosilicates and zeolites. Although much of the N enrichment and isotope fractionation presented here is not definitively biogenic, given several unknown factors, we suggest that a combination of textures, major and trace element alteration and N and other isotope geochemical compositions could constitute a compelling biosignature in samples from Mars' surface/near-surface.
AB - Mars exploration is focused on seeking evidence of habitable environments and microbial life. Terrestrial glassy basalts may be the closest Mars-surface weathering analog and observations increasingly indicate their potential to preserve biogeochemical records. The textures, major and trace element geochemistry, and N concentrations and isotopic compositions of subaerial, subglacial and continental lacustrine hyaloclastites from Antarctica, Iceland, and Oregon, respectively, were studied using micro-imaging and chemical methods, including gas-source mass spectrometry. Alteration by meteoric-sourced waters occurred in circum-neutral, increasingly alkaline low-temperature conditions of ∼60°C–100°C (Iceland) and ∼60°C–170°C (Antarctica). Incompatible large ion lithophile element (LILE) enrichments compared to mid-ocean ridge basalt (MORB) are consistent with more advanced alteration in Antarctic breccias consisting of heulandite-clinoptilolite, calcite, erionite, quartz, and fluorapophyllite. Granular and tubular alteration textures and radial apatite represent possible microbial traces. Most samples contain more N than fresh MORB or ocean island basalt reflecting enrichment beyond concentrations attributable to igneous processes. Antarctic samples contain 52–1,143 ppm N and have δ15Νair values of −20.8‰ to −7.1‰. Iceland-Oregon basalts contain 1.6–172 ppm N with δ15Ν of −6.7‰ to +7.3‰. Correlations between alteration extents, N concentrations, and concentrations of K2O, other LILEs, and Li and B, reflect the siting of secondary N likely as NH4+ replacing K+ and potentially as N2 in phyllosilicates and zeolites. Although much of the N enrichment and isotope fractionation presented here is not definitively biogenic, given several unknown factors, we suggest that a combination of textures, major and trace element alteration and N and other isotope geochemical compositions could constitute a compelling biosignature in samples from Mars' surface/near-surface.
KW - basalt alteration
KW - biogeochemistry
KW - hyaloclastites
KW - Mars
KW - planetary sample-return
KW - stable isotopes (nitrogen)
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U2 - 10.1029/2021JE007052
DO - 10.1029/2021JE007052
M3 - Article
AN - SCOPUS:85125133764
SN - 2169-9097
VL - 127
JO - Journal of Geophysical Research: Planets
JF - Journal of Geophysical Research: Planets
IS - 2
M1 - e2021JE007052
ER -