Hyperspectral mapping of alteration assemblages within a hydrothermal vug at the Haughton impact structure, Canada

• Published in: Meteoritics & Planetary Science
• Main Authors: Greenberger, Rebecca N., Mustard, John F., Osinski, Gordon R., Tornabene, Livio L., Pontefract, Alexandra J., Marion, Cassandra L., Flemming, Roberta L., Wilson, Janette H., Cloutis, Edward A.
• Other Authors: Natural Sciences and Engineering Research Council of Canada
• Format: Article in Journal/Newspaper
• Language: English
• Published: Wiley 2016
• Subjects: Space and Planetary Science; Geophysics; Nunavut; Canada; Devon Island
• Online Access: http://dx.doi.org/10.1111/maps.12716; https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1111%2Fmaps.12716; https://onlinelibrary.wiley.com/doi/pdf/10.1111/maps.12716

Abstract Meteorite impacts on Earth and Mars can generate hydrothermal systems that alter the primary mineralogies of rocks and provide suitable environments for microbial colonization. We investigate a calcite–marcasite‐bearing vug at the ~23 km diameter Haughton impact structure, Devon Island, Nunavut, Canada, using imaging spectroscopy of the outcrop in the field (0.65–1.1 μm) and samples in the laboratory (0.4–2.5 μm), point spectroscopy (0.35–2.5 μm), major element chemistry, and X‐ray diffraction analyses. The mineral assemblages mapped at the outcrop include marcasite; marcasite with minor gypsum and jarosite; fibroferrite and copiapite with minor gypsum and melanterite; gypsum, Fe 3+ oxides, and jarosite; and calcite, gypsum, clay, microcline, and quartz. Hyperspectral mapping of alteration phases shows spatial patterns that illuminate changes in alteration conditions and formation of specific mineral phases. Marcasite formed from the postimpact hydrothermal system under reducing conditions, while subsequent weathering oxidized the marcasite at low temperatures and water/rock ratios. The acidic fluids resulting from the oxidation collected on flat‐lying portions of the outcrop, precipitating fibroferrite + copiapite. That assemblage then likely dissolved, and the changing chemistry and pH resulting from interaction with the calcite‐rich host rock formed gypsum‐bearing red coatings. These results have implications for understanding water–rock interactions and habitabilities at this site and on Mars.