{"id":4633,"date":"2015-05-15T19:15:59","date_gmt":"2015-05-15T17:15:59","guid":{"rendered":"http:\/\/karmaka.de\/?p=4633"},"modified":"2015-05-15T19:36:06","modified_gmt":"2015-05-15T17:36:06","slug":"spatial-distributions-of-secondary-minerals-in-the-martian-meteorite-mil-03346168-determined-by-raman-spectroscopic-imaging","status":"publish","type":"post","link":"https:\/\/karmaka.de\/?p=4633","title":{"rendered":"Spatial distributions of secondary minerals in the Martian meteorite MIL 03346,168 determined by Raman spectroscopic imaging"},"content":{"rendered":"<p>Zongcheng Ling and Alian Wang<\/p>\n<p>Journal of Geophysical Research: Planets<br \/>\nAccepted manuscript online: 15 MAY 2015<br \/>\nDOI: 10.1002\/2015JE004805<\/p>\n<p><a href=\"http:\/\/onlinelibrary.wiley.com\/doi\/10.1002\/2015JE004805\/full\" target=\"_blank\"><strong>LINK<\/strong><\/a><\/p>\n<div class=\"su-quote su-quote-style-default\"><div class=\"su-quote-inner su-u-clearfix su-u-trim\">Miller Range (MIL) 03346 is a nakhlite meteorite that has been extensively studied due to its unique complex secondary mineral phases and their potential implications for the hydrologic history of Mars. We conducted a set of Raman spectroscopic and Raman imaging studies of MIL 03346,168, focusing on the secondary mineral phases and their spatial distributions, with a goal to better understand the possible processes by which they were generated on Mars. This study revealed three types of calcium sulfates, a solid solutions of (K, Na)-jarosite and two groups of hydrated species with low crystallinity (HSLC) in the veins and\/or mesostasis areas of the meteorite. The most abundant Ca-sulfate is bassanite that suggests two possible paths for its direct precipitation from a Ca-S-H2O brine, either having low water activity or with incomplete development (producing bassanite with gypsum microcrystals) on Mars. The second most abundant Ca-sulfate is soluble \u03b3-CaSO4 which raises a new question on the origins of this phase in the martian meteorite, since \u03b3-CaSO4 readily hydrates in the laboratory but is apparently stable in Atacama Desert. The close spatial relationship of (K, Na)-jarosite solid solutions with rasvumite (KFe2S3), magnetite, HSLC, and fine-grained low crystallinity alkali feldspar in mesostasis suggests a potential in situ formation of mesostasis jarosite from these Fe-K,Na-S-O-H2O species.<\/div><\/div>\n","protected":false},"excerpt":{"rendered":"<p>Zongcheng Ling and Alian Wang Journal of Geophysical Research: Planets Accepted manuscript online: 15 MAY 2015 DOI: 10.1002\/2015JE004805 LINK<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[42,44],"tags":[1828,638,696,1830,264,1418],"_links":{"self":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/4633"}],"collection":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=4633"}],"version-history":[{"count":2,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/4633\/revisions"}],"predecessor-version":[{"id":4635,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/4633\/revisions\/4635"}],"wp:attachment":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=4633"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=4633"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=4633"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}