{"id":20355,"date":"2019-09-02T06:55:08","date_gmt":"2019-09-02T04:55:08","guid":{"rendered":"http:\/\/karmaka.de\/?p=20355"},"modified":"2019-09-02T06:55:11","modified_gmt":"2019-09-02T04:55:11","slug":"silica-minerals-in-cumulate-eucrites-insights-into-their-thermal-histories","status":"publish","type":"post","link":"https:\/\/karmaka.de\/?p=20355","title":{"rendered":"Silica minerals in cumulate eucrites: Insights into their thermal histories"},"content":{"rendered":"\n<p class=\"justify-text\">Haruka Ono, Atsushi Takenouchi, Takashi Mikouchi, Akira Yamaguchi <\/p>\n\n\n\n<p>Meteoritics &amp; Planetary Science<br>\nFirst Published:  1 September 2019<\/p>\n\n\n\n<p><a href=\"https:\/\/onlinelibrary.wiley.com\/doi\/full\/10.1111\/maps.13384\" target=\"_blank\" rel=\"noreferrer noopener\"><strong>LINK<\/strong><\/a><\/p>\n\n\n\n<p class=\"justify-text\">&#8220;Some eucrites contain up to 10 vol% silica minerals; however, silica minerals have not been studied in detail so far. We performed a mineralogical study of silica minerals in three cumulate eucrites (Moore County, Moama, and Yamato [Y] 980433). Monoclinic tridymite was common in all three samples. Moama contained orthorhombic tridymite as lamellae within monoclinic tridymite grains. Y 980433 included quartz around an impact melt vein. The presence of orthorhombic tridymite in Moama indicates that Moama cooled more rapidly than the other two samples at low temperatures (&lt;400 \u00b0C). This result is different from the slower cooling rates of Moama (\u22730.0004 \u00b0C yr\u22121) than that of Moore County (>0.3 \u00b0C yr\u22121, after the shock event) at high temperatures (>500 \u00b0C) estimated from compositional profiles of pyroxene exsolution lamellae. The difference of the cooling rates may reflejustify-textct their geological settings. Y 980433 cooled slowly at low temperature, as did Moore County. Quartz in Y 980433 could be a local product transformed from monoclinic tridymite by a shock event. We suggest that silica minerals in meteorites record thermal histories at low temperatures and shock events.&#8221;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Haruka Ono, Atsushi Takenouchi, Takashi Mikouchi, Akira Yamaguchi Meteoritics &amp; Planetary Science First Published: 1 September 2019 LINK &#8220;Some eucrites contain up to 10 vol% silica minerals; however, silica minerals have not been studied in&#8230;<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[35,33],"tags":[2827,1823,212,5162,2833,5163],"_links":{"self":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/20355"}],"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=20355"}],"version-history":[{"count":1,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/20355\/revisions"}],"predecessor-version":[{"id":20356,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/20355\/revisions\/20356"}],"wp:attachment":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=20355"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=20355"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=20355"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}