{"id":21975,"date":"2020-05-04T12:44:42","date_gmt":"2020-05-04T10:44:42","guid":{"rendered":"http:\/\/karmaka.de\/?p=21975"},"modified":"2020-05-04T12:44:55","modified_gmt":"2020-05-04T10:44:55","slug":"the-effects-of-secondary-processing-in-the-unique-carbonaceous-chondrite-miller-range-07687","status":"publish","type":"post","link":"https:\/\/karmaka.de\/?p=21975","title":{"rendered":"The effects of secondary processing in the unique carbonaceous chondrite Miller Range 07687"},"content":{"rendered":"\n<p>Pierre Haenecour, Christine Floss, Adrian J. Brearley, Thomas J. Zega<\/p>\n\n\n\n<p>Meteoritics &amp; Planetary Science<br>First Published: 3 May 2020<\/p>\n\n\n\n<p><a href=\"https:\/\/onlinelibrary.wiley.com\/doi\/full\/10.1111\/maps.13477\" target=\"_blank\" rel=\"noreferrer noopener\"><strong>LINK<\/strong><\/a><\/p>\n\n\n\n<p class=\"justify-text\">&#8220;Our detailed mineralogical, elemental, and isotopic study of the Miller Range (MIL) 07687 meteorite showed that, although this meteorite has affinities to CO chondrites, it also exhibits sufficient differences to warrant classification as an ungrouped carbonaceous chondrite. The most notable feature of MIL 07687 is the presence of two distinct matrix lithologies that result from highly localized aqueous alteration. One of these lithologies is Fe\u2010rich and exhibits evidence for interaction with water, including the presence of fibrous (dendritic) ferrihydrite. The other lithology, which is Fe\u2010poor, appears to represent relatively unaltered protolith material. MIL 07687 has presolar grain abundances consistent with those observed in other modestly altered carbonaceous chondrites: the overall abundance of O\u2010rich presolar grains is 137 \u00b1 3 ppm and the overall abundance of SiC grains is 71 \u00b1 11 ppm. However, there is a large difference in the observed O\u2010rich and SiC grain number densities between altered and unaltered areas, reflecting partial destruction of presolar grains (both O\u2010 and C\u2010rich grains) due to the aqueous alteration experienced by MIL 07687 under highly oxidizing conditions. Detailed coordinated NanoSIMS\u2010TEM analysis of a large hotspot composed of an isotopically normal core surrounded by a rim composed of 17O\u2010rich grains is consistent with either original condensation of the core and surrounding grains in the same parent AGB star, or with grain accretion in the ISM or solar nebula.&#8221;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Pierre Haenecour, Christine Floss, Adrian J. Brearley, Thomas J. Zega Meteoritics &amp; Planetary ScienceFirst Published: 3 May 2020 LINK &#8220;Our detailed mineralogical, elemental, and isotopic study of the Miller Range (MIL) 07687 meteorite showed that,&#8230;<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[9,335],"tags":[3273,1590,964,1731],"_links":{"self":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/21975"}],"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=21975"}],"version-history":[{"count":1,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/21975\/revisions"}],"predecessor-version":[{"id":21976,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/21975\/revisions\/21976"}],"wp:attachment":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=21975"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=21975"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=21975"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}