{"id":228,"date":"2018-02-15T20:26:40","date_gmt":"2018-02-15T20:26:40","guid":{"rendered":"http:\/\/e-probe.epss.ucla.edu\/?page_id=228"},"modified":"2021-06-12T17:41:06","modified_gmt":"2021-06-12T17:41:06","slug":"what-we-do","status":"publish","type":"page","link":"https:\/\/dev-probe.epss.ucla.edu\/?page_id=228","title":{"rendered":"Geology"},"content":{"rendered":"\n<h4 class=\"has-text-align-center has-vivid-cyan-blue-color has-text-color wp-block-heading\" style=\"font-size:28px\"><strong>Elemental Maps and Quantitative Analysis of Minerals<\/strong><\/h4>\n\n\n\n<figure class=\"wp-block-image\"><a href=\"https:\/\/e-probe.epss.ucla.edu\/wp-content\/uploads\/2018\/02\/ar6-e1614852135390.jpg\"><img loading=\"lazy\" decoding=\"async\" width=\"1233\" height=\"1262\" src=\"https:\/\/e-probe.epss.ucla.edu\/wp-content\/uploads\/2018\/02\/ar6-e1614852135390.jpg\" alt=\"\" class=\"wp-image-227\"\/><\/a><\/figure>\n\n\n\n<p><span style=\"color: #800080;\">Elemental X-ray maps of a metamorphic garnet from Kongur Shan in China. Also included are a photomicrograph image in transmitted light (top-left) and a backscattered electron (BSE) image (center-left).&nbsp; The maps resulted from 2000 x 2000 analyzed spots with a 1 \u00b5m interval.&nbsp; Maps were created during four days of work.&nbsp; Quantitative analyses of selected oxides are showed on the center-right image.  Images are courtesy of Frank Kyte. <\/span><\/p>\n\n\n\n<div style=\"height:24px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<h4 class=\"has-text-align-center has-vivid-cyan-blue-color has-text-color wp-block-heading\" style=\"font-size:28px\"><strong>Asteroid Impact Ejecta <\/strong><\/h4>\n\n\n\n<div style=\"height:25px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<figure class=\"wp-block-image size-full is-resized\"><a href=\"https:\/\/e-probe.epss.ucla.edu\/wp-content\/uploads\/2021\/03\/Kyte_Fig1-scaled.jpg\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/e-probe.epss.ucla.edu\/wp-content\/uploads\/2021\/03\/Kyte_Fig1-scaled.jpg\" alt=\"\" class=\"wp-image-1197\" width=\"640\" height=\"605\" srcset=\"https:\/\/dev-probe.epss.ucla.edu\/wp-content\/uploads\/2021\/03\/Kyte_Fig1-scaled.jpg 2560w, https:\/\/dev-probe.epss.ucla.edu\/wp-content\/uploads\/2021\/03\/Kyte_Fig1-300x284.jpg 300w, https:\/\/dev-probe.epss.ucla.edu\/wp-content\/uploads\/2021\/03\/Kyte_Fig1-1024x968.jpg 1024w, https:\/\/dev-probe.epss.ucla.edu\/wp-content\/uploads\/2021\/03\/Kyte_Fig1-768x726.jpg 768w, https:\/\/dev-probe.epss.ucla.edu\/wp-content\/uploads\/2021\/03\/Kyte_Fig1-1536x1453.jpg 1536w, https:\/\/dev-probe.epss.ucla.edu\/wp-content\/uploads\/2021\/03\/Kyte_Fig1-2048x1937.jpg 2048w, https:\/\/dev-probe.epss.ucla.edu\/wp-content\/uploads\/2021\/03\/Kyte_Fig1-317x300.jpg 317w\" sizes=\"auto, (max-width: 640px) 100vw, 640px\" \/><\/a><\/figure>\n\n\n\n<div style=\"height:20px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n<p><span style=\"color: #800080;\">BSE images of impact spherules (scale bars = 10 ?m).&nbsp; A) Well-preserved Ca-rich pyroxene in a glass matrix with traces of Cr-rich spinel.&nbsp; B) Poorly preserved pyroxene that has been partially dissolved by seawater etching, leaving feathery voids.&nbsp; Bright grains near rim are small spinels (&lt;1 ?m).&nbsp; C,D) Strongly altered and flattened spherules with material missing from their rims.&nbsp; Composed mainly of Fe-rich oxides; silicates have been altered to clays.&nbsp; C) Well-developed spinels with skeletal textures in clay matrix. D) Abundant spinel crystals.&nbsp; Images are courtesy of Frank Kyte.<br><\/span><\/p>\n<p><span style=\"color: #800080;\">Modified from Kyte, F.T., Shukolyukov, A., Hildebrand, A.R., Lugmair, G.W., and Hanova, J., 2014.&nbsp; Chromium-isotopes in Late Eocene impact spherules indicate a likely asteroid belt provenance: <em>Earth and Planetary Science Letters<\/em> 302, 279-286.<\/span><\/p>\n<p><a href=\"https:\/\/www.sciencedirect.com\/science\/article\/pii\/S0012821X10007582\">https:\/\/www.sciencedirect.com\/science\/article\/pii\/S0012821X10007582<\/a><\/p>\n\n\n<div style=\"height:25px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<h4 class=\"has-text-align-center has-vivid-cyan-blue-color has-text-color wp-block-heading\" style=\"font-size:28px\"><strong>CAI from Meteorite <\/strong><\/h4>\n\n\n\n<div style=\"height:25px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-image\"><figure class=\"alignleft size-large is-resized\"><a href=\"https:\/\/e-probe.epss.ucla.edu\/wp-content\/uploads\/2021\/06\/CAI_Dunham.jpg\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/e-probe.epss.ucla.edu\/wp-content\/uploads\/2021\/06\/CAI_Dunham-1024x1018.jpg\" alt=\"\" class=\"wp-image-1333\" width=\"648\" height=\"644\" srcset=\"https:\/\/dev-probe.epss.ucla.edu\/wp-content\/uploads\/2021\/06\/CAI_Dunham-1024x1018.jpg 1024w, https:\/\/dev-probe.epss.ucla.edu\/wp-content\/uploads\/2021\/06\/CAI_Dunham-300x298.jpg 300w, https:\/\/dev-probe.epss.ucla.edu\/wp-content\/uploads\/2021\/06\/CAI_Dunham-150x150.jpg 150w, https:\/\/dev-probe.epss.ucla.edu\/wp-content\/uploads\/2021\/06\/CAI_Dunham-768x764.jpg 768w, https:\/\/dev-probe.epss.ucla.edu\/wp-content\/uploads\/2021\/06\/CAI_Dunham-1536x1528.jpg 1536w, https:\/\/dev-probe.epss.ucla.edu\/wp-content\/uploads\/2021\/06\/CAI_Dunham-302x300.jpg 302w, https:\/\/dev-probe.epss.ucla.edu\/wp-content\/uploads\/2021\/06\/CAI_Dunham.jpg 1854w\" sizes=\"auto, (max-width: 648px) 100vw, 648px\" \/><\/a><\/figure><\/div>\n\n\n\n<div style=\"height:20px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n<p><span style=\"color: #800080;\"><strong>C<\/strong>alcium-rich, <strong>A<\/strong>luminum-rich <strong>I<\/strong>nclusions (CAIs) are the first solids formed in our Solar System and preserve information about the earliest events in the solar nebula. Shown here is a small CAI that is composed of corundum (Al<sub>2<\/sub>O<sub>3<\/sub>) and hibonite (Ca(Al,Ti,Mg)<sub>12<\/sub>O<sub>19<\/sub>), which are high-temperature minerals that form out of solar composition gas &gt;1600 \u00b0C. The X-ray elemental maps show the minerals more clearly and the Ti map shows that the hibonite has some Ti that distributed unevenly. This CAI was found in a pristine ordinary chondrite meteorite, NWA 8576, which was loaned from the UCLA meteorite collection by Alan Rubin.&nbsp; Images are courtesy of Emilie Dunham.<\/span><\/p>\n<p><span style=\"color: #800080;\">This project is funded by the 51 Pegasi b Fellowship:<\/span><\/p>\n<p><a href=\"https:\/\/www.hsfoundation.org\/fellow\/emilie-dunham-ph-d-candidate\/\">https:\/\/www.hsfoundation.org\/fellow\/emilie-dunham-ph-d-candidate\/<\/a><\/p>\n\n\n<div style=\"height:25px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n","protected":false},"excerpt":{"rendered":"<p>Elemental Maps and Quantitative Analysis of Minerals Elemental X-ray maps of a metamorphic garnet from Kongur Shan in China. Also included are a photomicrograph image in transmitted light (top-left) and a backscattered electron (BSE) image (center-left).&nbsp; The maps resulted from 2000 x 2000 analyzed spots with a 1 \u00b5m interval.&nbsp; Maps were created during four&#8230;<\/p>\n","protected":false},"author":5,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-228","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/dev-probe.epss.ucla.edu\/index.php?rest_route=\/wp\/v2\/pages\/228","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/dev-probe.epss.ucla.edu\/index.php?rest_route=\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/dev-probe.epss.ucla.edu\/index.php?rest_route=\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/dev-probe.epss.ucla.edu\/index.php?rest_route=\/wp\/v2\/users\/5"}],"replies":[{"embeddable":true,"href":"https:\/\/dev-probe.epss.ucla.edu\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=228"}],"version-history":[{"count":54,"href":"https:\/\/dev-probe.epss.ucla.edu\/index.php?rest_route=\/wp\/v2\/pages\/228\/revisions"}],"predecessor-version":[{"id":1346,"href":"https:\/\/dev-probe.epss.ucla.edu\/index.php?rest_route=\/wp\/v2\/pages\/228\/revisions\/1346"}],"wp:attachment":[{"href":"https:\/\/dev-probe.epss.ucla.edu\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=228"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}