{"id":28681,"date":"2021-09-02T08:42:35","date_gmt":"2021-09-02T06:42:35","guid":{"rendered":"https:\/\/karmaka.de\/?p=28681"},"modified":"2021-09-02T08:42:36","modified_gmt":"2021-09-02T06:42:36","slug":"noble-gases-and-nitrogen-in-cv3-chondrite-bukhara","status":"publish","type":"post","link":"https:\/\/karmaka.de\/?p=28681","title":{"rendered":"Noble gases and nitrogen in CV3 chondrite Bukhara"},"content":{"rendered":"\n<p>Ramakant R. Mahajan, Shuhrat A. Ehgamberdiev, Sekhar Naik<\/p>\n\n\n\n<p>Planetary and Space Science<br>In Press, Journal Pre-proof, Available online 1 September 2021<\/p>\n\n\n\n<p><a href=\"https:\/\/www.sciencedirect.com\/science\/article\/abs\/pii\/S0032063321001732\" target=\"_blank\" rel=\"noreferrer noopener\"><strong>LINK<\/strong><\/a><\/p>\n\n\n\n<p>&#8220;Highlights<\/p>\n\n\n\n<p>\u2022 Noble gas and nitrogen isotopic were studied in CV3 chondrite Bukhara.<br>\u2022 We calculate cosmic ray exposure age of 22.6\u202f\u00b1\u202f4.0\u202fMa from noble gases.<br>\u2022 Trapped nitrogen is distinct compared with CV3 chondrites.&#8221;<\/p>\n\n\n\n<p class=\"justify-text\">&#8220;We investigated noble gas (He, Ne, Ar, Kr and Xe) and nitrogen isotopic composition in the carbonaceous chondrite Bukhara (CV3). This is the first report of N and noble gases measured in the same aliquot of bulk sample among the CV3 chondrites. Isotopic compositions of noble gases are mixtures of solar wind and Q-gases. We derive cosmic ray exposure (CRE) age of 22.6\u202f\u00b1\u202f4.0\u202fMa from cosmogenic 21Ne and 38Ar for Bukhara. Nitrogen abundance observed in Bukhara is lowest compared with the data from CV3 chondrites. We estimate the trapped nitrogen composition of \u03b415N = + 10.9 \u00b1 1.6\u2030 for Bukhara, distinct from average (\u03b415N\u202f=\u202f- 16.3\u202f\u00b1\u202f1.5\u2030) in the bulk CV3 chondrites. Bukhara shows signature of heavy nitrogen, which is distinct than the solar wind (SW) and Q-gas. Trapped nitrogen is mixture of the components, SW, Q and comet. It is observed that there is no correlation of nitrogen composition with N content in the CV3 chondrites.&#8221;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Ramakant R. Mahajan, Shuhrat A. Ehgamberdiev, Sekhar Naik Planetary and Space ScienceIn Press, Journal Pre-proof, Available online 1 September 2021 LINK &#8220;Highlights \u2022 Noble gas and nitrogen isotopic were studied in CV3 chondrite Bukhara.\u2022 We&#8230;<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[9,69,14,506],"tags":[6097,3273,1849,1812,2346,1270],"_links":{"self":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/28681"}],"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=28681"}],"version-history":[{"count":1,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/28681\/revisions"}],"predecessor-version":[{"id":28682,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/28681\/revisions\/28682"}],"wp:attachment":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=28681"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=28681"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=28681"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}