Loading…
Chromium isotopes identify the extraterrestrial component in impactites from Dhala impact structure, India
The Dhala structure in north‐central India is a confirmed complex impact structure of Paleoproterozoic age. The presence of an extraterrestrial component in impactites from the Dhala structure was recognized by geochemical analyses of highly siderophile elements and Os isotopic compositions; however...
Saved in:
Published in: | Meteoritics & planetary science 2023-05, Vol.58 (5), p.722-736 |
---|---|
Main Authors: | , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
cited_by | cdi_FETCH-LOGICAL-a3602-2fa359580c216dc6c9bb143e01245c7ba6335916a712bc77a537701b5d53c2423 |
---|---|
cites | cdi_FETCH-LOGICAL-a3602-2fa359580c216dc6c9bb143e01245c7ba6335916a712bc77a537701b5d53c2423 |
container_end_page | 736 |
container_issue | 5 |
container_start_page | 722 |
container_title | Meteoritics & planetary science |
container_volume | 58 |
creator | Anand, Aryavart Singh, Anuj Kumar Mezger, Klaus Pati, Jayanta Kumar |
description | The Dhala structure in north‐central India is a confirmed complex impact structure of Paleoproterozoic age. The presence of an extraterrestrial component in impactites from the Dhala structure was recognized by geochemical analyses of highly siderophile elements and Os isotopic compositions; however, the impactor type has remained unidentified. This study uses Cr isotope systematics to identify the type of projectile involved in the formation of the Dhala structure. Unlike the composition of siderophile elements (e.g., Ni, Cr, Co, and platinum group elements) and their inter‐element ratios that may get compromised due to the extreme energy generated during an impact, Cr isotopes retain the distinct composition of the impactor. The distinct ε54Cr value of −0.31 ± 0.09 for a Dhala impact melt breccia sample (D6‐57) indicates inheritance from an impactor originating within the non‐carbonaceous reservoir, that is, the inner Solar System. Based on the Ni/Cr ratio, Os abundance, and Cr isotopic composition of the samples, the impactor is constrained to be of ureilite type. Binary mixing calculations also indicate contamination of the target rock by 0.1–0.3 wt% of material from a ureilite‐like impactor. Together with the previously identified impactors that formed El'gygytgyn, Zhamanshin, and Lonar impact structures, the Cr isotopic compositions of the Dhala impactites argue for a much more diverse source of the objects that collided with the Earth over its geological history than has been supposed previously. |
doi_str_mv | 10.1111/maps.13982 |
format | article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_journals_2813994139</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2813994139</sourcerecordid><originalsourceid>FETCH-LOGICAL-a3602-2fa359580c216dc6c9bb143e01245c7ba6335916a712bc77a537701b5d53c2423</originalsourceid><addsrcrecordid>eNp9kE1LxDAQhoMouK5e_AUBb2LXfDRNc1zWT1hRUM8hTVM2S9vUJEX335u1ezaHyTDzvDPDC8AlRguc3m2nhrDAVJTkCMywyFnGMELHKUdlkQnKxSk4C2GLEGWY5jOwXW286-zYQRtcdIMJ0Namj7bZwbgx0PxEr6Lx3oTorWqhdt3g-kRA20PbDUpHG5OqSWPg3Ua16lCFSTDqOHpzA5_72qpzcNKoNpiLwz8Hnw_3H6unbP36-LxarjNFC0Qy0ijKBCuRJriodaFFVeGcGoRJzjSvVEFTHxeKY1JpzhWjnCNcsZpRTXJC5-Bqmjt49zWmu-XWjb5PKyUpkzciTyFR1xOlvQvBm0YO3nbK7yRGcu-l3Hsp_7xMMJ7gb9ua3T-kfFm-vU-aX611d7k</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2813994139</pqid></control><display><type>article</type><title>Chromium isotopes identify the extraterrestrial component in impactites from Dhala impact structure, India</title><source>Wiley-Blackwell Read & Publish Collection</source><creator>Anand, Aryavart ; Singh, Anuj Kumar ; Mezger, Klaus ; Pati, Jayanta Kumar</creator><creatorcontrib>Anand, Aryavart ; Singh, Anuj Kumar ; Mezger, Klaus ; Pati, Jayanta Kumar</creatorcontrib><description>The Dhala structure in north‐central India is a confirmed complex impact structure of Paleoproterozoic age. The presence of an extraterrestrial component in impactites from the Dhala structure was recognized by geochemical analyses of highly siderophile elements and Os isotopic compositions; however, the impactor type has remained unidentified. This study uses Cr isotope systematics to identify the type of projectile involved in the formation of the Dhala structure. Unlike the composition of siderophile elements (e.g., Ni, Cr, Co, and platinum group elements) and their inter‐element ratios that may get compromised due to the extreme energy generated during an impact, Cr isotopes retain the distinct composition of the impactor. The distinct ε54Cr value of −0.31 ± 0.09 for a Dhala impact melt breccia sample (D6‐57) indicates inheritance from an impactor originating within the non‐carbonaceous reservoir, that is, the inner Solar System. Based on the Ni/Cr ratio, Os abundance, and Cr isotopic composition of the samples, the impactor is constrained to be of ureilite type. Binary mixing calculations also indicate contamination of the target rock by 0.1–0.3 wt% of material from a ureilite‐like impactor. Together with the previously identified impactors that formed El'gygytgyn, Zhamanshin, and Lonar impact structures, the Cr isotopic compositions of the Dhala impactites argue for a much more diverse source of the objects that collided with the Earth over its geological history than has been supposed previously.</description><identifier>ISSN: 1086-9379</identifier><identifier>EISSN: 1945-5100</identifier><identifier>DOI: 10.1111/maps.13982</identifier><language>eng</language><publisher>Hoboken: Wiley Subscription Services, Inc</publisher><subject>Breccia ; Chromium ; Chromium isotopes ; Composition ; Impact melts ; Impactors ; Inner solar system ; Isotope composition ; Isotopes ; Osmium ; Platinum ; Projectiles ; Systematics</subject><ispartof>Meteoritics & planetary science, 2023-05, Vol.58 (5), p.722-736</ispartof><rights>2023 The Authors. published by Wiley Periodicals LLC on behalf of The Meteoritical Society.</rights><rights>2023. This article is published under http://creativecommons.org/licenses/by-nc/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a3602-2fa359580c216dc6c9bb143e01245c7ba6335916a712bc77a537701b5d53c2423</citedby><cites>FETCH-LOGICAL-a3602-2fa359580c216dc6c9bb143e01245c7ba6335916a712bc77a537701b5d53c2423</cites><orcidid>0000-0003-3760-0862 ; 0000-0002-9826-2097 ; 0000-0003-2764-7499 ; 0000-0002-2443-8539</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Anand, Aryavart</creatorcontrib><creatorcontrib>Singh, Anuj Kumar</creatorcontrib><creatorcontrib>Mezger, Klaus</creatorcontrib><creatorcontrib>Pati, Jayanta Kumar</creatorcontrib><title>Chromium isotopes identify the extraterrestrial component in impactites from Dhala impact structure, India</title><title>Meteoritics & planetary science</title><description>The Dhala structure in north‐central India is a confirmed complex impact structure of Paleoproterozoic age. The presence of an extraterrestrial component in impactites from the Dhala structure was recognized by geochemical analyses of highly siderophile elements and Os isotopic compositions; however, the impactor type has remained unidentified. This study uses Cr isotope systematics to identify the type of projectile involved in the formation of the Dhala structure. Unlike the composition of siderophile elements (e.g., Ni, Cr, Co, and platinum group elements) and their inter‐element ratios that may get compromised due to the extreme energy generated during an impact, Cr isotopes retain the distinct composition of the impactor. The distinct ε54Cr value of −0.31 ± 0.09 for a Dhala impact melt breccia sample (D6‐57) indicates inheritance from an impactor originating within the non‐carbonaceous reservoir, that is, the inner Solar System. Based on the Ni/Cr ratio, Os abundance, and Cr isotopic composition of the samples, the impactor is constrained to be of ureilite type. Binary mixing calculations also indicate contamination of the target rock by 0.1–0.3 wt% of material from a ureilite‐like impactor. Together with the previously identified impactors that formed El'gygytgyn, Zhamanshin, and Lonar impact structures, the Cr isotopic compositions of the Dhala impactites argue for a much more diverse source of the objects that collided with the Earth over its geological history than has been supposed previously.</description><subject>Breccia</subject><subject>Chromium</subject><subject>Chromium isotopes</subject><subject>Composition</subject><subject>Impact melts</subject><subject>Impactors</subject><subject>Inner solar system</subject><subject>Isotope composition</subject><subject>Isotopes</subject><subject>Osmium</subject><subject>Platinum</subject><subject>Projectiles</subject><subject>Systematics</subject><issn>1086-9379</issn><issn>1945-5100</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>24P</sourceid><recordid>eNp9kE1LxDAQhoMouK5e_AUBb2LXfDRNc1zWT1hRUM8hTVM2S9vUJEX335u1ezaHyTDzvDPDC8AlRguc3m2nhrDAVJTkCMywyFnGMELHKUdlkQnKxSk4C2GLEGWY5jOwXW286-zYQRtcdIMJ0Namj7bZwbgx0PxEr6Lx3oTorWqhdt3g-kRA20PbDUpHG5OqSWPg3Ua16lCFSTDqOHpzA5_72qpzcNKoNpiLwz8Hnw_3H6unbP36-LxarjNFC0Qy0ijKBCuRJriodaFFVeGcGoRJzjSvVEFTHxeKY1JpzhWjnCNcsZpRTXJC5-Bqmjt49zWmu-XWjb5PKyUpkzciTyFR1xOlvQvBm0YO3nbK7yRGcu-l3Hsp_7xMMJ7gb9ua3T-kfFm-vU-aX611d7k</recordid><startdate>202305</startdate><enddate>202305</enddate><creator>Anand, Aryavart</creator><creator>Singh, Anuj Kumar</creator><creator>Mezger, Klaus</creator><creator>Pati, Jayanta Kumar</creator><general>Wiley Subscription Services, Inc</general><scope>24P</scope><scope>WIN</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0003-3760-0862</orcidid><orcidid>https://orcid.org/0000-0002-9826-2097</orcidid><orcidid>https://orcid.org/0000-0003-2764-7499</orcidid><orcidid>https://orcid.org/0000-0002-2443-8539</orcidid></search><sort><creationdate>202305</creationdate><title>Chromium isotopes identify the extraterrestrial component in impactites from Dhala impact structure, India</title><author>Anand, Aryavart ; Singh, Anuj Kumar ; Mezger, Klaus ; Pati, Jayanta Kumar</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a3602-2fa359580c216dc6c9bb143e01245c7ba6335916a712bc77a537701b5d53c2423</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Breccia</topic><topic>Chromium</topic><topic>Chromium isotopes</topic><topic>Composition</topic><topic>Impact melts</topic><topic>Impactors</topic><topic>Inner solar system</topic><topic>Isotope composition</topic><topic>Isotopes</topic><topic>Osmium</topic><topic>Platinum</topic><topic>Projectiles</topic><topic>Systematics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Anand, Aryavart</creatorcontrib><creatorcontrib>Singh, Anuj Kumar</creatorcontrib><creatorcontrib>Mezger, Klaus</creatorcontrib><creatorcontrib>Pati, Jayanta Kumar</creatorcontrib><collection>Wiley Online Library Open Access</collection><collection>Wiley Online Library Free Content</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Meteoritics & planetary science</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Anand, Aryavart</au><au>Singh, Anuj Kumar</au><au>Mezger, Klaus</au><au>Pati, Jayanta Kumar</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Chromium isotopes identify the extraterrestrial component in impactites from Dhala impact structure, India</atitle><jtitle>Meteoritics & planetary science</jtitle><date>2023-05</date><risdate>2023</risdate><volume>58</volume><issue>5</issue><spage>722</spage><epage>736</epage><pages>722-736</pages><issn>1086-9379</issn><eissn>1945-5100</eissn><abstract>The Dhala structure in north‐central India is a confirmed complex impact structure of Paleoproterozoic age. The presence of an extraterrestrial component in impactites from the Dhala structure was recognized by geochemical analyses of highly siderophile elements and Os isotopic compositions; however, the impactor type has remained unidentified. This study uses Cr isotope systematics to identify the type of projectile involved in the formation of the Dhala structure. Unlike the composition of siderophile elements (e.g., Ni, Cr, Co, and platinum group elements) and their inter‐element ratios that may get compromised due to the extreme energy generated during an impact, Cr isotopes retain the distinct composition of the impactor. The distinct ε54Cr value of −0.31 ± 0.09 for a Dhala impact melt breccia sample (D6‐57) indicates inheritance from an impactor originating within the non‐carbonaceous reservoir, that is, the inner Solar System. Based on the Ni/Cr ratio, Os abundance, and Cr isotopic composition of the samples, the impactor is constrained to be of ureilite type. Binary mixing calculations also indicate contamination of the target rock by 0.1–0.3 wt% of material from a ureilite‐like impactor. Together with the previously identified impactors that formed El'gygytgyn, Zhamanshin, and Lonar impact structures, the Cr isotopic compositions of the Dhala impactites argue for a much more diverse source of the objects that collided with the Earth over its geological history than has been supposed previously.</abstract><cop>Hoboken</cop><pub>Wiley Subscription Services, Inc</pub><doi>10.1111/maps.13982</doi><tpages>736</tpages><orcidid>https://orcid.org/0000-0003-3760-0862</orcidid><orcidid>https://orcid.org/0000-0002-9826-2097</orcidid><orcidid>https://orcid.org/0000-0003-2764-7499</orcidid><orcidid>https://orcid.org/0000-0002-2443-8539</orcidid><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 1086-9379 |
ispartof | Meteoritics & planetary science, 2023-05, Vol.58 (5), p.722-736 |
issn | 1086-9379 1945-5100 |
language | eng |
recordid | cdi_proquest_journals_2813994139 |
source | Wiley-Blackwell Read & Publish Collection |
subjects | Breccia Chromium Chromium isotopes Composition Impact melts Impactors Inner solar system Isotope composition Isotopes Osmium Platinum Projectiles Systematics |
title | Chromium isotopes identify the extraterrestrial component in impactites from Dhala impact structure, India |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-29T18%3A30%3A47IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Chromium%20isotopes%20identify%20the%20extraterrestrial%20component%20in%20impactites%20from%20Dhala%20impact%20structure,%20India&rft.jtitle=Meteoritics%20&%20planetary%20science&rft.au=Anand,%20Aryavart&rft.date=2023-05&rft.volume=58&rft.issue=5&rft.spage=722&rft.epage=736&rft.pages=722-736&rft.issn=1086-9379&rft.eissn=1945-5100&rft_id=info:doi/10.1111/maps.13982&rft_dat=%3Cproquest_cross%3E2813994139%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-a3602-2fa359580c216dc6c9bb143e01245c7ba6335916a712bc77a537701b5d53c2423%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2813994139&rft_id=info:pmid/&rfr_iscdi=true |