Noble Gases in Stratospheric Dust Particles: Confirmation of Extraterrestrial Origin
Noble gas elemental and isotopic ratios were measured in a group of 13 ``chondritic'' stratospheric dust particles. Neon and argon are present in ``solar'' proportions; xenon appears to be dominated by contributions from ``planetary'' sources. The apparent xenon concent...
Gespeichert in:
Veröffentlicht in: | Science (American Association for the Advancement of Science) 1981-01, Vol.211 (4480), p.383-386 |
---|---|
Hauptverfasser: | , , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 386 |
---|---|
container_issue | 4480 |
container_start_page | 383 |
container_title | Science (American Association for the Advancement of Science) |
container_volume | 211 |
creator | Hudson, B. Flynn, G. J. Fraundorf, P. Hohenberg, C. M. Shirck, J. |
description | Noble gas elemental and isotopic ratios were measured in a group of 13 ``chondritic'' stratospheric dust particles. Neon and argon are present in ``solar'' proportions; xenon appears to be dominated by contributions from ``planetary'' sources. The apparent xenon concentration is higher than that measured in any bulk meteorite, approaching the concentration found in the noble gas-rich, acid-insoluble residues from carbonaceous chondrites. |
doi_str_mv | 10.1126/science.211.4480.383 |
format | Article |
fullrecord | <record><control><sourceid>jstor_osti_</sourceid><recordid>TN_cdi_proquest_miscellaneous_733188620</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><jstor_id>1685349</jstor_id><sourcerecordid>1685349</sourcerecordid><originalsourceid>FETCH-LOGICAL-a405t-d8717e3bf4f31cb503394db3023c450c678ae1f7108311d6a7bb3e95e3e382623</originalsourceid><addsrcrecordid>eNpFkE1vEzEQhi0EomngH1TI4sJpU8-O1_ZyQ6FfUkWRKGfL68xSV5t1sB0J_n0dJVJPc3ifd2b0MHYBYgXQqsvsA82eVi3ASkojVmjwDVuA6LumbwW-ZQshUDVG6O6Mnef8LETNenzPzkBraVoNC_b4Iw4T8RuXKfMw818luRLz7olS8Pz7Phf-06US_ET5K1_HeQxp60qIM48jv_p3wCklyiUFN_GHFP6E-QN7N7op08fTXLLf11eP69vm_uHmbv3tvnFSdKXZGA2acBjliOCHTiD2cjOgaNHLTniljSMYNQiDABvl9DAg9R0hoWlVi0v2-bg35hJsFVLIP_k4z-SLVQoVdFihL0dol-LffX3UbkP2NE1uprjPViOCMaoaWzJ5JH2KOSca7S6FrUv_LQh7cG5Pzm11bg_ObXVea59OB_bDljavpZPkClwcgedcYnrNlelQ9vgCSTaHvQ</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>733188620</pqid></control><display><type>article</type><title>Noble Gases in Stratospheric Dust Particles: Confirmation of Extraterrestrial Origin</title><source>American Association for the Advancement of Science</source><source>Jstor Complete Legacy</source><creator>Hudson, B. ; Flynn, G. J. ; Fraundorf, P. ; Hohenberg, C. M. ; Shirck, J.</creator><creatorcontrib>Hudson, B. ; Flynn, G. J. ; Fraundorf, P. ; Hohenberg, C. M. ; Shirck, J. ; Washington Univ., St. Louis, MO</creatorcontrib><description>Noble gas elemental and isotopic ratios were measured in a group of 13 ``chondritic'' stratospheric dust particles. Neon and argon are present in ``solar'' proportions; xenon appears to be dominated by contributions from ``planetary'' sources. The apparent xenon concentration is higher than that measured in any bulk meteorite, approaching the concentration found in the noble gas-rich, acid-insoluble residues from carbonaceous chondrites.</description><identifier>ISSN: 0036-8075</identifier><identifier>EISSN: 1095-9203</identifier><identifier>DOI: 10.1126/science.211.4480.383</identifier><identifier>PMID: 17748271</identifier><language>eng</language><publisher>United States: The American Association for the Advancement of Science</publisher><subject>640107 -- Astrophysics & Cosmology-- Planetary Phenomena ; ARGON ; Atmospherics ; Average linear density ; CHEMICAL COMPOSITION ; CHONDRITES ; CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ; COSMIC GASES ; DATA ; Dunes ; DUSTS ; EARTH ATMOSPHERE ; ELEMENTS ; EXPERIMENTAL DATA ; FLUIDS ; GASES ; INFORMATION ; ISOTOPE RATIO ; METEORITES ; NEON ; Noble gases ; NONMETALS ; NUMERICAL DATA ; Particle mass ; PARTICLE SIZE ; RARE GASES ; Sand ; SIZE ; Solar wind ; STONE METEORITES 640200 -- Atmospheric Physics ; STRATOSPHERE ; XENON</subject><ispartof>Science (American Association for the Advancement of Science), 1981-01, Vol.211 (4480), p.383-386</ispartof><rights>Copyright 1981 The American Association for the Advancement of Science</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a405t-d8717e3bf4f31cb503394db3023c450c678ae1f7108311d6a7bb3e95e3e382623</citedby><cites>FETCH-LOGICAL-a405t-d8717e3bf4f31cb503394db3023c450c678ae1f7108311d6a7bb3e95e3e382623</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.jstor.org/stable/pdf/1685349$$EPDF$$P50$$Gjstor$$H</linktopdf><linktohtml>$$Uhttps://www.jstor.org/stable/1685349$$EHTML$$P50$$Gjstor$$H</linktohtml><link.rule.ids>314,776,780,799,881,2871,2872,27901,27902,57992,58225</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/17748271$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/6636153$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Hudson, B.</creatorcontrib><creatorcontrib>Flynn, G. J.</creatorcontrib><creatorcontrib>Fraundorf, P.</creatorcontrib><creatorcontrib>Hohenberg, C. M.</creatorcontrib><creatorcontrib>Shirck, J.</creatorcontrib><creatorcontrib>Washington Univ., St. Louis, MO</creatorcontrib><title>Noble Gases in Stratospheric Dust Particles: Confirmation of Extraterrestrial Origin</title><title>Science (American Association for the Advancement of Science)</title><addtitle>Science</addtitle><description>Noble gas elemental and isotopic ratios were measured in a group of 13 ``chondritic'' stratospheric dust particles. Neon and argon are present in ``solar'' proportions; xenon appears to be dominated by contributions from ``planetary'' sources. The apparent xenon concentration is higher than that measured in any bulk meteorite, approaching the concentration found in the noble gas-rich, acid-insoluble residues from carbonaceous chondrites.</description><subject>640107 -- Astrophysics & Cosmology-- Planetary Phenomena</subject><subject>ARGON</subject><subject>Atmospherics</subject><subject>Average linear density</subject><subject>CHEMICAL COMPOSITION</subject><subject>CHONDRITES</subject><subject>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</subject><subject>COSMIC GASES</subject><subject>DATA</subject><subject>Dunes</subject><subject>DUSTS</subject><subject>EARTH ATMOSPHERE</subject><subject>ELEMENTS</subject><subject>EXPERIMENTAL DATA</subject><subject>FLUIDS</subject><subject>GASES</subject><subject>INFORMATION</subject><subject>ISOTOPE RATIO</subject><subject>METEORITES</subject><subject>NEON</subject><subject>Noble gases</subject><subject>NONMETALS</subject><subject>NUMERICAL DATA</subject><subject>Particle mass</subject><subject>PARTICLE SIZE</subject><subject>RARE GASES</subject><subject>Sand</subject><subject>SIZE</subject><subject>Solar wind</subject><subject>STONE METEORITES 640200 -- Atmospheric Physics</subject><subject>STRATOSPHERE</subject><subject>XENON</subject><issn>0036-8075</issn><issn>1095-9203</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1981</creationdate><recordtype>article</recordtype><recordid>eNpFkE1vEzEQhi0EomngH1TI4sJpU8-O1_ZyQ6FfUkWRKGfL68xSV5t1sB0J_n0dJVJPc3ifd2b0MHYBYgXQqsvsA82eVi3ASkojVmjwDVuA6LumbwW-ZQshUDVG6O6Mnef8LETNenzPzkBraVoNC_b4Iw4T8RuXKfMw818luRLz7olS8Pz7Phf-06US_ET5K1_HeQxp60qIM48jv_p3wCklyiUFN_GHFP6E-QN7N7op08fTXLLf11eP69vm_uHmbv3tvnFSdKXZGA2acBjliOCHTiD2cjOgaNHLTniljSMYNQiDABvl9DAg9R0hoWlVi0v2-bg35hJsFVLIP_k4z-SLVQoVdFihL0dol-LffX3UbkP2NE1uprjPViOCMaoaWzJ5JH2KOSca7S6FrUv_LQh7cG5Pzm11bg_ObXVea59OB_bDljavpZPkClwcgedcYnrNlelQ9vgCSTaHvQ</recordid><startdate>19810123</startdate><enddate>19810123</enddate><creator>Hudson, B.</creator><creator>Flynn, G. J.</creator><creator>Fraundorf, P.</creator><creator>Hohenberg, C. M.</creator><creator>Shirck, J.</creator><general>The American Association for the Advancement of Science</general><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7X8</scope><scope>OTOTI</scope></search><sort><creationdate>19810123</creationdate><title>Noble Gases in Stratospheric Dust Particles: Confirmation of Extraterrestrial Origin</title><author>Hudson, B. ; Flynn, G. J. ; Fraundorf, P. ; Hohenberg, C. M. ; Shirck, J.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a405t-d8717e3bf4f31cb503394db3023c450c678ae1f7108311d6a7bb3e95e3e382623</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1981</creationdate><topic>640107 -- Astrophysics & Cosmology-- Planetary Phenomena</topic><topic>ARGON</topic><topic>Atmospherics</topic><topic>Average linear density</topic><topic>CHEMICAL COMPOSITION</topic><topic>CHONDRITES</topic><topic>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</topic><topic>COSMIC GASES</topic><topic>DATA</topic><topic>Dunes</topic><topic>DUSTS</topic><topic>EARTH ATMOSPHERE</topic><topic>ELEMENTS</topic><topic>EXPERIMENTAL DATA</topic><topic>FLUIDS</topic><topic>GASES</topic><topic>INFORMATION</topic><topic>ISOTOPE RATIO</topic><topic>METEORITES</topic><topic>NEON</topic><topic>Noble gases</topic><topic>NONMETALS</topic><topic>NUMERICAL DATA</topic><topic>Particle mass</topic><topic>PARTICLE SIZE</topic><topic>RARE GASES</topic><topic>Sand</topic><topic>SIZE</topic><topic>Solar wind</topic><topic>STONE METEORITES 640200 -- Atmospheric Physics</topic><topic>STRATOSPHERE</topic><topic>XENON</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Hudson, B.</creatorcontrib><creatorcontrib>Flynn, G. J.</creatorcontrib><creatorcontrib>Fraundorf, P.</creatorcontrib><creatorcontrib>Hohenberg, C. M.</creatorcontrib><creatorcontrib>Shirck, J.</creatorcontrib><creatorcontrib>Washington Univ., St. Louis, MO</creatorcontrib><collection>PubMed</collection><collection>CrossRef</collection><collection>MEDLINE - Academic</collection><collection>OSTI.GOV</collection><jtitle>Science (American Association for the Advancement of Science)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Hudson, B.</au><au>Flynn, G. J.</au><au>Fraundorf, P.</au><au>Hohenberg, C. M.</au><au>Shirck, J.</au><aucorp>Washington Univ., St. Louis, MO</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Noble Gases in Stratospheric Dust Particles: Confirmation of Extraterrestrial Origin</atitle><jtitle>Science (American Association for the Advancement of Science)</jtitle><addtitle>Science</addtitle><date>1981-01-23</date><risdate>1981</risdate><volume>211</volume><issue>4480</issue><spage>383</spage><epage>386</epage><pages>383-386</pages><issn>0036-8075</issn><eissn>1095-9203</eissn><abstract>Noble gas elemental and isotopic ratios were measured in a group of 13 ``chondritic'' stratospheric dust particles. Neon and argon are present in ``solar'' proportions; xenon appears to be dominated by contributions from ``planetary'' sources. The apparent xenon concentration is higher than that measured in any bulk meteorite, approaching the concentration found in the noble gas-rich, acid-insoluble residues from carbonaceous chondrites.</abstract><cop>United States</cop><pub>The American Association for the Advancement of Science</pub><pmid>17748271</pmid><doi>10.1126/science.211.4480.383</doi><tpages>4</tpages></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0036-8075 |
ispartof | Science (American Association for the Advancement of Science), 1981-01, Vol.211 (4480), p.383-386 |
issn | 0036-8075 1095-9203 |
language | eng |
recordid | cdi_proquest_miscellaneous_733188620 |
source | American Association for the Advancement of Science; Jstor Complete Legacy |
subjects | 640107 -- Astrophysics & Cosmology-- Planetary Phenomena ARGON Atmospherics Average linear density CHEMICAL COMPOSITION CHONDRITES CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS COSMIC GASES DATA Dunes DUSTS EARTH ATMOSPHERE ELEMENTS EXPERIMENTAL DATA FLUIDS GASES INFORMATION ISOTOPE RATIO METEORITES NEON Noble gases NONMETALS NUMERICAL DATA Particle mass PARTICLE SIZE RARE GASES Sand SIZE Solar wind STONE METEORITES 640200 -- Atmospheric Physics STRATOSPHERE XENON |
title | Noble Gases in Stratospheric Dust Particles: Confirmation of Extraterrestrial Origin |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-06T14%3A44%3A07IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-jstor_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Noble%20Gases%20in%20Stratospheric%20Dust%20Particles:%20Confirmation%20of%20Extraterrestrial%20Origin&rft.jtitle=Science%20(American%20Association%20for%20the%20Advancement%20of%20Science)&rft.au=Hudson,%20B.&rft.aucorp=Washington%20Univ.,%20St.%20Louis,%20MO&rft.date=1981-01-23&rft.volume=211&rft.issue=4480&rft.spage=383&rft.epage=386&rft.pages=383-386&rft.issn=0036-8075&rft.eissn=1095-9203&rft_id=info:doi/10.1126/science.211.4480.383&rft_dat=%3Cjstor_osti_%3E1685349%3C/jstor_osti_%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=733188620&rft_id=info:pmid/17748271&rft_jstor_id=1685349&rfr_iscdi=true |