Samples of Stars beyond the Solar System: Silicate Grains in Interplanetary Dust
We have identified six circumstellar silicate grains within interplanetary dust particles (IDPs). Their extrasolar origins are demonstrated by their extremely anomalous oxygen isotopic compositions. Three $^{17}O-rich$ grains appear to originate from red giant or asymptotic giant branch stars. One $...
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Veröffentlicht in: | Science (American Association for the Advancement of Science) 2003-04, Vol.300 (5616), p.105-108 |
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description | We have identified six circumstellar silicate grains within interplanetary dust particles (IDPs). Their extrasolar origins are demonstrated by their extremely anomalous oxygen isotopic compositions. Three $^{17}O-rich$ grains appear to originate from red giant or asymptotic giant branch stars. One $^{16}O-rich$ grain may be from a metal-poor star. Two $^{16}O-poor$ grains have unknown stellar sources. One of the grains is forsterite, and two are amorphous silicate "GEMS" (glass with embedded metal and sulfides), which is consistent with astronomical identifications of crystalline and amorphous silicates in the outflows of evolved stars. These observations suggest cometary origins of these IDPs and underscore the perplexing absence of silicates among circumstellar dust grains from meteorites. |
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Their extrasolar origins are demonstrated by their extremely anomalous oxygen isotopic compositions. Three $^{17}O-rich$ grains appear to originate from red giant or asymptotic giant branch stars. One $^{16}O-rich$ grain may be from a metal-poor star. Two $^{16}O-poor$ grains have unknown stellar sources. One of the grains is forsterite, and two are amorphous silicate "GEMS" (glass with embedded metal and sulfides), which is consistent with astronomical identifications of crystalline and amorphous silicates in the outflows of evolved stars. These observations suggest cometary origins of these IDPs and underscore the perplexing absence of silicates among circumstellar dust grains from meteorites.</description><identifier>ISSN: 0036-8075</identifier><identifier>EISSN: 1095-9203</identifier><identifier>DOI: 10.1126/science.1080576</identifier><identifier>PMID: 12610229</identifier><identifier>CODEN: SCIEAS</identifier><language>eng</language><publisher>Washington, DC: American Association for the Advancement of Science</publisher><subject>Astronomical Phenomena ; Astronomy ; Carbon ; Chemical composition ; Circumstellar grains ; Circumstellar shells, clouds, and expanding envelopes. Circumstellar masers ; Cosmic Dust ; Dust ; Earth, ocean, space ; Exact sciences and technology ; Gem stones ; Interplanetary dust ; Interplanetary gas and dust (including gegenschein and zodiacal light) ; Interplanetary space ; Materials ; Meteorites ; Meteoroids ; Meteors, meteoroids and meteor streams ; Mineralogy ; Oxygen ; Oxygen Isotopes ; Silica ; Silicates ; Soil structure ; Solar System ; Solar systems ; Stars ; Stars & galaxies ; Stellar characteristics and properties ; Temperature</subject><ispartof>Science (American Association for the Advancement of Science), 2003-04, Vol.300 (5616), p.105-108</ispartof><rights>Copyright 2003 American Association for the Advancement of Science</rights><rights>2003 INIST-CNRS</rights><rights>COPYRIGHT 2003 American Association for the Advancement of Science</rights><rights>COPYRIGHT 2003 American Association for the Advancement of Science</rights><rights>Copyright American Association for the Advancement of Science Apr 4, 2003</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a907t-eddbafa0c387086f36d3517bb1b044e1ba515201c21d40752e8614384cd257b13</citedby><cites>FETCH-LOGICAL-a907t-eddbafa0c387086f36d3517bb1b044e1ba515201c21d40752e8614384cd257b13</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.jstor.org/stable/pdf/3834309$$EPDF$$P50$$Gjstor$$H</linktopdf><linktohtml>$$Uhttps://www.jstor.org/stable/3834309$$EHTML$$P50$$Gjstor$$H</linktohtml><link.rule.ids>314,776,780,799,2871,2872,27901,27902,57992,58225</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=14733968$$DView record in Pascal Francis$$Hfree_for_read</backlink><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/12610229$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Messenger, Scott</creatorcontrib><creatorcontrib>Keller, Lindsay P.</creatorcontrib><creatorcontrib>Stadermann, Frank J.</creatorcontrib><creatorcontrib>Walker, Robert M.</creatorcontrib><creatorcontrib>Zinner, Ernst</creatorcontrib><title>Samples of Stars beyond the Solar System: Silicate Grains in Interplanetary Dust</title><title>Science (American Association for the Advancement of Science)</title><addtitle>Science</addtitle><description>We have identified six circumstellar silicate grains within interplanetary dust particles (IDPs). Their extrasolar origins are demonstrated by their extremely anomalous oxygen isotopic compositions. Three $^{17}O-rich$ grains appear to originate from red giant or asymptotic giant branch stars. One $^{16}O-rich$ grain may be from a metal-poor star. Two $^{16}O-poor$ grains have unknown stellar sources. One of the grains is forsterite, and two are amorphous silicate "GEMS" (glass with embedded metal and sulfides), which is consistent with astronomical identifications of crystalline and amorphous silicates in the outflows of evolved stars. These observations suggest cometary origins of these IDPs and underscore the perplexing absence of silicates among circumstellar dust grains from meteorites.</description><subject>Astronomical Phenomena</subject><subject>Astronomy</subject><subject>Carbon</subject><subject>Chemical composition</subject><subject>Circumstellar grains</subject><subject>Circumstellar shells, clouds, and expanding envelopes. Circumstellar masers</subject><subject>Cosmic Dust</subject><subject>Dust</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Gem stones</subject><subject>Interplanetary dust</subject><subject>Interplanetary gas and dust (including gegenschein and zodiacal light)</subject><subject>Interplanetary space</subject><subject>Materials</subject><subject>Meteorites</subject><subject>Meteoroids</subject><subject>Meteors, meteoroids and meteor streams</subject><subject>Mineralogy</subject><subject>Oxygen</subject><subject>Oxygen Isotopes</subject><subject>Silica</subject><subject>Silicates</subject><subject>Soil structure</subject><subject>Solar System</subject><subject>Solar systems</subject><subject>Stars</subject><subject>Stars & galaxies</subject><subject>Stellar characteristics and properties</subject><subject>Temperature</subject><issn>0036-8075</issn><issn>1095-9203</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2003</creationdate><recordtype>article</recordtype><sourceid>EIF</sourceid><sourceid>8G5</sourceid><sourceid>BEC</sourceid><sourceid>BENPR</sourceid><sourceid>GUQSH</sourceid><sourceid>M2O</sourceid><recordid>eNqN0--L0zAYB_AiijdPX_tGpBx44ovu8jRpk_junDoHwwlV35Y0fTo7-mMmKbj__jJWPCbDG30RaD7fJ22SJwheApkCxOmN1TV2GqdABEl4-iiYAJFJJGNCHwcTQmgaCcKTi-CZtRtC_JykT4MLHwUSx3ISfMtUu23Qhn0VZk4ZGxa467sydL8wzPpGmTDbWYft-zCrm1orh-HcqLqzYd2Fi86h2TaqQx_dhR8H654HTyrVWHwxjpfBj8-fvs--RMvVfDG7XUZKEu4iLMtCVYpoKjgRaUXTkibAiwIKwhhCoRJIYgI6hpL5P4hRpMCoYLqME14AvQzeHupuTf97QOvytrYam_3H9IPNOaMsSRgnXl7_X1JIpBAPw1gIkHBGxRgYSAb0QQiCgz8k6eHVP3DTD6bzG-iL0cQztl82OqC1ajCvu6p3Ruk1dmhU03dY1f71rS8InMVceD894f1TYlvrk4F3RwFvHP5xazVYmy-yr-fb1c_z7Yf52VbMl8c2OmV13zS4xtzft9nq2N8cvDa9tQarfGvq1t_cHEi-76d87Kd87CefeD2ey1C0WN77sYE8eDMCZbVqKqM6Xdt7xzilMt0v_ergNtb15u88FZRRIukdWOQpsw</recordid><startdate>20030404</startdate><enddate>20030404</enddate><creator>Messenger, Scott</creator><creator>Keller, Lindsay P.</creator><creator>Stadermann, Frank J.</creator><creator>Walker, Robert M.</creator><creator>Zinner, Ernst</creator><general>American Association for the Advancement of Science</general><general>The American Association for the Advancement of Science</general><scope>IQODW</scope><scope>CGR</scope><scope>CUY</scope><scope>CVF</scope><scope>ECM</scope><scope>EIF</scope><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8GL</scope><scope>IBG</scope><scope>IOV</scope><scope>ISN</scope><scope>0-V</scope><scope>3V.</scope><scope>7QF</scope><scope>7QG</scope><scope>7QL</scope><scope>7QP</scope><scope>7QQ</scope><scope>7QR</scope><scope>7SC</scope><scope>7SE</scope><scope>7SN</scope><scope>7SP</scope><scope>7SR</scope><scope>7SS</scope><scope>7T7</scope><scope>7TA</scope><scope>7TB</scope><scope>7TK</scope><scope>7TM</scope><scope>7U5</scope><scope>7U9</scope><scope>7X2</scope><scope>7X7</scope><scope>7XB</scope><scope>88A</scope><scope>88B</scope><scope>88E</scope><scope>88I</scope><scope>8AF</scope><scope>8BQ</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FH</scope><scope>8FI</scope><scope>8FJ</scope><scope>8FK</scope><scope>8G5</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AEUYN</scope><scope>AFKRA</scope><scope>ALSLI</scope><scope>ARAPS</scope><scope>ATCPS</scope><scope>AZQEC</scope><scope>BBNVY</scope><scope>BEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>C1K</scope><scope>CCPQU</scope><scope>CJNVE</scope><scope>D1I</scope><scope>DWQXO</scope><scope>F28</scope><scope>FR3</scope><scope>FYUFA</scope><scope>GHDGH</scope><scope>GNUQQ</scope><scope>GUQSH</scope><scope>H8D</scope><scope>H8G</scope><scope>H94</scope><scope>HCIFZ</scope><scope>JG9</scope><scope>JQ2</scope><scope>K9-</scope><scope>K9.</scope><scope>KB.</scope><scope>KR7</scope><scope>L6V</scope><scope>L7M</scope><scope>LK8</scope><scope>L~C</scope><scope>L~D</scope><scope>M0K</scope><scope>M0P</scope><scope>M0R</scope><scope>M0S</scope><scope>M1P</scope><scope>M2O</scope><scope>M2P</scope><scope>M7N</scope><scope>M7P</scope><scope>M7S</scope><scope>MBDVC</scope><scope>P5Z</scope><scope>P62</scope><scope>P64</scope><scope>PATMY</scope><scope>PCBAR</scope><scope>PDBOC</scope><scope>PQEDU</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>PYCSY</scope><scope>Q9U</scope><scope>R05</scope><scope>RC3</scope><scope>7TG</scope><scope>KL.</scope><scope>7X8</scope></search><sort><creationdate>20030404</creationdate><title>Samples of Stars beyond the Solar System: Silicate Grains in Interplanetary Dust</title><author>Messenger, Scott ; 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Their extrasolar origins are demonstrated by their extremely anomalous oxygen isotopic compositions. Three $^{17}O-rich$ grains appear to originate from red giant or asymptotic giant branch stars. One $^{16}O-rich$ grain may be from a metal-poor star. Two $^{16}O-poor$ grains have unknown stellar sources. One of the grains is forsterite, and two are amorphous silicate "GEMS" (glass with embedded metal and sulfides), which is consistent with astronomical identifications of crystalline and amorphous silicates in the outflows of evolved stars. These observations suggest cometary origins of these IDPs and underscore the perplexing absence of silicates among circumstellar dust grains from meteorites.</abstract><cop>Washington, DC</cop><pub>American Association for the Advancement of Science</pub><pmid>12610229</pmid><doi>10.1126/science.1080576</doi><tpages>4</tpages><oa>free_for_read</oa></addata></record> |
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subjects | Astronomical Phenomena Astronomy Carbon Chemical composition Circumstellar grains Circumstellar shells, clouds, and expanding envelopes. Circumstellar masers Cosmic Dust Dust Earth, ocean, space Exact sciences and technology Gem stones Interplanetary dust Interplanetary gas and dust (including gegenschein and zodiacal light) Interplanetary space Materials Meteorites Meteoroids Meteors, meteoroids and meteor streams Mineralogy Oxygen Oxygen Isotopes Silica Silicates Soil structure Solar System Solar systems Stars Stars & galaxies Stellar characteristics and properties Temperature |
title | Samples of Stars beyond the Solar System: Silicate Grains in Interplanetary Dust |
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