Jesenice—A new meteorite fall from Slovenia
Identifieur interne : 000E19 ( Istex/Corpus ); précédent : 000E18; suivant : 000E20Jesenice—A new meteorite fall from Slovenia
Auteurs : Addi Bischoff ; Miha Jersek ; Thomas Grau ; Breda Mirtic ; Ulrich Ott ; Jan Ku Era ; Marian Horstmann ; Matthias Laubenstein ; Siegfried Herrmann ; Zden K Anda ; Marc Weber ; Gerd HeusserSource :
- Meteoritics & Planetary Science [ 1086-9379 ] ; 2011-06.
Abstract
Abstract– On April 9, 2009, at 3:00 CEST, a very bright fireball appeared over Carinthia and the Karavanke Mountains. The meteoroid entered the atmosphere at a very steep angle and disintegrated into a large number of objects. Two main objects were seen as separate fireballs up to an altitude of approximately 5 km, and witnesses reported loud explosions. Three stones were found with a total weight of approximately 3.611 kg. The measured activity of short‐lived cosmogenic radionuclides clearly indicates that two specimens result from a very recent meteorite fall. All cosmogenic radionuclide concentrations suggest a rather small preatmospheric radius of <20 cm; a nominal cosmic‐ray exposure age based on 21Ne is approximately 4 Ma, but the noble gas and radionuclide results in combination indicate a complex irradiation. Jesenice is a highly recrystallized rock with only a few relic chondrules visible in hand specimen and thin section. The texture, the large grain size of plagioclase, and the homogeneous compositions of olivines and pyroxenes clearly indicate that Jesenice is a L6 chondrite. The bulk composition of Jesenice is very close to the published average element concentration for L ordinary chondrites. The chondrite is weakly shocked (S3) as indicated by the undulatory extinction in olivine and plagioclase and the presence of planar fractures in olivine. Being weakly shocked and with gas retention ages of >1.7 Ga (4He) and approximately 4.3 Ga (40Ar), Jesenice seems not to have been strongly affected by the catastrophic disruption of the L‐chondrite parent body approximately 500 Ma ago.
Url:
DOI: 10.1111/j.1945-5100.2011.01191.x
Links to Exploration step
ISTEX:DB8113B9614DFC9BE7681347A05B7D98CB2BA5E7Le document en format XML
<record><TEI wicri:istexFullTextTei="biblStruct"><teiHeader><fileDesc><titleStmt><title xml:lang="en">Jesenice—A new meteorite fall from Slovenia</title><author><name sortKey="Bischoff, Addi" sort="Bischoff, Addi" uniqKey="Bischoff A" first="Addi" last="Bischoff">Addi Bischoff</name><affiliation><mods:affiliation>Institut für Planetologie, Wilhelm‐Klemm‐Str. 10, 48149 Münster, Germany</mods:affiliation></affiliation></author><author><name sortKey="Jersek, Miha" sort="Jersek, Miha" uniqKey="Jersek M" first="Miha" last="Jersek">Miha Jersek</name><affiliation><mods:affiliation>Slovenian Museum of Natural History, Presernova 20, SI‐1000 Ljubljana, Slovenia</mods:affiliation></affiliation></author><author><name sortKey="Grau, Thomas" sort="Grau, Thomas" uniqKey="Grau T" first="Thomas" last="Grau">Thomas Grau</name><affiliation><mods:affiliation>European Research Center for Fireballs and Meteorites (ERFM), Puschkinstraße 23, 16321 Bernau bei Berlin, Germany</mods:affiliation></affiliation></author><author><name sortKey="Mirtic, Breda" sort="Mirtic, Breda" uniqKey="Mirtic B" first="Breda" last="Mirtic">Breda Mirtic</name><affiliation><mods:affiliation>Department of Geology, Faculty of Natural Sciences and Engineering, University of Ljubljana, SI‐1000 Ljubljana, Slovenia</mods:affiliation></affiliation></author><author><name sortKey="Ott, Ulrich" sort="Ott, Ulrich" uniqKey="Ott U" first="Ulrich" last="Ott">Ulrich Ott</name><affiliation><mods:affiliation>Abteilung Biogeochemie, Max‐Planck‐Institut für Chemie, Joh.‐J.‐Becher‐Weg 27, 55128 Mainz, Germany</mods:affiliation></affiliation></author><author><name sortKey="Ku Era, Jan" sort="Ku Era, Jan" uniqKey="Ku Era J" first="Jan" last="Ku Era">Jan Ku Era</name><affiliation><mods:affiliation>Nuclear Physics Institute, Academy of Sciences of the Czech Republic, CZ‐250 68 Řež near Prague, Czech Republic</mods:affiliation></affiliation><affiliation><mods:affiliation>Research Center Řež, Ltd., CZ‐250 68 Řež, Czech Republic</mods:affiliation></affiliation></author><author><name sortKey="Horstmann, Marian" sort="Horstmann, Marian" uniqKey="Horstmann M" first="Marian" last="Horstmann">Marian Horstmann</name><affiliation><mods:affiliation>Institut für Planetologie, Wilhelm‐Klemm‐Str. 10, 48149 Münster, Germany</mods:affiliation></affiliation></author><author><name sortKey="Laubenstein, Matthias" sort="Laubenstein, Matthias" uniqKey="Laubenstein M" first="Matthias" last="Laubenstein">Matthias Laubenstein</name><affiliation><mods:affiliation>Laboratori Nazionali del Gran Sasso – I.N.F.N., S.S.17/bis, km 18+910, I‐67010 Assergi (AQ), Italy</mods:affiliation></affiliation></author><author><name sortKey="Herrmann, Siegfried" sort="Herrmann, Siegfried" uniqKey="Herrmann S" first="Siegfried" last="Herrmann">Siegfried Herrmann</name><affiliation><mods:affiliation>Abteilung Biogeochemie, Max‐Planck‐Institut für Chemie, Joh.‐J.‐Becher‐Weg 27, 55128 Mainz, Germany</mods:affiliation></affiliation></author><author><name sortKey=" Anda, Zden K" sort=" Anda, Zden K" uniqKey=" Anda Z" first="Zden K" last=" Anda">Zden K Anda</name><affiliation><mods:affiliation>Nuclear Physics Institute, Academy of Sciences of the Czech Republic, CZ‐250 68 Řež near Prague, Czech Republic</mods:affiliation></affiliation></author><author><name sortKey="Weber, Marc" sort="Weber, Marc" uniqKey="Weber M" first="Marc" last="Weber">Marc Weber</name><affiliation><mods:affiliation>Max‐Planck‐Institut für Kernphysik, Postfach 103980, 69029 Heidelberg, Germany</mods:affiliation></affiliation></author><author><name sortKey="Heusser, Gerd" sort="Heusser, Gerd" uniqKey="Heusser G" first="Gerd" last="Heusser">Gerd Heusser</name><affiliation><mods:affiliation>Max‐Planck‐Institut für Kernphysik, Postfach 103980, 69029 Heidelberg, Germany</mods:affiliation></affiliation></author></titleStmt><publicationStmt><idno type="wicri:source">ISTEX</idno><idno type="RBID">ISTEX:DB8113B9614DFC9BE7681347A05B7D98CB2BA5E7</idno><date when="2011" year="2011">2011</date><idno type="doi">10.1111/j.1945-5100.2011.01191.x</idno><idno type="url">https://api.istex.fr/document/DB8113B9614DFC9BE7681347A05B7D98CB2BA5E7/fulltext/pdf</idno><idno type="wicri:Area/Istex/Corpus">000E19</idno><idno type="wicri:explorRef" wicri:stream="Istex" wicri:step="Corpus" wicri:corpus="ISTEX">000E19</idno></publicationStmt><sourceDesc><biblStruct><analytic><title level="a" type="main" xml:lang="en">Jesenice—A new meteorite fall from Slovenia</title><author><name sortKey="Bischoff, Addi" sort="Bischoff, Addi" uniqKey="Bischoff A" first="Addi" last="Bischoff">Addi Bischoff</name><affiliation><mods:affiliation>Institut für Planetologie, Wilhelm‐Klemm‐Str. 10, 48149 Münster, Germany</mods:affiliation></affiliation></author><author><name sortKey="Jersek, Miha" sort="Jersek, Miha" uniqKey="Jersek M" first="Miha" last="Jersek">Miha Jersek</name><affiliation><mods:affiliation>Slovenian Museum of Natural History, Presernova 20, SI‐1000 Ljubljana, Slovenia</mods:affiliation></affiliation></author><author><name sortKey="Grau, Thomas" sort="Grau, Thomas" uniqKey="Grau T" first="Thomas" last="Grau">Thomas Grau</name><affiliation><mods:affiliation>European Research Center for Fireballs and Meteorites (ERFM), Puschkinstraße 23, 16321 Bernau bei Berlin, Germany</mods:affiliation></affiliation></author><author><name sortKey="Mirtic, Breda" sort="Mirtic, Breda" uniqKey="Mirtic B" first="Breda" last="Mirtic">Breda Mirtic</name><affiliation><mods:affiliation>Department of Geology, Faculty of Natural Sciences and Engineering, University of Ljubljana, SI‐1000 Ljubljana, Slovenia</mods:affiliation></affiliation></author><author><name sortKey="Ott, Ulrich" sort="Ott, Ulrich" uniqKey="Ott U" first="Ulrich" last="Ott">Ulrich Ott</name><affiliation><mods:affiliation>Abteilung Biogeochemie, Max‐Planck‐Institut für Chemie, Joh.‐J.‐Becher‐Weg 27, 55128 Mainz, Germany</mods:affiliation></affiliation></author><author><name sortKey="Ku Era, Jan" sort="Ku Era, Jan" uniqKey="Ku Era J" first="Jan" last="Ku Era">Jan Ku Era</name><affiliation><mods:affiliation>Nuclear Physics Institute, Academy of Sciences of the Czech Republic, CZ‐250 68 Řež near Prague, Czech Republic</mods:affiliation></affiliation><affiliation><mods:affiliation>Research Center Řež, Ltd., CZ‐250 68 Řež, Czech Republic</mods:affiliation></affiliation></author><author><name sortKey="Horstmann, Marian" sort="Horstmann, Marian" uniqKey="Horstmann M" first="Marian" last="Horstmann">Marian Horstmann</name><affiliation><mods:affiliation>Institut für Planetologie, Wilhelm‐Klemm‐Str. 10, 48149 Münster, Germany</mods:affiliation></affiliation></author><author><name sortKey="Laubenstein, Matthias" sort="Laubenstein, Matthias" uniqKey="Laubenstein M" first="Matthias" last="Laubenstein">Matthias Laubenstein</name><affiliation><mods:affiliation>Laboratori Nazionali del Gran Sasso – I.N.F.N., S.S.17/bis, km 18+910, I‐67010 Assergi (AQ), Italy</mods:affiliation></affiliation></author><author><name sortKey="Herrmann, Siegfried" sort="Herrmann, Siegfried" uniqKey="Herrmann S" first="Siegfried" last="Herrmann">Siegfried Herrmann</name><affiliation><mods:affiliation>Abteilung Biogeochemie, Max‐Planck‐Institut für Chemie, Joh.‐J.‐Becher‐Weg 27, 55128 Mainz, Germany</mods:affiliation></affiliation></author><author><name sortKey=" Anda, Zden K" sort=" Anda, Zden K" uniqKey=" Anda Z" first="Zden K" last=" Anda">Zden K Anda</name><affiliation><mods:affiliation>Nuclear Physics Institute, Academy of Sciences of the Czech Republic, CZ‐250 68 Řež near Prague, Czech Republic</mods:affiliation></affiliation></author><author><name sortKey="Weber, Marc" sort="Weber, Marc" uniqKey="Weber M" first="Marc" last="Weber">Marc Weber</name><affiliation><mods:affiliation>Max‐Planck‐Institut für Kernphysik, Postfach 103980, 69029 Heidelberg, Germany</mods:affiliation></affiliation></author><author><name sortKey="Heusser, Gerd" sort="Heusser, Gerd" uniqKey="Heusser G" first="Gerd" last="Heusser">Gerd Heusser</name><affiliation><mods:affiliation>Max‐Planck‐Institut für Kernphysik, Postfach 103980, 69029 Heidelberg, Germany</mods:affiliation></affiliation></author></analytic><monogr></monogr><series><title level="j">Meteoritics & Planetary Science</title><idno type="ISSN">1086-9379</idno><idno type="eISSN">1945-5100</idno><imprint><publisher>Blackwell Publishing Ltd</publisher><pubPlace>Oxford, UK</pubPlace><date type="published" when="2011-06">2011-06</date><biblScope unit="volume">46</biblScope><biblScope unit="issue">6</biblScope><biblScope unit="page" from="793">793</biblScope><biblScope unit="page" to="804">804</biblScope></imprint><idno type="ISSN">1086-9379</idno></series><idno type="istex">DB8113B9614DFC9BE7681347A05B7D98CB2BA5E7</idno><idno type="DOI">10.1111/j.1945-5100.2011.01191.x</idno><idno type="ArticleID">MAPS1191</idno></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">1086-9379</idno></seriesStmt></fileDesc><profileDesc><textClass></textClass><langUsage><language ident="en">en</language></langUsage></profileDesc></teiHeader><front><div type="abstract">Abstract– On April 9, 2009, at 3:00 CEST, a very bright fireball appeared over Carinthia and the Karavanke Mountains. The meteoroid entered the atmosphere at a very steep angle and disintegrated into a large number of objects. Two main objects were seen as separate fireballs up to an altitude of approximately 5 km, and witnesses reported loud explosions. Three stones were found with a total weight of approximately 3.611 kg. The measured activity of short‐lived cosmogenic radionuclides clearly indicates that two specimens result from a very recent meteorite fall. All cosmogenic radionuclide concentrations suggest a rather small preatmospheric radius of <20 cm; a nominal cosmic‐ray exposure age based on 21Ne is approximately 4 Ma, but the noble gas and radionuclide results in combination indicate a complex irradiation. Jesenice is a highly recrystallized rock with only a few relic chondrules visible in hand specimen and thin section. The texture, the large grain size of plagioclase, and the homogeneous compositions of olivines and pyroxenes clearly indicate that Jesenice is a L6 chondrite. The bulk composition of Jesenice is very close to the published average element concentration for L ordinary chondrites. The chondrite is weakly shocked (S3) as indicated by the undulatory extinction in olivine and plagioclase and the presence of planar fractures in olivine. Being weakly shocked and with gas retention ages of >1.7 Ga (4He) and approximately 4.3 Ga (40Ar), Jesenice seems not to have been strongly affected by the catastrophic disruption of the L‐chondrite parent body approximately 500 Ma ago.</div></front></TEI><istex><corpusName>wiley</corpusName><author><json:item><name>Addi BISCHOFF</name><affiliations><json:string>Institut für Planetologie, Wilhelm‐Klemm‐Str. 10, 48149 Münster, Germany</json:string></affiliations></json:item><json:item><name>Miha JERSEK</name><affiliations><json:string>Slovenian Museum of Natural History, Presernova 20, SI‐1000 Ljubljana, Slovenia</json:string></affiliations></json:item><json:item><name>Thomas GRAU</name><affiliations><json:string>European Research Center for Fireballs and Meteorites (ERFM), Puschkinstraße 23, 16321 Bernau bei Berlin, Germany</json:string></affiliations></json:item><json:item><name>Breda MIRTIC</name><affiliations><json:string>Department of Geology, Faculty of Natural Sciences and Engineering, University of Ljubljana, SI‐1000 Ljubljana, Slovenia</json:string></affiliations></json:item><json:item><name>Ulrich OTT</name><affiliations><json:string>Abteilung Biogeochemie, Max‐Planck‐Institut für Chemie, Joh.‐J.‐Becher‐Weg 27, 55128 Mainz, Germany</json:string></affiliations></json:item><json:item><name>Jan KUČERA</name><affiliations><json:string>Nuclear Physics Institute, Academy of Sciences of the Czech Republic, CZ‐250 68 Řež near Prague, Czech Republic</json:string><json:string>Research Center Řež, Ltd., CZ‐250 68 Řež, Czech Republic</json:string></affiliations></json:item><json:item><name>Marian HORSTMANN</name><affiliations><json:string>Institut für Planetologie, Wilhelm‐Klemm‐Str. 10, 48149 Münster, Germany</json:string></affiliations></json:item><json:item><name>Matthias LAUBENSTEIN</name><affiliations><json:string>Laboratori Nazionali del Gran Sasso – I.N.F.N., S.S.17/bis, km 18+910, I‐67010 Assergi (AQ), Italy</json:string></affiliations></json:item><json:item><name>Siegfried HERRMANN</name><affiliations><json:string>Abteilung Biogeochemie, Max‐Planck‐Institut für Chemie, Joh.‐J.‐Becher‐Weg 27, 55128 Mainz, Germany</json:string></affiliations></json:item><json:item><name>Zdeněk ŘANDA</name><affiliations><json:string>Nuclear Physics Institute, Academy of Sciences of the Czech Republic, CZ‐250 68 Řež near Prague, Czech Republic</json:string></affiliations></json:item><json:item><name>Marc WEBER</name><affiliations><json:string>Max‐Planck‐Institut für Kernphysik, Postfach 103980, 69029 Heidelberg, Germany</json:string></affiliations></json:item><json:item><name>Gerd HEUSSER</name><affiliations><json:string>Max‐Planck‐Institut für Kernphysik, Postfach 103980, 69029 Heidelberg, Germany</json:string></affiliations></json:item></author><articleId><json:string>MAPS1191</json:string></articleId><language><json:string>eng</json:string></language><originalGenre><json:string>article</json:string></originalGenre><abstract>Abstract– On April 9, 2009, at 3:00 CEST, a very bright fireball appeared over Carinthia and the Karavanke Mountains. The meteoroid entered the atmosphere at a very steep angle and disintegrated into a large number of objects. Two main objects were seen as separate fireballs up to an altitude of approximately 5 km, and witnesses reported loud explosions. Three stones were found with a total weight of approximately 3.611 kg. The measured activity of short‐lived cosmogenic radionuclides clearly indicates that two specimens result from a very recent meteorite fall. All cosmogenic radionuclide concentrations suggest a rather small preatmospheric radius of >20 cm; a nominal cosmic‐ray exposure age based on 21Ne is approximately 4 Ma, but the noble gas and radionuclide results in combination indicate a complex irradiation. Jesenice is a highly recrystallized rock with only a few relic chondrules visible in hand specimen and thin section. The texture, the large grain size of plagioclase, and the homogeneous compositions of olivines and pyroxenes clearly indicate that Jesenice is a L6 chondrite. The bulk composition of Jesenice is very close to the published average element concentration for L ordinary chondrites. The chondrite is weakly shocked (S3) as indicated by the undulatory extinction in olivine and plagioclase and the presence of planar fractures in olivine. Being weakly shocked and with gas retention ages of >1.7 Ga (4He) and approximately 4.3 Ga (40Ar), Jesenice seems not to have been strongly affected by the catastrophic disruption of the L‐chondrite parent body approximately 500 Ma ago.</abstract><qualityIndicators><score>7.904</score><pdfVersion>1.3</pdfVersion><pdfPageSize>595.276 x 790.866 pts</pdfPageSize><refBibsNative>true</refBibsNative><keywordCount>0</keywordCount><abstractCharCount>1617</abstractCharCount><pdfWordCount>5735</pdfWordCount><pdfCharCount>37915</pdfCharCount><pdfPageCount>12</pdfPageCount><abstractWordCount>242</abstractWordCount></qualityIndicators><title>Jesenice—A new meteorite fall from Slovenia</title><genre><json:string>article</json:string></genre><host><volume>46</volume><publisherId><json:string>MAPS</json:string></publisherId><pages><total>12</total><last>804</last><first>793</first></pages><issn><json:string>1086-9379</json:string></issn><issue>6</issue><genre><json:string>journal</json:string></genre><language><json:string>unknown</json:string></language><eissn><json:string>1945-5100</json:string></eissn><title>Meteoritics & Planetary Science</title><doi><json:string>10.1111/(ISSN)1945-5100</json:string></doi></host><publicationDate>2011</publicationDate><copyrightDate>2011</copyrightDate><doi><json:string>10.1111/j.1945-5100.2011.01191.x</json:string></doi><id>DB8113B9614DFC9BE7681347A05B7D98CB2BA5E7</id><score>0.055909332</score><fulltext><json:item><original>true</original><mimetype>application/pdf</mimetype><extension>pdf</extension><uri>https://api.istex.fr/document/DB8113B9614DFC9BE7681347A05B7D98CB2BA5E7/fulltext/pdf</uri></json:item><json:item><original>false</original><mimetype>application/zip</mimetype><extension>zip</extension><uri>https://api.istex.fr/document/DB8113B9614DFC9BE7681347A05B7D98CB2BA5E7/fulltext/zip</uri></json:item><istex:fulltextTEI uri="https://api.istex.fr/document/DB8113B9614DFC9BE7681347A05B7D98CB2BA5E7/fulltext/tei"><teiHeader><fileDesc><titleStmt><title level="a" type="main" xml:lang="en">Jesenice—A new meteorite fall from Slovenia</title></titleStmt><publicationStmt><authority>ISTEX</authority><publisher>Blackwell Publishing Ltd</publisher><pubPlace>Oxford, UK</pubPlace><availability><p>© The Meteoritical Society, 2011</p></availability><date>2011</date></publicationStmt><sourceDesc><biblStruct type="inbook"><analytic><title level="a" type="main" xml:lang="en">Jesenice—A new meteorite fall from Slovenia</title><author xml:id="author-1"><persName><forename type="first">Addi</forename><surname>BISCHOFF</surname></persName><note type="correspondence"><p>Correspondence: Corresponding author. E‐mail:</p></note><affiliation>Institut für Planetologie, Wilhelm‐Klemm‐Str. 10, 48149 Münster, Germany</affiliation></author><author xml:id="author-2"><persName><forename type="first">Miha</forename><surname>JERSEK</surname></persName><affiliation>Slovenian Museum of Natural History, Presernova 20, SI‐1000 Ljubljana, Slovenia</affiliation></author><author xml:id="author-3"><persName><forename type="first">Thomas</forename><surname>GRAU</surname></persName><affiliation>European Research Center for Fireballs and Meteorites (ERFM), Puschkinstraße 23, 16321 Bernau bei Berlin, Germany</affiliation></author><author xml:id="author-4"><persName><forename type="first">Breda</forename><surname>MIRTIC</surname></persName><affiliation>Department of Geology, Faculty of Natural Sciences and Engineering, University of Ljubljana, SI‐1000 Ljubljana, Slovenia</affiliation></author><author xml:id="author-5"><persName><forename type="first">Ulrich</forename><surname>OTT</surname></persName><affiliation>Abteilung Biogeochemie, Max‐Planck‐Institut für Chemie, Joh.‐J.‐Becher‐Weg 27, 55128 Mainz, Germany</affiliation></author><author xml:id="author-6"><persName><forename type="first">Jan</forename><surname>KUČERA</surname></persName><affiliation>Nuclear Physics Institute, Academy of Sciences of the Czech Republic, CZ‐250 68 Řež near Prague, Czech Republic</affiliation><affiliation>Research Center Řež, Ltd., CZ‐250 68 Řež, Czech Republic</affiliation></author><author xml:id="author-7"><persName><forename type="first">Marian</forename><surname>HORSTMANN</surname></persName><affiliation>Institut für Planetologie, Wilhelm‐Klemm‐Str. 10, 48149 Münster, Germany</affiliation></author><author xml:id="author-8"><persName><forename type="first">Matthias</forename><surname>LAUBENSTEIN</surname></persName><affiliation>Laboratori Nazionali del Gran Sasso – I.N.F.N., S.S.17/bis, km 18+910, I‐67010 Assergi (AQ), Italy</affiliation></author><author xml:id="author-9"><persName><forename type="first">Siegfried</forename><surname>HERRMANN</surname></persName><affiliation>Abteilung Biogeochemie, Max‐Planck‐Institut für Chemie, Joh.‐J.‐Becher‐Weg 27, 55128 Mainz, Germany</affiliation></author><author xml:id="author-10"><persName><forename type="first">Zdeněk</forename><surname>ŘANDA</surname></persName><affiliation>Nuclear Physics Institute, Academy of Sciences of the Czech Republic, CZ‐250 68 Řež near Prague, Czech Republic</affiliation></author><author xml:id="author-11"><persName><forename type="first">Marc</forename><surname>WEBER</surname></persName><affiliation>Max‐Planck‐Institut für Kernphysik, Postfach 103980, 69029 Heidelberg, Germany</affiliation></author><author xml:id="author-12"><persName><forename type="first">Gerd</forename><surname>HEUSSER</surname></persName><affiliation>Max‐Planck‐Institut für Kernphysik, Postfach 103980, 69029 Heidelberg, Germany</affiliation></author></analytic><monogr><title level="j">Meteoritics & Planetary Science</title><idno type="pISSN">1086-9379</idno><idno type="eISSN">1945-5100</idno><idno type="DOI">10.1111/(ISSN)1945-5100</idno><imprint><publisher>Blackwell Publishing Ltd</publisher><pubPlace>Oxford, UK</pubPlace><date type="published" when="2011-06"></date><biblScope unit="volume">46</biblScope><biblScope unit="issue">6</biblScope><biblScope unit="page" from="793">793</biblScope><biblScope unit="page" to="804">804</biblScope></imprint></monogr><idno type="istex">DB8113B9614DFC9BE7681347A05B7D98CB2BA5E7</idno><idno type="DOI">10.1111/j.1945-5100.2011.01191.x</idno><idno type="ArticleID">MAPS1191</idno></biblStruct></sourceDesc></fileDesc><profileDesc><creation><date>2011</date></creation><langUsage><language ident="en">en</language></langUsage><abstract><p>Abstract– On April 9, 2009, at 3:00 CEST, a very bright fireball appeared over Carinthia and the Karavanke Mountains. The meteoroid entered the atmosphere at a very steep angle and disintegrated into a large number of objects. Two main objects were seen as separate fireballs up to an altitude of approximately 5 km, and witnesses reported loud explosions. Three stones were found with a total weight of approximately 3.611 kg. The measured activity of short‐lived cosmogenic radionuclides clearly indicates that two specimens result from a very recent meteorite fall. All cosmogenic radionuclide concentrations suggest a rather small preatmospheric radius of <20 cm; a nominal cosmic‐ray exposure age based on 21Ne is approximately 4 Ma, but the noble gas and radionuclide results in combination indicate a complex irradiation. Jesenice is a highly recrystallized rock with only a few relic chondrules visible in hand specimen and thin section. The texture, the large grain size of plagioclase, and the homogeneous compositions of olivines and pyroxenes clearly indicate that Jesenice is a L6 chondrite. The bulk composition of Jesenice is very close to the published average element concentration for L ordinary chondrites. The chondrite is weakly shocked (S3) as indicated by the undulatory extinction in olivine and plagioclase and the presence of planar fractures in olivine. Being weakly shocked and with gas retention ages of >1.7 Ga (4He) and approximately 4.3 Ga (40Ar), Jesenice seems not to have been strongly affected by the catastrophic disruption of the L‐chondrite parent body approximately 500 Ma ago.</p></abstract></profileDesc><revisionDesc><change when="2011-06">Published</change></revisionDesc></teiHeader></istex:fulltextTEI><json:item><original>false</original><mimetype>text/plain</mimetype><extension>txt</extension><uri>https://api.istex.fr/document/DB8113B9614DFC9BE7681347A05B7D98CB2BA5E7/fulltext/txt</uri></json:item></fulltext><metadata><istex:metadataXml wicri:clean="Wiley, elements deleted: body"><istex:xmlDeclaration>version="1.0" encoding="UTF-8" standalone="yes"</istex:xmlDeclaration><istex:document><component version="2.0" type="serialArticle" xml:lang="en"><header><publicationMeta level="product"><publisherInfo><publisherName>Blackwell Publishing Ltd</publisherName><publisherLoc>Oxford, UK</publisherLoc></publisherInfo><doi origin="wiley" registered="yes">10.1111/(ISSN)1945-5100</doi><issn type="print">1086-9379</issn><issn type="electronic">1945-5100</issn><idGroup><id type="product" value="MAPS"></id><id type="publisherDivision" value="ST"></id></idGroup><titleGroup><title type="main" sort="METEORITICS AND PLANETARY SCIENCE">Meteoritics & Planetary Science</title></titleGroup></publicationMeta><publicationMeta level="part" position="06106"><doi origin="wiley">10.1111/maps.2011.46.issue-6</doi><numberingGroup><numbering type="journalVolume" number="46">46</numbering><numbering type="journalIssue" number="6">6</numbering></numberingGroup><coverDate startDate="2011-06">June 2011</coverDate></publicationMeta><publicationMeta level="unit" type="article" position="3" status="forIssue"><doi origin="wiley">10.1111/j.1945-5100.2011.01191.x</doi><idGroup><id type="unit" value="MAPS1191"></id></idGroup><countGroup><count type="pageTotal" number="12"></count></countGroup><titleGroup><title type="tocHeading1">Articles</title></titleGroup><copyright>© The Meteoritical Society, 2011</copyright><eventGroup><event type="xmlConverted" agent="Converter:BPG_TO_WML3G version:2.5.2 mode:FullText" date="2011-06-22"></event><event type="publishedOnlineEarlyUnpaginated" date="2011-04-15"></event><event type="publishedOnlineFinalForm" date="2011-06-13"></event><event type="firstOnline" date="2011-04-15"></event><event type="xmlConverted" agent="Converter:WILEY_ML3G_TO_WILEY_ML3GV2 version:4.0.1" date="2014-03-20"></event><event type="xmlConverted" agent="Converter:WML3G_To_WML3G version:4.1.7 mode:FullText,remove_FC" date="2014-10-31"></event></eventGroup><numberingGroup><numbering type="pageFirst" number="793">793</numbering><numbering type="pageLast" number="804">804</numbering></numberingGroup><correspondenceTo> Corresponding author. E‐mail: <email normalForm="bischoa@uni-muenster.de">bischoa@uni‐muenster.de</email></correspondenceTo><objectNameGroup><objectName elementName="appendix">Appendix</objectName></objectNameGroup><linkGroup><link type="toTypesetVersion" href="file:MAPS.MAPS1191.pdf"></link></linkGroup></publicationMeta><contentMeta><unparsedEditorialHistory>(Received 11 March 2010; revision accepted 16 January 2011)</unparsedEditorialHistory><countGroup><count type="figureTotal" number="4"></count><count type="tableTotal" number="4"></count></countGroup><titleGroup><title type="main">Jesenice—A new meteorite fall from Slovenia</title><title type="shortAuthors">A. Bischoff et al.</title><title type="short">Jesenice—A new meteorite fall from Slovenia</title></titleGroup><creators><creator creatorRole="author" xml:id="cr1" affiliationRef="#a1" corresponding="yes"><personName><givenNames>Addi</givenNames><familyName>BISCHOFF</familyName></personName></creator><creator creatorRole="author" xml:id="cr2" affiliationRef="#a2"><personName><givenNames>Miha</givenNames><familyName>JERSEK</familyName></personName></creator><creator creatorRole="author" xml:id="cr3" affiliationRef="#a3"><personName><givenNames>Thomas</givenNames><familyName>GRAU</familyName></personName></creator><creator creatorRole="author" xml:id="cr4" affiliationRef="#a4"><personName><givenNames>Breda</givenNames><familyName>MIRTIC</familyName></personName></creator><creator creatorRole="author" xml:id="cr5" affiliationRef="#a5"><personName><givenNames>Ulrich</givenNames><familyName>OTT</familyName></personName></creator><creator creatorRole="author" xml:id="cr6" affiliationRef="#a6 #a7"><personName><givenNames>Jan</givenNames><familyName>KUČERA</familyName></personName></creator><creator creatorRole="author" xml:id="cr7" affiliationRef="#a1"><personName><givenNames>Marian</givenNames><familyName>HORSTMANN</familyName></personName></creator><creator creatorRole="author" xml:id="cr8" affiliationRef="#a8"><personName><givenNames>Matthias</givenNames><familyName>LAUBENSTEIN</familyName></personName></creator><creator creatorRole="author" xml:id="cr9" affiliationRef="#a5"><personName><givenNames>Siegfried</givenNames><familyName>HERRMANN</familyName></personName></creator><creator creatorRole="author" xml:id="cr10" affiliationRef="#a6"><personName><givenNames>Zdeněk</givenNames><familyName>ŘANDA</familyName></personName></creator><creator creatorRole="author" xml:id="cr11" affiliationRef="#a9"><personName><givenNames>Marc</givenNames><familyName>WEBER</familyName></personName></creator><creator creatorRole="author" xml:id="cr12" affiliationRef="#a9"><personName><givenNames>Gerd</givenNames><familyName>HEUSSER</familyName></personName></creator></creators><affiliationGroup><affiliation xml:id="a1" countryCode="DE"><unparsedAffiliation>Institut für Planetologie, Wilhelm‐Klemm‐Str. 10, 48149 Münster, Germany</unparsedAffiliation></affiliation><affiliation xml:id="a2" countryCode="SI"><unparsedAffiliation>Slovenian Museum of Natural History, Presernova 20, SI‐1000 Ljubljana, Slovenia</unparsedAffiliation></affiliation><affiliation xml:id="a3" countryCode="DE"><unparsedAffiliation>European Research Center for Fireballs and Meteorites (ERFM), Puschkinstraße 23, 16321 Bernau bei Berlin, Germany</unparsedAffiliation></affiliation><affiliation xml:id="a4" countryCode="SI"><unparsedAffiliation>Department of Geology, Faculty of Natural Sciences and Engineering, University of Ljubljana, SI‐1000 Ljubljana, Slovenia</unparsedAffiliation></affiliation><affiliation xml:id="a5" countryCode="DE"><unparsedAffiliation>Abteilung Biogeochemie, Max‐Planck‐Institut für Chemie, Joh.‐J.‐Becher‐Weg 27, 55128 Mainz, Germany</unparsedAffiliation></affiliation><affiliation xml:id="a6" countryCode="CZ"><unparsedAffiliation>Nuclear Physics Institute, Academy of Sciences of the Czech Republic, CZ‐250 68 Řež near Prague, Czech Republic</unparsedAffiliation></affiliation><affiliation xml:id="a7" countryCode="CZ"><unparsedAffiliation>Research Center Řež, Ltd., CZ‐250 68 Řež, Czech Republic</unparsedAffiliation></affiliation><affiliation xml:id="a8" countryCode="IT"><unparsedAffiliation>Laboratori Nazionali del Gran Sasso – I.N.F.N., S.S.17/bis, km 18+910, I‐67010 Assergi (AQ), Italy</unparsedAffiliation></affiliation><affiliation xml:id="a9" countryCode="DE"><unparsedAffiliation>Max‐Planck‐Institut für Kernphysik, Postfach 103980, 69029 Heidelberg, Germany</unparsedAffiliation></affiliation></affiliationGroup><abstractGroup><abstract type="main" xml:lang="en"><p><b>Abstract–</b> On April 9, 2009, at 3:00 CEST, a very bright fireball appeared over Carinthia and the Karavanke Mountains. The meteoroid entered the atmosphere at a very steep angle and disintegrated into a large number of objects. Two main objects were seen as separate fireballs up to an altitude of approximately 5 km, and witnesses reported loud explosions. Three stones were found with a total weight of approximately 3.611 kg. The measured activity of short‐lived cosmogenic radionuclides clearly indicates that two specimens result from a very recent meteorite fall. All cosmogenic radionuclide concentrations suggest a rather small preatmospheric radius of <20 cm; a nominal cosmic‐ray exposure age based on <sup>21</sup>Ne is approximately 4 Ma, but the noble gas and radionuclide results in combination indicate a complex irradiation. Jesenice is a highly recrystallized rock with only a few relic chondrules visible in hand specimen and thin section. The texture, the large grain size of plagioclase, and the homogeneous compositions of olivines and pyroxenes clearly indicate that Jesenice is a L6 chondrite. The bulk composition of Jesenice is very close to the published average element concentration for L ordinary chondrites. The chondrite is weakly shocked (S3) as indicated by the undulatory extinction in olivine and plagioclase and the presence of planar fractures in olivine. Being weakly shocked and with gas retention ages of >1.7 Ga (<sup>4</sup>He) and approximately 4.3 Ga (<sup>40</sup>Ar), Jesenice seems not to have been strongly affected by the catastrophic disruption of the L‐chondrite parent body approximately 500 Ma ago.</p></abstract></abstractGroup></contentMeta></header></component></istex:document></istex:metadataXml><mods version="3.6"><titleInfo lang="en"><title>Jesenice—A new meteorite fall from Slovenia</title></titleInfo><titleInfo type="abbreviated" lang="en"><title>Jesenice—A new meteorite fall from Slovenia</title></titleInfo><titleInfo type="alternative" contentType="CDATA" lang="en"><title>Jesenice—A new meteorite fall from Slovenia</title></titleInfo><name type="personal"><namePart type="given">Addi</namePart><namePart type="family">BISCHOFF</namePart><affiliation>Institut für Planetologie, Wilhelm‐Klemm‐Str. 10, 48149 Münster, Germany</affiliation><description>Correspondence: Corresponding author. E‐mail: </description><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Miha</namePart><namePart type="family">JERSEK</namePart><affiliation>Slovenian Museum of Natural History, Presernova 20, SI‐1000 Ljubljana, Slovenia</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Thomas</namePart><namePart type="family">GRAU</namePart><affiliation>European Research Center for Fireballs and Meteorites (ERFM), Puschkinstraße 23, 16321 Bernau bei Berlin, Germany</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Breda</namePart><namePart type="family">MIRTIC</namePart><affiliation>Department of Geology, Faculty of Natural Sciences and Engineering, University of Ljubljana, SI‐1000 Ljubljana, Slovenia</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Ulrich</namePart><namePart type="family">OTT</namePart><affiliation>Abteilung Biogeochemie, Max‐Planck‐Institut für Chemie, Joh.‐J.‐Becher‐Weg 27, 55128 Mainz, Germany</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Jan</namePart><namePart type="family">KUČERA</namePart><affiliation>Nuclear Physics Institute, Academy of Sciences of the Czech Republic, CZ‐250 68 Řež near Prague, Czech Republic</affiliation><affiliation>Research Center Řež, Ltd., CZ‐250 68 Řež, Czech Republic</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Marian</namePart><namePart type="family">HORSTMANN</namePart><affiliation>Institut für Planetologie, Wilhelm‐Klemm‐Str. 10, 48149 Münster, Germany</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Matthias</namePart><namePart type="family">LAUBENSTEIN</namePart><affiliation>Laboratori Nazionali del Gran Sasso – I.N.F.N., S.S.17/bis, km 18+910, I‐67010 Assergi (AQ), Italy</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Siegfried</namePart><namePart type="family">HERRMANN</namePart><affiliation>Abteilung Biogeochemie, Max‐Planck‐Institut für Chemie, Joh.‐J.‐Becher‐Weg 27, 55128 Mainz, Germany</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Zdeněk</namePart><namePart type="family">ŘANDA</namePart><affiliation>Nuclear Physics Institute, Academy of Sciences of the Czech Republic, CZ‐250 68 Řež near Prague, Czech Republic</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Marc</namePart><namePart type="family">WEBER</namePart><affiliation>Max‐Planck‐Institut für Kernphysik, Postfach 103980, 69029 Heidelberg, Germany</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Gerd</namePart><namePart type="family">HEUSSER</namePart><affiliation>Max‐Planck‐Institut für Kernphysik, Postfach 103980, 69029 Heidelberg, Germany</affiliation><role><roleTerm type="text">author</roleTerm></role></name><typeOfResource>text</typeOfResource><genre type="article" displayLabel="article"></genre><originInfo><publisher>Blackwell Publishing Ltd</publisher><place><placeTerm type="text">Oxford, UK</placeTerm></place><dateIssued encoding="w3cdtf">2011-06</dateIssued><edition>(Received 11 March 2010; revision accepted 16 January 2011)</edition><copyrightDate encoding="w3cdtf">2011</copyrightDate></originInfo><language><languageTerm type="code" authority="rfc3066">en</languageTerm><languageTerm type="code" authority="iso639-2b">eng</languageTerm></language><physicalDescription><internetMediaType>text/html</internetMediaType><extent unit="figures">4</extent><extent unit="tables">4</extent></physicalDescription><abstract>Abstract– On April 9, 2009, at 3:00 CEST, a very bright fireball appeared over Carinthia and the Karavanke Mountains. The meteoroid entered the atmosphere at a very steep angle and disintegrated into a large number of objects. Two main objects were seen as separate fireballs up to an altitude of approximately 5 km, and witnesses reported loud explosions. Three stones were found with a total weight of approximately 3.611 kg. The measured activity of short‐lived cosmogenic radionuclides clearly indicates that two specimens result from a very recent meteorite fall. All cosmogenic radionuclide concentrations suggest a rather small preatmospheric radius of <20 cm; a nominal cosmic‐ray exposure age based on 21Ne is approximately 4 Ma, but the noble gas and radionuclide results in combination indicate a complex irradiation. Jesenice is a highly recrystallized rock with only a few relic chondrules visible in hand specimen and thin section. The texture, the large grain size of plagioclase, and the homogeneous compositions of olivines and pyroxenes clearly indicate that Jesenice is a L6 chondrite. The bulk composition of Jesenice is very close to the published average element concentration for L ordinary chondrites. The chondrite is weakly shocked (S3) as indicated by the undulatory extinction in olivine and plagioclase and the presence of planar fractures in olivine. Being weakly shocked and with gas retention ages of >1.7 Ga (4He) and approximately 4.3 Ga (40Ar), Jesenice seems not to have been strongly affected by the catastrophic disruption of the L‐chondrite parent body approximately 500 Ma ago.</abstract><relatedItem type="host"><titleInfo><title>Meteoritics & Planetary Science</title></titleInfo><genre type="journal">journal</genre><identifier type="ISSN">1086-9379</identifier><identifier type="eISSN">1945-5100</identifier><identifier type="DOI">10.1111/(ISSN)1945-5100</identifier><identifier type="PublisherID">MAPS</identifier><part><date>2011</date><detail type="volume"><caption>vol.</caption><number>46</number></detail><detail type="issue"><caption>no.</caption><number>6</number></detail><extent unit="pages"><start>793</start><end>804</end><total>12</total></extent></part></relatedItem><identifier type="istex">DB8113B9614DFC9BE7681347A05B7D98CB2BA5E7</identifier><identifier type="DOI">10.1111/j.1945-5100.2011.01191.x</identifier><identifier type="ArticleID">MAPS1191</identifier><accessCondition type="use and reproduction" contentType="copyright">© The Meteoritical Society, 2011</accessCondition><recordInfo><recordContentSource>WILEY</recordContentSource><recordOrigin>Blackwell Publishing Ltd</recordOrigin></recordInfo></mods></metadata><serie></serie></istex></record>Pour manipuler ce document sous Unix (Dilib)
EXPLOR_STEP=$WICRI_ROOT/Wicri/Terre/explor/CobaltMaghrebV1/Data/Istex/Corpus
HfdSelect -h $EXPLOR_STEP/biblio.hfd -nk 000E19 | SxmlIndent | more
Ou
HfdSelect -h $EXPLOR_AREA/Data/Istex/Corpus/biblio.hfd -nk 000E19 | SxmlIndent | more
Pour mettre un lien sur cette page dans le réseau Wicri
{{Explor lien
|wiki= Wicri/Terre
|area= CobaltMaghrebV1
|flux= Istex
|étape= Corpus
|type= RBID
|clé= ISTEX:DB8113B9614DFC9BE7681347A05B7D98CB2BA5E7
|texte= Jesenice—A new meteorite fall from Slovenia
}}
| This area was generated with Dilib version V0.6.32. |  |