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Magnetic properties of the Chelyabinsk meteorite: Preliminary results
This paper presents the distribution of magnetic susceptibility, χ 0 , in fragments of the Chelyabinsk ordinary chondrite (LL5, S4, W0, fall of February 15, 2013) from the collection of the Vernadsky Institute of Geochemistry and Analytical Chemistry, Russian Academy of Sciences, and results obtaine...
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Published in: | Geochemistry international 2013-07, Vol.51 (7), p.568-574 |
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description | This paper presents the distribution of magnetic susceptibility, χ
0
, in fragments of the Chelyabinsk ordinary chondrite (LL5, S4, W0, fall of February 15, 2013) from the collection of the Vernadsky Institute of Geochemistry and Analytical Chemistry, Russian Academy of Sciences, and results obtained by standard magnetic techniques for the meteorite material, including thermomagnetic analysis, measurements of natural remanent magnetization (NRM) and saturation isothermal remanent magnetization (SIRM), as well as the spectra of their alternating field demagnetization at amplitudes up to 170 mT, measurements of hysteresis loops and back-field remanence demagnetization curves at temperatures from 10 K to 700°C etc. The mean logχ
0
values for the light-colored (main) lithology of the meteorite material and impact-melt breccia from our collection are 4.54 ± 0.10 (
n
= 66) and 4.65 ± 0.09 (
n
= 38) (×10
−9
m
3
/kg), respectively. According to international magnetic classification of meteorites, Chelyabinsk falls within the range of LL5 chondrites. The mean metal content was estimated from the saturation magnetization,
M
s
, of the light- and dark-colored lithologies as 3.7 and 4.1 wt %, respectively. Hence, the dark lithology is richer in metal. The metal grains are multidomain at room temperature and show low coercive force,
B
c
(75 K. In the temperature range below 75 K, magnetic properties are controlled by chromite; the magnetic hardness of the samples is maximal at 10 K and equals to 606 and 157 mT for the light- and dark-colored lithologies, respectively. |
doi_str_mv | 10.1134/S0016702913070082 |
format | article |
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0
, in fragments of the Chelyabinsk ordinary chondrite (LL5, S4, W0, fall of February 15, 2013) from the collection of the Vernadsky Institute of Geochemistry and Analytical Chemistry, Russian Academy of Sciences, and results obtained by standard magnetic techniques for the meteorite material, including thermomagnetic analysis, measurements of natural remanent magnetization (NRM) and saturation isothermal remanent magnetization (SIRM), as well as the spectra of their alternating field demagnetization at amplitudes up to 170 mT, measurements of hysteresis loops and back-field remanence demagnetization curves at temperatures from 10 K to 700°C etc. The mean logχ
0
values for the light-colored (main) lithology of the meteorite material and impact-melt breccia from our collection are 4.54 ± 0.10 (
n
= 66) and 4.65 ± 0.09 (
n
= 38) (×10
−9
m
3
/kg), respectively. According to international magnetic classification of meteorites, Chelyabinsk falls within the range of LL5 chondrites. The mean metal content was estimated from the saturation magnetization,
M
s
, of the light- and dark-colored lithologies as 3.7 and 4.1 wt %, respectively. Hence, the dark lithology is richer in metal. The metal grains are multidomain at room temperature and show low coercive force,
B
c
(<2 mT) and remanent coercive force,
B
cr
(15–23 mT). The thermomagnetic analyses of the samples showed that the magnetic properties of the Chelyabinsk meteorite are controlled mainly by taenite and kamacite at temperatures >75 K. In the temperature range below 75 K, magnetic properties are controlled by chromite; the magnetic hardness of the samples is maximal at 10 K and equals to 606 and 157 mT for the light- and dark-colored lithologies, respectively.</description><identifier>ISSN: 0016-7029</identifier><identifier>EISSN: 1556-1968</identifier><identifier>DOI: 10.1134/S0016702913070082</identifier><language>eng</language><publisher>Boston: Springer US</publisher><subject>Chondrites ; Coercive force ; Controlled atmospheres ; Earth and Environmental Science ; Earth Sciences ; Geochemistry ; Lithology ; Magnetic properties ; Magnetism ; Magnetization ; Meteorites ; Meteors & meteorites ; Mineralogy ; Petrology</subject><ispartof>Geochemistry international, 2013-07, Vol.51 (7), p.568-574</ispartof><rights>Pleiades Publishing, Ltd. 2013</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a405t-ae0ba39f8a443180a25324e9a0e62de52bcfdb699146f3033cd54a0ba0d2946f3</citedby><cites>FETCH-LOGICAL-a405t-ae0ba39f8a443180a25324e9a0e62de52bcfdb699146f3033cd54a0ba0d2946f3</cites></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>Bezaeva, N. S.</creatorcontrib><creatorcontrib>Badyukov, D. D.</creatorcontrib><creatorcontrib>Nazarov, M. A.</creatorcontrib><creatorcontrib>Rochette, P.</creatorcontrib><creatorcontrib>Feinberg, J.</creatorcontrib><title>Magnetic properties of the Chelyabinsk meteorite: Preliminary results</title><title>Geochemistry international</title><addtitle>Geochem. Int</addtitle><description>This paper presents the distribution of magnetic susceptibility, χ
0
, in fragments of the Chelyabinsk ordinary chondrite (LL5, S4, W0, fall of February 15, 2013) from the collection of the Vernadsky Institute of Geochemistry and Analytical Chemistry, Russian Academy of Sciences, and results obtained by standard magnetic techniques for the meteorite material, including thermomagnetic analysis, measurements of natural remanent magnetization (NRM) and saturation isothermal remanent magnetization (SIRM), as well as the spectra of their alternating field demagnetization at amplitudes up to 170 mT, measurements of hysteresis loops and back-field remanence demagnetization curves at temperatures from 10 K to 700°C etc. The mean logχ
0
values for the light-colored (main) lithology of the meteorite material and impact-melt breccia from our collection are 4.54 ± 0.10 (
n
= 66) and 4.65 ± 0.09 (
n
= 38) (×10
−9
m
3
/kg), respectively. According to international magnetic classification of meteorites, Chelyabinsk falls within the range of LL5 chondrites. The mean metal content was estimated from the saturation magnetization,
M
s
, of the light- and dark-colored lithologies as 3.7 and 4.1 wt %, respectively. Hence, the dark lithology is richer in metal. The metal grains are multidomain at room temperature and show low coercive force,
B
c
(<2 mT) and remanent coercive force,
B
cr
(15–23 mT). The thermomagnetic analyses of the samples showed that the magnetic properties of the Chelyabinsk meteorite are controlled mainly by taenite and kamacite at temperatures >75 K. In the temperature range below 75 K, magnetic properties are controlled by chromite; the magnetic hardness of the samples is maximal at 10 K and equals to 606 and 157 mT for the light- and dark-colored lithologies, respectively.</description><subject>Chondrites</subject><subject>Coercive force</subject><subject>Controlled atmospheres</subject><subject>Earth and Environmental Science</subject><subject>Earth Sciences</subject><subject>Geochemistry</subject><subject>Lithology</subject><subject>Magnetic properties</subject><subject>Magnetism</subject><subject>Magnetization</subject><subject>Meteorites</subject><subject>Meteors & meteorites</subject><subject>Mineralogy</subject><subject>Petrology</subject><issn>0016-7029</issn><issn>1556-1968</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><recordid>eNqFkU1PwzAMhiMEEmPwA7hV4sKl4Hw0bbihaQOkIZCAc5W27pbRj5Gkh_17Uo0DAiFOluzntV_bhJxTuKKUi-sXACpTYIpySAEydkAmNElkTJXMDslkLMdj_ZicOLcBEIKrdELmj3rVoTdltLX9Fq036KK-jvwao9kam50uTOfeoxY99tZ4vImeLTamNZ22u8iiGxrvTslRrRuHZ19xSt4W89fZfbx8unuY3S5jLSDxsUYoNFd1psN0moFmCWcClQaUrMKEFWVdFVIpKmTNgfOySoQOGqiYGlNTcrnvG8x-DOh83hpXYtPoDvvB5TRNgYtMMfo_moDkMpV8RC9-oJt-sF1YJKeCpgKCzSxQdE-VtnfOYp1vrWnDEXIK-fiD_NcPgobtNS6w3Qrtt85_ij4B3P2G7A</recordid><startdate>20130701</startdate><enddate>20130701</enddate><creator>Bezaeva, N. S.</creator><creator>Badyukov, D. D.</creator><creator>Nazarov, M. A.</creator><creator>Rochette, P.</creator><creator>Feinberg, J.</creator><general>Springer US</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7QH</scope><scope>7UA</scope><scope>7XB</scope><scope>88I</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ATCPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>C1K</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>F1W</scope><scope>GNUQQ</scope><scope>H96</scope><scope>HCIFZ</scope><scope>L.G</scope><scope>M2P</scope><scope>PATMY</scope><scope>PCBAR</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PYCSY</scope><scope>Q9U</scope><scope>8FD</scope><scope>FR3</scope><scope>H8D</scope><scope>KR7</scope><scope>L7M</scope></search><sort><creationdate>20130701</creationdate><title>Magnetic properties of the Chelyabinsk meteorite: Preliminary results</title><author>Bezaeva, N. S. ; Badyukov, D. D. ; Nazarov, M. A. ; Rochette, P. ; Feinberg, J.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a405t-ae0ba39f8a443180a25324e9a0e62de52bcfdb699146f3033cd54a0ba0d2946f3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>Chondrites</topic><topic>Coercive force</topic><topic>Controlled atmospheres</topic><topic>Earth and Environmental Science</topic><topic>Earth Sciences</topic><topic>Geochemistry</topic><topic>Lithology</topic><topic>Magnetic properties</topic><topic>Magnetism</topic><topic>Magnetization</topic><topic>Meteorites</topic><topic>Meteors & meteorites</topic><topic>Mineralogy</topic><topic>Petrology</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Bezaeva, N. S.</creatorcontrib><creatorcontrib>Badyukov, D. D.</creatorcontrib><creatorcontrib>Nazarov, M. A.</creatorcontrib><creatorcontrib>Rochette, P.</creatorcontrib><creatorcontrib>Feinberg, J.</creatorcontrib><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>Aqualine</collection><collection>Water Resources Abstracts</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Science Database (Alumni Edition)</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>Agricultural & Environmental Science Collection</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Natural Science Collection</collection><collection>Earth, Atmospheric & Aquatic Science Collection</collection><collection>Environmental Sciences and Pollution Management</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>ProQuest Central Student</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>SciTech Premium Collection</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><collection>Science Database</collection><collection>Environmental Science Database</collection><collection>Earth, Atmospheric & Aquatic Science Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>Environmental Science Collection</collection><collection>ProQuest Central Basic</collection><collection>Technology Research Database</collection><collection>Engineering Research Database</collection><collection>Aerospace Database</collection><collection>Civil Engineering Abstracts</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Geochemistry international</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Bezaeva, N. S.</au><au>Badyukov, D. D.</au><au>Nazarov, M. A.</au><au>Rochette, P.</au><au>Feinberg, J.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Magnetic properties of the Chelyabinsk meteorite: Preliminary results</atitle><jtitle>Geochemistry international</jtitle><stitle>Geochem. Int</stitle><date>2013-07-01</date><risdate>2013</risdate><volume>51</volume><issue>7</issue><spage>568</spage><epage>574</epage><pages>568-574</pages><issn>0016-7029</issn><eissn>1556-1968</eissn><abstract>This paper presents the distribution of magnetic susceptibility, χ
0
, in fragments of the Chelyabinsk ordinary chondrite (LL5, S4, W0, fall of February 15, 2013) from the collection of the Vernadsky Institute of Geochemistry and Analytical Chemistry, Russian Academy of Sciences, and results obtained by standard magnetic techniques for the meteorite material, including thermomagnetic analysis, measurements of natural remanent magnetization (NRM) and saturation isothermal remanent magnetization (SIRM), as well as the spectra of their alternating field demagnetization at amplitudes up to 170 mT, measurements of hysteresis loops and back-field remanence demagnetization curves at temperatures from 10 K to 700°C etc. The mean logχ
0
values for the light-colored (main) lithology of the meteorite material and impact-melt breccia from our collection are 4.54 ± 0.10 (
n
= 66) and 4.65 ± 0.09 (
n
= 38) (×10
−9
m
3
/kg), respectively. According to international magnetic classification of meteorites, Chelyabinsk falls within the range of LL5 chondrites. The mean metal content was estimated from the saturation magnetization,
M
s
, of the light- and dark-colored lithologies as 3.7 and 4.1 wt %, respectively. Hence, the dark lithology is richer in metal. The metal grains are multidomain at room temperature and show low coercive force,
B
c
(<2 mT) and remanent coercive force,
B
cr
(15–23 mT). The thermomagnetic analyses of the samples showed that the magnetic properties of the Chelyabinsk meteorite are controlled mainly by taenite and kamacite at temperatures >75 K. In the temperature range below 75 K, magnetic properties are controlled by chromite; the magnetic hardness of the samples is maximal at 10 K and equals to 606 and 157 mT for the light- and dark-colored lithologies, respectively.</abstract><cop>Boston</cop><pub>Springer US</pub><doi>10.1134/S0016702913070082</doi><tpages>7</tpages></addata></record> |
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subjects | Chondrites Coercive force Controlled atmospheres Earth and Environmental Science Earth Sciences Geochemistry Lithology Magnetic properties Magnetism Magnetization Meteorites Meteors & meteorites Mineralogy Petrology |
title | Magnetic properties of the Chelyabinsk meteorite: Preliminary results |
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