TY - JOUR
T1 - Evidence for multiple dynamic events and subsequent decompression stage recorded in a shock vein
AU - Miyahara, Masaaki
AU - Otani, Eiji
AU - Kimura, Makoto
AU - Ozawa, Shin
AU - Nagase, Toshiro
AU - Nishijima, Masahiko
AU - Hiraga, Kenji
N1 - Funding Information:
We are grateful to Prof. A. El Goresy and two anonymous reviewers who helped in considerably improving the manuscript. We thank the National Institute of the Polar Research for providing us a chance to study the shocked L6 chondrite Y-791384 sample. We appreciate the help of Ito, Y. and Kawanobe, Y. for EMPA analysis. A part of this work was supported by "Nanotechnology Support Project" of the Ministry of Education, Culture, Sports, Science and Technology (MEXT) , Japan. This study was also partly supported by the grant-in-aids for the Scientific Research (No. 18104009 and 22000002 ) of MEXT to E.O. and grant-in-aids for the Scientific Research (No. 19540500 and 22540488 ) of MEXT to M.K. This work was conducted as a part of Tohoku University Global COE program “Global Education and Research Center for Earth and Planetary Dynamics”.
PY - 2011/7/15
Y1 - 2011/7/15
N2 - We investigated a shock vein of the Yamato 791384 L6 chondrite to clarify the nature and sequence of the dynamic processes that resulted from the shock events. The chondritic host-rock of Y-791384 mainly consists of olivine (Fa24-25), low-Ca pyroxene (Fs18-22), albitic feldspar (An9-10Ab84-86Or5-7), troilite and metallic Fe-Ni. The shock vein contains majorite (or majorite-pyropess) and magnesiowüstite (+ minor jadeite) as high-pressure polymorphs. Two different dynamic events were recorded in the shock vein. The majorite grain contained vitrified (Mg,Fe)SiO3-perovskite inclusions. The (Mg,Fe)SiO3-perovskite was crystallized from a chondritic melt, and is a remnant of a first dynamic event. The majorite and magnesiowüstite were also crystallized directly from a chondritic melt but induced by a second dynamic event. The pressure condition for the first and second dynamic events would be >~24GPa and <~22GPa, respectively. Pervasive feather-shaped olivine (Fa16) nucleated on the magnesiowüstite and majorite. This feather-shaped olivine is evidence for rapidly grown olivine from the melt related to the shock event. Phase relations deduced from high-pressure melting experiments of the Allende meteorite and peridotite indicate that the magnesiowüstite and majorite+olivine pair cannot coexist at equilibrium condition. The disequilibrium assemblage reflects a decompression stage. These features demonstrate the complexity of events during a natural dynamic process.
AB - We investigated a shock vein of the Yamato 791384 L6 chondrite to clarify the nature and sequence of the dynamic processes that resulted from the shock events. The chondritic host-rock of Y-791384 mainly consists of olivine (Fa24-25), low-Ca pyroxene (Fs18-22), albitic feldspar (An9-10Ab84-86Or5-7), troilite and metallic Fe-Ni. The shock vein contains majorite (or majorite-pyropess) and magnesiowüstite (+ minor jadeite) as high-pressure polymorphs. Two different dynamic events were recorded in the shock vein. The majorite grain contained vitrified (Mg,Fe)SiO3-perovskite inclusions. The (Mg,Fe)SiO3-perovskite was crystallized from a chondritic melt, and is a remnant of a first dynamic event. The majorite and magnesiowüstite were also crystallized directly from a chondritic melt but induced by a second dynamic event. The pressure condition for the first and second dynamic events would be >~24GPa and <~22GPa, respectively. Pervasive feather-shaped olivine (Fa16) nucleated on the magnesiowüstite and majorite. This feather-shaped olivine is evidence for rapidly grown olivine from the melt related to the shock event. Phase relations deduced from high-pressure melting experiments of the Allende meteorite and peridotite indicate that the magnesiowüstite and majorite+olivine pair cannot coexist at equilibrium condition. The disequilibrium assemblage reflects a decompression stage. These features demonstrate the complexity of events during a natural dynamic process.
KW - Decompression
KW - Melting
KW - Olivine dendrite
KW - Shocked meteorite
KW - TEM
UR - http://www.scopus.com/inward/record.url?scp=79959757171&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=79959757171&partnerID=8YFLogxK
U2 - 10.1016/j.epsl.2011.05.010
DO - 10.1016/j.epsl.2011.05.010
M3 - Article
AN - SCOPUS:79959757171
VL - 307
SP - 361
EP - 368
JO - Earth and Planetary Sciences Letters
JF - Earth and Planetary Sciences Letters
SN - 0012-821X
IS - 3-4
ER -