Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
Fe-ni-p-s melt pockets in elga iie iron meteorite : Evidence for the origin at high-pressures up to 20 gpa. / Litasov, Konstantin D.; Teplyakova, Svetlana N.; Shatskiy, Anton и др.
в: Minerals, Том 9, № 10, 616, 01.10.2019.Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
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TY - JOUR
T1 - Fe-ni-p-s melt pockets in elga iie iron meteorite
T2 - Evidence for the origin at high-pressures up to 20 gpa
AU - Litasov, Konstantin D.
AU - Teplyakova, Svetlana N.
AU - Shatskiy, Anton
AU - Kuper, Konstantin E.
PY - 2019/10/1
Y1 - 2019/10/1
N2 - Here we report new data on high-pressure microstructures in Elga group IIE iron meteorites, made of solidified Fe-Ni-P-S melt pockets and microcrystalline aggregates, which could be formed only at high pressures and temperatures according to the experimental data. The bulk composition of the melt pockets and crystals correspond to the Fe3 P-Fe3 S solid solution with the closure of an immiscibility gap at pressures near 20 GPa in static experiments. Some other melt pockets fit with the Fe2 S-Fe2 P compositions, which could also correspond to high pressures and temperatures. The results suggest a late shock episode during the formation of the IIE iron parent body, which may be prior or due to the final disruption that caused the meteorite arrival to Earth. It also has an important implication to the shock features in other meteorites, such as ureilite.
AB - Here we report new data on high-pressure microstructures in Elga group IIE iron meteorites, made of solidified Fe-Ni-P-S melt pockets and microcrystalline aggregates, which could be formed only at high pressures and temperatures according to the experimental data. The bulk composition of the melt pockets and crystals correspond to the Fe3 P-Fe3 S solid solution with the closure of an immiscibility gap at pressures near 20 GPa in static experiments. Some other melt pockets fit with the Fe2 S-Fe2 P compositions, which could also correspond to high pressures and temperatures. The results suggest a late shock episode during the formation of the IIE iron parent body, which may be prior or due to the final disruption that caused the meteorite arrival to Earth. It also has an important implication to the shock features in other meteorites, such as ureilite.
KW - High-pressure phases
KW - Iron meteorite
KW - Phosphide
KW - Shock metamorphism
KW - Sulfide
KW - phosphide
KW - SYSTEM
KW - MINERALS
KW - STABILITY
KW - POLYMORPH
KW - high-pressure phases
KW - PHASE
KW - EVOLUTION
KW - iron meteorite
KW - BULK MODULUS
KW - sulfide
KW - shock metamorphism
UR - http://www.scopus.com/inward/record.url?scp=85073516215&partnerID=8YFLogxK
U2 - 10.3390/min9100616
DO - 10.3390/min9100616
M3 - Article
AN - SCOPUS:85073516215
VL - 9
JO - Minerals
JF - Minerals
SN - 2075-163X
IS - 10
M1 - 616
ER -
ID: 21937398