TY - JOUR
T1 - Moissanite (SiC) with metal-silicide and silicon inclusions from tuff of Israel
T2 - Raman spectroscopy and electron microscope studies
AU - Dobrzhinetskaya, Larissa
AU - Mukhin, Pavel
AU - Wang, Qin
AU - Wirth, Richard
AU - O'Bannon, Earl
AU - Zhao, Wenxia
AU - Eppelbaum, Lev
AU - Sokhonchuk, Tatiana
N1 - Publisher Copyright:
© 2017 Elsevier B.V.
PY - 2018/6
Y1 - 2018/6
N2 - Here, we present studies of natural SiC that occurs in situ in tuff related to the Miocene alkaline basalt formation deposited in northern part of Israel. Raman spectroscopy, SEM and FIB-assisted TEM studies revealed that SiC is primarily hexagonal polytypes 4H-SiC and 6H-SiC, and that the 4H-SiC polytype is the predominant phase. Both SiC polytypes contain crystalline inclusions of silicon (Sio) and inclusions of metal-silicide with varying compositions (e.g. Si58V25Ti12Cr3Fe2, Si41Fe24Ti20Ni7V5Zr3, and Si43Fe40Ni17). The silicides crystal structure parameters match Si2TiV5 (Pm-3m space group, cubic), FeSi2Ti (Pbam space group, orthorhombic), and FeSi2 (Cmca space group, orthorhombic) respectively. We hypothesize that SiC was formed in a local ultra-reduced environment at respectively shallow depths (60–100 km), through a reaction of SiO2 with highly reducing fluids (H2O–CH4–H2–C2H6) arisen from the mantle “hot spot” and passing through alkaline basalt magma reservoir. SiO2 interacting with the fluids may originate from the walls of the crustal rocks surrounding this magmatic reservoir. This process led to the formation of SiC and accompanied by the reducing of metal-oxides to native metals, alloys, and silicides. The latter were trapped by SiC during its growth. Hence, interplate “hot spot” alkali basalt volcanism can now be included as a geological environment where SiC, silicon, and silicides can be found.
AB - Here, we present studies of natural SiC that occurs in situ in tuff related to the Miocene alkaline basalt formation deposited in northern part of Israel. Raman spectroscopy, SEM and FIB-assisted TEM studies revealed that SiC is primarily hexagonal polytypes 4H-SiC and 6H-SiC, and that the 4H-SiC polytype is the predominant phase. Both SiC polytypes contain crystalline inclusions of silicon (Sio) and inclusions of metal-silicide with varying compositions (e.g. Si58V25Ti12Cr3Fe2, Si41Fe24Ti20Ni7V5Zr3, and Si43Fe40Ni17). The silicides crystal structure parameters match Si2TiV5 (Pm-3m space group, cubic), FeSi2Ti (Pbam space group, orthorhombic), and FeSi2 (Cmca space group, orthorhombic) respectively. We hypothesize that SiC was formed in a local ultra-reduced environment at respectively shallow depths (60–100 km), through a reaction of SiO2 with highly reducing fluids (H2O–CH4–H2–C2H6) arisen from the mantle “hot spot” and passing through alkaline basalt magma reservoir. SiO2 interacting with the fluids may originate from the walls of the crustal rocks surrounding this magmatic reservoir. This process led to the formation of SiC and accompanied by the reducing of metal-oxides to native metals, alloys, and silicides. The latter were trapped by SiC during its growth. Hence, interplate “hot spot” alkali basalt volcanism can now be included as a geological environment where SiC, silicon, and silicides can be found.
KW - 4H-SiC
KW - 6H-SiC
KW - Metal-silicides
KW - Moissanite
KW - Silicon
KW - Tuff-tuffite
UR - http://www.scopus.com/inward/record.url?scp=85047243970&partnerID=8YFLogxK
U2 - 10.1016/j.lithos.2017.04.001
DO - 10.1016/j.lithos.2017.04.001
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AN - SCOPUS:85047243970
SN - 0024-4937
VL - 310-311
SP - 355
EP - 368
JO - Lithos
JF - Lithos
ER -