TY - JOUR
T1 - Mineral chemistry from the Late Cretaceous peralkaline rhyolite at Hadjer el Khamis, Chad
T2 - constraints on magmatic conditions
AU - Shellnutt, J. Gregory
AU - Iizuka, Yoshiyuki
AU - Lee, Tung Yi
AU - Chen, Wei Yu
N1 - Publisher Copyright:
© 2022 E. Schweizerbart’sche Verlagsbuchhandlung, Stuttgart, Germany.
PY - 2022/9
Y1 - 2022/9
N2 - The Late Cretaceous (74.4 ± 1.3 Ma) peralkaline rhyolite from Hadjer el Khamis erupted during a period of rifting within the Bornu and Termit basins of the Lake Chad region. The rhyolites are representative of a residual silicic magma that was derived by fractional crystallization of mantle derived basaltic parental magma. The primary phenocrysts of the rocks are quartz, alkali feldspar, arfvedsonite, aegirine, hedenbergite, and ilmenite. From the whole rock and mineral compositions, we conclude that the pre-eruptive temperatures were between 800 °C and 900 °C, but probably closer to 850 °C to 900 °C. The Fe-rich mafic mineral compositions and absence of magnetite indicate that the relative oxidation state of the melt was below the fayalite-magnetite-quartz buffer. The estimated relative oxidation state is calculated to range from ∆FMQ –1.1 to ∆FMQ – 2.8. The water content of the magma was likely close to or at saturation (i.e. H2O ≈ 3.2 wt%) whereas the fluorine content was likely less than saturation (i.e. Fmeltwt% < 0.6 wt%) due to the absence of magmatic fluo-rite. The pre-eruptive magma was likely volatile-rich, but underwent a period of significant degassing prior to or during eruption that led to a drier lava with higher viscosity, lower effusivity that allowed for slow cooling, the development of columnar joints, and the crystallization of hypersolvus feldspar.
AB - The Late Cretaceous (74.4 ± 1.3 Ma) peralkaline rhyolite from Hadjer el Khamis erupted during a period of rifting within the Bornu and Termit basins of the Lake Chad region. The rhyolites are representative of a residual silicic magma that was derived by fractional crystallization of mantle derived basaltic parental magma. The primary phenocrysts of the rocks are quartz, alkali feldspar, arfvedsonite, aegirine, hedenbergite, and ilmenite. From the whole rock and mineral compositions, we conclude that the pre-eruptive temperatures were between 800 °C and 900 °C, but probably closer to 850 °C to 900 °C. The Fe-rich mafic mineral compositions and absence of magnetite indicate that the relative oxidation state of the melt was below the fayalite-magnetite-quartz buffer. The estimated relative oxidation state is calculated to range from ∆FMQ –1.1 to ∆FMQ – 2.8. The water content of the magma was likely close to or at saturation (i.e. H2O ≈ 3.2 wt%) whereas the fluorine content was likely less than saturation (i.e. Fmeltwt% < 0.6 wt%) due to the absence of magmatic fluo-rite. The pre-eruptive magma was likely volatile-rich, but underwent a period of significant degassing prior to or during eruption that led to a drier lava with higher viscosity, lower effusivity that allowed for slow cooling, the development of columnar joints, and the crystallization of hypersolvus feldspar.
KW - Chad
KW - Late Cretaceous
KW - mineral chemistry
KW - peralkaline rhyolite
KW - temperature
KW - ƒO
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U2 - 10.1127/njma/2022/0338
DO - 10.1127/njma/2022/0338
M3 - Article
AN - SCOPUS:85137748721
SN - 0077-7757
VL - 198
SP - 25
EP - 44
JO - Neues Jahrbuch fur Mineralogie, Abhandlungen
JF - Neues Jahrbuch fur Mineralogie, Abhandlungen
IS - 1
ER -