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The Complicated Geologic History of Asteroid 4 Vesta. Spectral studies of the HED meteorites show that they likely come from asteroid 4 Vesta. HED stands for: Howardites, which are mixtures of: Eucrites (basaltic lava flows) Diogenites (orthopyroxenites) - PowerPoint PPT Presentation
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Granite-like samples of Vesta COSMOCHEMISTRY iLLUSTRATED
The Complicated Geologic History The Complicated Geologic History
of Asteroid 4 Vestaof Asteroid 4 Vesta• Spectral studies of the HED
meteorites show that they likely come from asteroid 4 Vesta.
• HED stands for: - Howardites, which are mixtures of: - Eucrites (basaltic lava flows) - Diogenites (orthopyroxenites)
• The howardites contain rock and mineral fragments, and impact-produced glasses
• The glass fragments and spherules record the compositions of a wide range of lithologies on Vesta
Granite-like samples of Vesta COSMOCHEMISTRY iLLUSTRATED
The Complicated Geologic History The Complicated Geologic History
of Asteroid 4 Vestaof Asteroid 4 Vesta• Rock samples of eucrites
plot in the basalt field on this widely-used diagram to classify igneous rocks.
• Most glasses are similar to the rocks, but are enriched in alkalis
• A few glasses are enriched in SiO2 and alkalis, falling into the dacite field (≈ granite)
• This indicates that extensive fractional crystallization of magmas occurred on Vesta
Granite-like samples of Vesta COSMOCHEMISTRY iLLUSTRATED
The Complicated Geologic History The Complicated Geologic History
of Asteroid 4 Vestaof Asteroid 4 VestaAn interesting picture of Vesta:
• Metamorphism• Intrusions into the crust:
magmatic differentiation, contact metamorphism
• Partial melting of the crust in some places
• Magma mixing between crustal partial melts and eucrite basalt magma
• Eucrite basalt magma migration through crust
• Granites could form in intrusions or in the residual magma ocean