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the information about silica concentrations collected by the spacecraft is likely more reliable than the silica information gleaned from infrared wavelengths detected from Mars's surface.
high silica concentrations on Mars likely formed from a different process than that which formed the crusts of other planets.
having a clearer understanding of the composition of Mars's crust and the processes by which it formed will provide more insight into how Earth's crust formed.
Mars's crust likely formed as a result of other major geological events in addition to the cooling of a magma ocean.