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cristobalite
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A triangular phase diagram shows the melting relationships among quartz, kalsilite, and forsterite, with labeled regions for minerals like cristobalite, protoenstatite, leucite, sanidine, and tridymite, and temperature lines marking melting points in degrees Celsius.
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Basalt sample returned by Apollo 15, from near a long sinous lunar valley called Hadley Rille. Measured at 3.3 years old.
(Bed) Rocks and (Flint) Stones
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cristobalite

mineral
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cristobalite, the stable form of silica (silicon dioxide, SiO2) between its melting point of 1,728° C (3,142° F) and 1,470° C (2,678° F), below which tridymite is the stable form. Cristobalite has two modifications: low-cristobalite, which occurs naturally up to 268° C (514° F) but is not stable; and high-cristobalite, which occurs above 268° C but is only stable above 1,470° C. Natural low-cristobalite usually occurs in sub-microcrystalline masses (see opal) or fibrous to columnar spherulites (see lussatite) in igneous rocks. Cristobalite has the same chemical composition as coesite, stishovite, quartz, and tridymite but has a different crystal structure. For detailed physical properties, see silica mineral (table).

This article was most recently revised and updated by John P. Rafferty.