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  2. Peridot - Wikipedia

    en.wikipedia.org/wiki/Peridot

    Oxidation of peridot does not occur at natural surface temperature and pressure but begins to occur slowly at 600 °C (870 K) with rates increasing with temperature. [7] The oxidation of the olivine occurs by an initial breakdown of the fayalite component, and subsequent reaction with the forsterite component, to give magnetite and orthopyroxene.

  3. Peridotite - Wikipedia

    en.wikipedia.org/wiki/Peridotite

    Peridotite. Peridotite (US: / ˈpɛrɪdoʊˌtaɪt, pəˈrɪdə -/ PERR-ih-doh-tyte, pə-RID-ə-) is a dense, coarse-grained igneous rock consisting mostly of the silicate minerals olivine and pyroxene. Peridotite is ultramafic, as the rock contains less than 45% silica. It is high in magnesium (Mg 2+), reflecting the high proportions of ...

  4. Peridot Mesa - Wikipedia

    en.wikipedia.org/wiki/Peridot_Mesa

    Peridot Mesa. The Peridot Mesa vent is a part of the San Carlos volcanic field located in San Carlos, Arizona, United States on the San Carlos Apache Indian Reservation. The mesa is about 3 km (1.9 mi) in diameter and is capped by a basalt flow 3 to 6 meters thick that originated from a volcanic cone located in the Southwest corner of the mesa.

  5. List of gemstones by species - Wikipedia

    en.wikipedia.org/wiki/List_of_gemstones_by_species

    Gadolinite; Gahnite; Gahnospinel; Garnet group: Pyralspite. Almandine; Pyrope; Spessartine; Ugrandite. Andradite. Demantoid; Melanite; Topazolite; Grossular ...

  6. Gemstone irradiation - Wikipedia

    en.wikipedia.org/wiki/Gemstone_irradiation

    C Irradiated by different doses and then annealed at 800 °C (1,470 °F) Gemstone irradiation is a process in which a gemstone is exposed to artificial radiation in order to enhance its optical properties. High levels of ionizing radiation can change the atomic structure of the gemstone's crystal lattice, which in turn alters the optical ...

  7. Pallasite - Wikipedia

    en.wikipedia.org/wiki/Pallasite

    Pallasite. A slice of the Esquel pallasite, clearly showing the large olivine crystals suspended in the metal matrix. The pallasites are a class of stony–iron meteorite. They are relatively rare, and can be distinguished by the presence of large olivine crystal inclusions in the ferro-nickel matrix.