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  2. L chondrite - Wikipedia

    en.wikipedia.org/wiki/L_chondrite

    The most abundant minerals are olivine and hypersthene (an orthopyroxene), as well as iron–nickel and troilite. Chromite, sodium-rich feldspar and calcium phosphates occur in minor amounts. Petrologic type 6 dominates, with over 60% of the L chondrites falling into this class. This indicates that the parent body was sizeable enough (greater ...

  3. QAPF diagram - Wikipedia

    en.wikipedia.org/wiki/QAPF_diagram

    QAPF diagram for classification of plutonic rocks. A QAPF diagram is a doubled-triangle plot diagram used to classify intrusive igneous rocks based on their mineralogy.The acronym QAPF stands for "Quartz, Alkali feldspar, Plagioclase, Feldspathoid (Foid)", which are the four mineral groups used for classification in a QAPF diagram.

  4. Chondrule - Wikipedia

    en.wikipedia.org/wiki/Chondrule

    The composition of olivine and pyroxene in chondrules varies widely, although the range is usually narrow within any single chondrule. Some chondrules contain very little iron oxide (FeO), resulting in olivine and pyroxene that are close to forsterite (Mg 2 SiO 4 ) and enstatite (MgSiO 3 ) in composition.

  5. Peridot - Wikipedia

    en.wikipedia.org/wiki/Peridot

    The atomic scale structure of olivine looking along the a axis. Oxygen is shown in red, silicon in pink, and magnesium/iron in blue. A projection of the unit cell is shown by the black rectangle. The molecular structure of peridot consists of isomorphic olivine, silicate, magnesium and iron in an orthorhombic crystal system.

  6. Carbonaceous chondrite - Wikipedia

    en.wikipedia.org/wiki/Carbonaceous_chondrite

    These are compounds that emerged early from the primeval solar nebula, condensed out and represent the oldest minerals formed in the Solar System. [ 3 ] [ 4 ] Some primitive carbonaceous chondrites, such as the CM chondrite Murchison , contain presolar minerals, including moissanite (natural silicon carbide ) and tiny nanometer-sized diamonds ...

  7. Serpentine subgroup - Wikipedia

    en.wikipedia.org/wiki/Serpentine_subgroup

    Serpentine minerals are often formed by the hydration of olivine-rich ultramafic rocks at relatively low temperatures (0 to ~600 °C). [15] The chemical reaction turns olivine into serpentine minerals. They may also have their origins in metamorphic alterations of peridotite and pyroxene.

  8. Dunite - Wikipedia

    en.wikipedia.org/wiki/Dunite

    Dunite may also form by the accumulation of olivine crystals on the floor of large basaltic or picritic magma chambers. These " cumulate " dunites typically occur in thick layers in layered intrusions , associated with cumulate layers of wehrlite , olivine pyroxenite , harzburgite , and even chromitite (a cumulate rock consisting largely of ...

  9. Iddingsite - Wikipedia

    en.wikipedia.org/wiki/Iddingsite

    Iddingsite is a rock that lacks a definite chemical composition, so exact compositions cannot be calculated. An approximated composition for a hypothetical end product of iddingsite has been calculated as being SiO 2 = 16%, Al 2 O 3 = 8%, Fe 2 O 3 = 62% and H 2 O = 14%.