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rock > metamorphic rock > shocked meteorite > S6 shock stage meteorite
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S6 shock stage meteorite comparison table
Subject has sediment mechanism has shock texture has metal abundance has part mean Ni content of sulfide has minerology has degree of shock metamorphism has age has refractory inclusion abundance has shock stage has distinguishing feature has part feldspar has part metal maximum bulk has olivine grain characteristic has pyroxene shock metamorphism has likely origin has degree of secondary process has solidification mechanism is independent of has shock diagnostic mineral has olivine shock metamorphism has chondrule glass type be shock has homogeneity of olivine and low Ca pyroxene has letter designation has chondrule abundance has part chondrule has total mass of find has structural state of low Ca pyroxene has peak temperature has plagioclase shock metamorphism has orthopyroxene shock metamorphism has parent body has part matrix has matrix abundance has petrologic type range has matrix composition has part carbon has characteristic mineral has part water has number of find has origin has shock pressure has solidification timescale has chondrule mean diameter has petrology
medium shock ureilite greater extent of fracturing, undulatory extinction, and kink banding  olivine, pyroxene (some combination of pigeonite, orthopyroxene, augite)medium  S4-S6no chondrules  reduced rims contacting carbonaceous matrix material 0.1 mm FeO-free olivine and/or enstatite rims riddled with tiny inclusions of low-Ni metalmay be cloudy due to glassy inclusionspartial melting residue cooling in deep underground chambers diamonds and/or lonsdaleitesub-grain boundaries may be prominent   AURE  9 kg (out of date)        carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume olivine-pigeonite about 90% by volume 6 (out of date)asteroidfrom 20 GPa to 100 GPavery slow coarse-grained granular
S6 shock stage chondriteagglomeration of particles, many of which record individual, diverse histories in volume %in weight % very strongly shockedoldest and most primitive rock in solar systemin volume %S6 usually plagioclase tectosilicatein weight %   providing insight into geological evolution of parent asteroid the nature and degree of thermal metamorphism or aqueous alterationorthopyroxene for enstatite chondritesolid state recrystallization and staining, ringwoodite, melting before, during or after other types of metamorphismdefinition goes here in volume %small sphere of about 1 mm diameter of formerly melted minerals485755 kgdefinition goes hereless than 950 degree Celsius during its entire history since solidificationshock melted (normal glass)majorite, meltingasteroid smaller than 100 km in diameterfine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituentsin volume %which depends on degree of aqueous alteration and thermal metamorphism in weight % in weight %1691meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal75 to 90 GPa millimeters 

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