medium shock ureilite | | greater extent of fracturing, undulatory extinction, and kink banding | | | olivine, pyroxene (some combination of pigeonite, orthopyroxene, augite) | medium | | | S4-S6 | no chondrules | | | reduced rims contacting carbonaceous matrix material 0.1 mm FeO-free olivine and/or enstatite rims riddled with tiny inclusions of low-Ni metal | may be cloudy due to glassy inclusions | partial melting residue | | cooling in deep underground chambers | | diamonds and/or lonsdaleite | sub-grain boundaries may be prominent | | | | AURE | | | 9 kg (out of date) | | | | | | | | | carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume | | olivine-pigeonite about 90% by volume | S6 shock stage meteorite | | 6 (out of date) | asteroid | from 20 GPa to 100 GPa | very slow | | coarse-grained granular |
S4 shock stage chondrite | agglomeration of particles, many of which record individual, diverse histories | | in volume % | in weight % | | moderately shocked | oldest and most primitive rock in solar system | in volume % | S4 | | usually plagioclase tectosilicate | in weight % | | | | providing insight into geological evolution of parent asteroid | | the nature and degree of thermal metamorphism or aqueous alteration | orthopyroxene for enstatite chondrite | weak mosaicism, planar fractures | | before, during or after other types of metamorphism | definition goes here | | in volume % | small sphere of about 1 mm diameter of formerly melted minerals | 485755 kg | definition goes here | less than 950 degree Celsius during its entire history since solidification | undulatory extinction, partially isotropic, planar deformation features | weak mosaicism, twinning on (100), planar fractures | asteroid smaller than 100 km in diameter | fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents | in volume % | which depends on degree of aqueous alteration and thermal metamorphism | | in weight % | | S4 shock stage meteorite | in weight % | 1691 | meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal | 30 to 35 GPa | | millimeters | |