LL6 Impact-Melt BrecciaWork in Progress ... A rock that is a mechanical mixture of different minerals and/or rock fragments (clasts). A breccia may also be distinguished by the origin of its clasts: (monomict breccia: monogenetic or monolithologic, and polymict breccia: polygenetic or polylithologic). The proportions of these fragments within the unbrecciated material (LL6 in MetBull 62)
Found 1958 38° 18′ 24′ N., 99° 42′ 36′ W. Initially, a 3 kg fragment was reported to have been found in Rush County, Kansas, about 6.8 km N. of Bison (G. Huss, 1982). Subsequently, meteoriteWork in progress. A solid natural object reaching a planet’s surface from interplanetary space. Solid portion of a meteoroid that survives its fall to Earth, or some other body. Meteorites are classified as stony meteorites, iron meteorites, and stony-iron meteorites. These groups are further divided according to their mineralogy and recovery field work conducted by Terry Schmidt led to the recovery of another 8 kg fragment, a mass which had been found by a farmer in 1938 a few miles from the later 3 kg mass findMeteorite not seen to fall, but recovered at some later date. For example, many finds from Antarctica fell 10,000 to 700,000 years ago.. This larger mass was stored by the farmer under a work bench in his garage during the intervening years.
Bison is an LL6 chondriteChondrites are the most common meteorites accounting for ~84% of falls. Chondrites are comprised mostly of Fe- and Mg-bearing silicate minerals (found in both chondrules and fine grained matrix), reduced Fe/Ni metal (found in various states like large blebs, small grains and/or even chondrule rims), and various refractory inclusions (such with a monomict composition of dark-colored, unmelted clasts containing highly shocked, relict chondrulesRoughly spherical aggregate of coarse crystals formed from the rapid cooling and solidification of a melt at ~1400 ° C. Large numbers of chondrules are found in all chondrites except for the CI group of carbonaceous chondrites. Chondrules are typically 0.5-2 mm in diameter and are usually composed of olivine, along with light-colored impact-melt breccia clasts devoid of chondrules, all embedded within an opaque, blackened host rock. This blackening is primarily the result of shock-induced microscopic troiliteBrass colored non-magnetic mineral of iron sulfide, FeS, found in a variety of meteorites. inclusions and veinlets interspersed throughout the matrixFine grained primary and silicate-rich material in chondrites that surrounds chondrules, refractory inclusions (like CAIs), breccia clasts and other constituents.. The poikilitic texture, depletion of metalElement that readily forms cations and has metallic bonds; sometimes said to be similar to a cation in a cloud of electrons. The metals are one of the three groups of elements as distinguished by their ionization and bonding properties, along with the metalloids and nonmetals. A diagonal line drawn and sulfides, and high CaO content in orthopyroxeneOrthorhombic, low-Ca pyroxene common in chondrites. Its compositional range runs from all Mg-rich enstatite, MgSiO3 to Fe-rich ferrosilite, FeSiO3. These end-members form an almost complete solid solution where Mg2+ substitutes for Fe2+ up to about 90 mol. % and Ca substitutes no more than ~5 mol. % (higher Ca2+ contents occur present in the light-colored clasts of Bison are all consistent with a rapid crystallizationPhysical or chemical process or action that results in the formation of regularly-shaped, -sized, and -patterned solid forms known as crystals. from a melt (Dominik and Bussy, 1994). A two-stage shock history has been suggested: 1) the first impact caused localized impact melting and brecciationThe formation of a breccia through a process by which rock fragments of of various types are recemented or fused together.; and 2) a subsequent impact produced features of shock stageA petrographic assessment, using features observed in minerals grains, of the degree to which a meteorite has undergone shock metamorphism. The highest stage observed in 25% of the indicator grains is used to determine the stage. Also called "shock level". S4. In an Ar–Ar dating study of two LL chondritesChondrites are the most common meteorites accounting for ~84% of falls. Chondrites are comprised mostly of Fe- and Mg-bearing silicate minerals (found in both chondrules and fine grained matrix), reduced Fe/Ni metal (found in various states like large blebs, small grains and/or even chondrule rims), and various refractory inclusions (such, Weirich et al. (2009) determined an age of ~1 b.y., possibly reflecting the last major impact on the LL chondriteOrdinary chondrites ("low Fe" / "low metal") with only 1 to 3% free metal. Their olivine is more Fe-rich than in the other ordinary chondrites (Fa27-32), implying that the LL types must have formed under more oxidizing conditions than their H or L cousins. Orthopyroxene compositions are also Fe-the richparent bodyThe body from which a meteorite or meteoroid was derived prior to its ejection. Some parent bodies were destroyed early in the formation of our Solar System, while others like the asteroid 4-Vesta and Mars are still observable today..
Bison has experienced a low degree of weathering. Shown above is a 13.79 g partial end section of Bison showing its brecciated structure.