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ungrouped chondrite comparison table
Subject has sediment mechanism has weather resistance has metal abundance has part mean Ni content of sulfide has degree of shock metamorphism fragment has age has shock stage has refractory inclusion abundance survive fall if is an instance of vaporize completely if has part feldspar has fragmentation probability has part metal maximum bulk be associated with has fall location has fall date has metamorphism mechanism has impact angle has degree of secondary process has name has shock diagnostic mineral is independent of has olivine shock metamorphism has genesi has chondrule glass type has weather be shock has weathering stage has homogeneity of olivine and low Ca pyroxene has acronym has chondrule abundance has relative abundance shatter has texture has part chondrule has value has total mass of find has structural state of low Ca pyroxene has impact velocity 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 fall coordinate has part carbon has composition has monetary value has original mass has part mineral has find date has part water has mass has image has origin has number of find has ablative mass loss produce has shock pressure has chondrule mean diameter have crater image has fall map
HaH 180agglomeration of particles, many of which record individual, diverse historieswhich depends on its compositionin volume %in weight %very weakly shockedduring meteor phaseoldest and most primitive rock in solar systemS2in volume %it fragments because smaller pieces with less mass are more easily slowed by the atmosphereS2 shock stage chondritesize is between 3 micrometers and 3 millimetersusually plagioclase tectosilicateduring meteor phase which depends on compositionin weight %craterHammadah al Hamrarecorded by eyewitness or inferred from dating methodsshock metamorphism providing insight into geological evolution of parent asteroidHaH 180orthopyroxene for enstatite chondritethe nature and degree of thermal metamorphism or aqueous alterationundulatory extinction, irregular fractures  can be severe due to long exposure time to environmental corrosion agentsbefore, during or after other types of metamorphismW4definition goes hereHaHin volume %85.7 % of meteorite fallsduring impact phase small sphere of about 1 mm diameter of formerly melted mineralslower because the fall was not witnessed27 kgdefinition goes herewhen it hits the ground which is smaller than its velocity before it enters the atmosphereless than 950 degree Celsius during its entire history since solidificationundulatory extinction, irregular fracturesundulatory extinction, irregular fractures, some planar fracturesasteroid 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 metamorphism28° 36.21' N., 13° 18.04' E.in weight %often minerals not found on Earthlarge if the fall was witnessedwhich can over an order of magnitude greater than total mass of fragment(s) collected at the impact site April 1996in weight %0.936 kg
meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal3directly proportional to initial velocitypower outages and failures in electrical equipment due to EMP (electromagnetic pulse)5 to 10 GPamillimeters which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity

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