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rock > metamorphic rock > altered chondrite > shocked chondrite > S2 shock stage chondrite > HaH 180
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HaH 180 comparison table
Subject has sediment mechanism has weather resistance has metal abundance has part mean Ni content of sulfide has degree of shock metamorphism has age has refractory inclusion abundance has shock stage is an instance of has part feldspar has part metal maximum bulk has fragmentation probability has fall location has metamorphism mechanism has degree of secondary process has name has shock diagnostic mineral is independent of has olivine shock metamorphism has weather has weathering stage be shock has homogeneity of olivine and low Ca pyroxene has acronym has chondrule abundance has relative abundance has part chondrule has value 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 fall coordinate has part carbon is a kind of has find date has part water has mass has image has number of find has ablative mass loss has shock pressure has chondrule mean diameter
Hammadah al Hamra meteorite which depends on its composition         during meteor phase which depends on compositionHammadah al Hamra  based on the locale, region, or nearby town in which the fall occurred   can be severe due to long exposure time to environmental corrosion agents   HaH   lower because the fall was not witnessed485755 kg        in degrees, minutes and seconds of lattitude and longitude Sahara meteoritewhen the meteorite was found   1691directly proportional to initial velocity  
S2 shock stage chondriteagglomeration of particles, many of which record individual, diverse historieswhich depends on its compositionin volume %in weight %very weakly shockedoldest and most primitive rock in solar systemin volume %S2 usually plagioclase tectosilicatein weight %during meteor phase which depends on compositionstrewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocityshock metamorphismproviding insight into geological evolution of parent asteroidbased on the locale, region, or nearby town in which the fall occurredorthopyroxene for enstatite chondritethe nature and degree of thermal metamorphism or aqueous alterationundulatory extinction, irregular fractures  before, during or after other types of metamorphismdefinition goes here in volume % small sphere of about 1 mm diameter of formerly melted minerals 485755 kgdefinition goes hereless 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 metamorphismin degrees, minutes and seconds of lattitude and longitudein weight %S2 shock stage meteorite in weight %  1691directly proportional to initial velocity5 to 10 GPamillimeters
ungrouped chondriteagglomeration of particles, many of which record individual, diverse historieslowin volume %in weight % oldest and most primitive rock in solar systemin volume %  usually plagioclase tectosilicatein weight %high because it is more friable than iron meteoritestrewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity  based on the locale, region, or nearby town in which the fall occurred      definition goes here in volume %85.7 % of meteorite fallssmall sphere of about 1 mm diameter of formerly melted minerals 27 kgdefinition goes hereless than 950 degree Celsius during its entire history since solidification  asteroid 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 metamorphismin degrees, minutes and seconds of lattitude and longitudein weight %chondrite in weight %  3high because it is more friable than iron meteorite millimeters
HaH 180agglomeration of particles, many of which record individual, diverse historieswhich depends on its compositionin volume %in weight %very weakly shockedoldest and most primitive rock in solar systemin volume %S2S2 shock stage chondriteusually plagioclase tectosilicatein weight %during meteor phase which depends on compositionHammadah al Hamrashock metamorphismproviding insight into geological evolution of parent asteroidHaH 180orthopyroxene for enstatite chondritethe nature and degree of thermal metamorphism or aqueous alterationundulatory extinction, irregular fracturescan be severe due to long exposure time to environmental corrosion agentsW4before, during or after other types of metamorphismdefinition goes hereHaHin volume %85.7 % of meteorite fallssmall sphere of about 1 mm diameter of formerly melted mineralslower because the fall was not witnessed27 kgdefinition goes hereless 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 % April 1996in weight %0.936 kg
3directly proportional to initial velocity5 to 10 GPamillimeters

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