Subject |
has weather resistance |
has synonym |
has olivine shock metamorphism |
has prototype |
is independent of |
has shock pressure |
has acronym |
has matrix abundance |
has weather |
has image |
has distinguishing feature |
has metal abundance |
has refractory inclusion abundance |
has relative abundance |
has fragmentation probability |
has oxidized iron content |
has chondrule mean diameter |
has weathering stage |
is a kind of |
has oxidation state |
has total iron content |
has number of find |
has find date |
has comment |
has orthopyroxene shock metamorphism |
has plagioclase shock metamorphism |
has iron metal and iron sulfide |
has degree of shock metamorphism |
has mass |
has abundance |
has shock diagnostic mineral |
has name |
be shock |
has fall location |
is an instance of |
has shock stage |
has composition |
has value |
has fall coordinate |
has ablative mass loss |
has total mass of find |
has chondrule abundance |
has metal iron content |
CK4 chondrite | low | | | ??? meteorite | | | | 75 % by volume | | | elemental carbon | 0.01 % by volume | 4 % by volume | 8 % of meteorite falls | high because it is more friable than iron meteorite | | 0.7 millimeters | | type 4 chondrite | | | 36 | | | | | | | | rare relative to other chondrite types | | based on the locale, region, or nearby town in which the fall occurred | | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | | | often minerals not found on Earth | | in degrees, minutes and seconds of lattitude and longitude | high because it is more friable than iron meteorite | 2577 kg | 15 % by volume | |
E4 chondrite | which depends on its composition | E chondrite | | | | | | in volume % | | | | in volume % | in volume % | | during meteor phase which depends on composition | zero | millimeters | | type 4 chondrite | highly reduced with very little FeO | | 5 | | | | | | | | | | based on the locale, region, or nearby town in which the fall occurred | | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | | | often minerals not found on Earth | | in degrees, minutes and seconds of lattitude and longitude | directly proportional to initial velocity | 143 kg | in volume % | |
H4 chondrite | low | bronzite chondrite | | | | | | 10 to 15 % by volume | | | | 10 % by volume | 0.1 to 1 % by volume | 85.7 % of meteorite falls | high because it is more friable than iron meteorite | | 0.3 millimeters | | type 4 chondrite | | high | 37 | | | | | 75 % of total iron | | | most common chondrite observed from falls | | based on the locale, region, or nearby town in which the fall occurred | | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | | | often minerals not found on Earth | | in degrees, minutes and seconds of lattitude and longitude | high because it is more friable than iron meteorite | 1251 kg | 60 to 80 % by volume | 12 to 21 % |
HaH 119 | which depends on its composition | rumurutiite | planar fractures, undulatory extinction, irregular fractures | Rumuruti meteorite | the nature and degree of thermal metamorphism or aqueous alteration | 15 to 20 GPa | HaH | 36 % by volume | can be severe due to long exposure time to environmental corrosion agents |
 | | 0.1 % by volume | 0 % by volume | | during meteor phase which depends on composition | | 0.4 millimeters | W4 | | highly oxidized | | 1691 | April 1995 | unbecciated | clinoenstatite lamellae on (100), undulatory extinction, planar fractures, irregular fractures | undulatory extinction | | weakly shocked | 0.352 kg | | orthopyroxene for enstatite chondrite | HaH 119 | before, during or after other types of metamorphism | Hammadah al Hamra | S3 shock stage chondrite | S3 | enriched in 17O isotope | lower because the fall was not witnessed | 28° 30.87' N., 12° 53.81' E. | directly proportional to initial velocity | 485755 kg | greater than 40 % by volume | |
L4 chondrite | low | hypersthene chondrite | | | | | | 10 to 15 % by volume | | | | 5 % by volume | 0.1 to 1 % by volume | 85.7 % of meteorite falls | high because it is more friable than iron meteorite | | 0.7 millimeters | | type 4 chondrite | | low | 21 | | | | | 50 % of total iron | | | most common chondrite observed from falls | | based on the locale, region, or nearby town in which the fall occurred | | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | | | often minerals not found on Earth | | in degrees, minutes and seconds of lattitude and longitude | high because it is more friable than iron meteorite | 1197 kg | 60 to 80 % by volume | 5 to 10 % |
LL4 chondrite | low | amphoterite | | | | | | 10 to 15 % by volume | | | | 2 % by volume | 0.1 to 1 % by volume | 85.7 % of meteorite falls | high because it is more friable than iron meteorite | | 0.9 millimeters | | type 4 chondrite | | low | 2 | | | | | 20 % of total iron | | | most common chondrite observed from falls | | based on the locale, region, or nearby town in which the fall occurred | | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | | | bronzite, olivine and minor oligoclase | | in degrees, minutes and seconds of lattitude and longitude | high because it is more friable than iron meteorite | 124 kg | 60 to 80 % by volume | about 2 % |