Subject |
has iron metal and iron sulfide |
has sediment mechanism |
has weather resistance |
has metal abundance |
has part mean Ni content of sulfide |
has alteration temperature range |
has age |
has refractory inclusion abundance |
is an instance of |
has total iron content |
has olivine and low Ca pyroxene homogeneity |
has part feldspar |
has fragmentation probability |
has metal iron content |
has part metal maximum bulk |
has fall location |
has metamorphism mechanism |
has degree of secondary process |
has name |
has chondrule glass type |
has weather |
has homogeneity of olivine and low Ca pyroxene |
has chondrule abundance |
has relative abundance |
has part chondrule |
has abundance |
has value |
has total mass of find |
has structural state of low Ca pyroxene |
has peak temperature |
has parent body |
has part matrix |
has degree of thermal metamorphism |
has fall coordinate |
has matrix abundance |
has petrologic type range |
has part carbon |
has petrologic type |
has part maximum bulk Ni in metal |
is a kind of |
has comment |
has find date |
has part water |
has image |
has number of find |
has ablative mass loss |
has synonym |
has definition |
has chondrule mean diameter |
has part sulfide Ni content |
L5 chondrite | 50 % of total iron | agglomeration of particles, many of which record individual, diverse histories | low | 5 % by volume | in weight % | the range over at which the alteration took place | oldest and most primitive rock in solar system | 0.1 to 1 % by volume | | low | homogeneous | secondary, 2 to 50 micron grains | high because it is more friable than iron meteorite | 5 to 10 % | in weight % | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | thermal metamorphism | providing insight into geological evolution of parent asteroid | based on the locale, region, or nearby town in which the fall occurred | devitrified, absent | | definition goes here | 60 to 80 % by volume | 85.7 % of meteorite falls | chondrules readily delineated | most common chondrite observed from falls | | 1256 kg | less than 20 % monoclinic | less than 950 degree Celsius during its entire history since solidification | asteroid smaller than 100 km in diameter | transparent, recrystallized, moderate size crystals | moderate | in degrees, minutes and seconds of lattitude and longitude | 10 to 15 % by volume | which depends on degree of aqueous alteration and thermal metamorphism | less than 0.2 % by weight | 5 | greater than 20 % by weight, kamacite and taenite in exsolution relationship | type 5 chondrite | | | less than 1.5 % by weight | | 44 | high because it is more friable than iron meteorite | hypersthene chondrite | | 0.7 millimeters | less than 0.5 % by weight |
meteorite find | | | which depends on its composition | | | | | | | | | | during meteor phase which depends on composition | | | strewn 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 | | can be severe due to long exposure time to environmental corrosion agents | | | | | | lower because the fall was not witnessed | 485755 kg | | | | | | in degrees, minutes and seconds of lattitude and longitude | | | | | | meteorite | | when the meteorite was found | | | 1691 | directly proportional to initial velocity | | a meteorite whose fall was not witnessed | | |
Cat Mountain | 50 % of total iron | agglomeration of particles, many of which record individual, diverse histories | which depends on its composition | 5 % by volume | in weight % | the range over at which the alteration took place | oldest and most primitive rock in solar system | 0.1 to 1 % by volume | meteorite find | low | homogeneous | secondary, 2 to 50 micron grains | during meteor phase which depends on composition | 5 to 10 % | in weight % | Tucson, Arizona | thermal metamorphism | providing insight into geological evolution of parent asteroid | Cat Mountain | devitrified, absent | can be severe due to long exposure time to environmental corrosion agents | definition goes here | 60 to 80 % by volume | | chondrules readily delineated | most common chondrite observed from falls | lower because the fall was not witnessed | 1256 kg | less than 20 % monoclinic | less than 950 degree Celsius during its entire history since solidification | asteroid smaller than 100 km in diameter | transparent, recrystallized, moderate size crystals | moderate | 32° 8.9' N., 111° 6.7' W. | 10 to 15 % by volume | which depends on degree of aqueous alteration and thermal metamorphism | less than 0.2 % by weight | 5 | greater than 20 % by weight, kamacite and taenite in exsolution relationship | | Impact Melt Breccia | 1980/81 | less than 1.5 % by weight |
 | 44 | directly proportional to initial velocity | hypersthene chondrite | | 0.7 millimeters | less than 0.5 % by weight |