Subject |
has part mean Ni content of sulfide |
has weather resistance |
has part carbon |
has olivine shock metamorphism |
has part matrix |
has prototype |
is independent of |
has shock pressure |
has degree of aqueous alteration |
has matrix abundance |
has sediment mechanism |
has image |
has weather |
has distinguishing feature |
has degree of secondary process |
has part feldspar |
has metal abundance |
has refractory inclusion abundance |
has relative abundance |
has fragmentation probability |
has chondrule mean diameter |
has metamorphism mechanism |
has fall date |
have composition |
has fall description |
is a kind of |
has chondrule glass type |
has age |
has part sulfide Ni content |
has part maximum bulk Ni in metal |
has definition |
has number of find |
has petrologic type |
has part water |
has orthopyroxene shock metamorphism |
has plagioclase shock metamorphism |
has degree of shock metamorphism |
has abundance |
has peak temperature |
has shock diagnostic mineral |
has name |
be shock |
has fall location |
is an instance of |
has tenacity |
has shock stage |
has part metal maximum bulk |
has homogeneity of olivine and low Ca pyroxene |
has structural state of low Ca pyroxene |
has value |
has fall coordinate |
has olivine and low Ca pyroxene homogeneity |
has ablative mass loss |
has total mass of find |
has chondrule abundance |
has parent body |
has part chondrule |
has petrologic type range |
CM chondrite | in weight % | low | 0.8 to 2.6 % by weight | | mostly fine, opaque | Mighei meteorite | | | moderate | 70 % by volume | agglomeration of particles, many of which record individual, diverse histories | | | elemental carbon | providing insight into geological evolution of parent asteroid | minor primary grains only | 0.1 % by volume | 5 % by volume | 8 % of meteorite falls | high because it is more friable than iron meteorite | 0.3 millimeters | aqueous altermation | recorded by eyewitness or inferred from dating methods | | | type 2 chondrite | rare | oldest and most primitive rock in solar system | greater than 0.5 % by weight | less than 20 % by weight; taenite minor or absent | | 36 | 2 | 2 to 16 % by weight | | | | rare relative to other chondrite types | less than 950 degree Celsius during its entire history since solidification | | 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 | | friable | | in weight % | definition goes here | predominantly monoclinic | | in degrees, minutes and seconds of lattitude and longitude | greater than 5 % deviations | high because it is more friable than iron meteorite | 2577 kg | 20 % by volume | asteroid smaller than 100 km in diameter | chondrules very sharply defined | which depends on degree of aqueous alteration and thermal metamorphism |
meteorite fall | | which depends on its composition | | | | | | | | | | | negligible due to quick recovery of meteorite before corrosion begins | | | | | | | during meteor phase which depends on composition | | | recorded by eyewitness or instruments | | what witnesses saw or what was recorded by instruments | meteorite | | | | | a meteorite whose fall was witnessed by human or electronic means | 1691 | | | | | | | | | 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 | | | | | | | higher because the fall was witnessed | in degrees, minutes and seconds of lattitude and longitude | | directly proportional to initial velocity | 485755 kg | | | | |
S1 shock stage chondrite | in weight % | which depends on its composition | in weight % | sharp optical extinction, irregular fractures | fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents | | the nature and degree of thermal metamorphism or aqueous alteration | less than 5 GPa | | in volume % | agglomeration of particles, many of which record individual, diverse histories | | | | providing insight into geological evolution of parent asteroid | usually plagioclase tectosilicate | in volume % | in volume % | | during meteor phase which depends on composition | millimeters | shock metamorphism | recorded by eyewitness or inferred from dating methods | | | S1 shock stage meteorite | | oldest and most primitive rock in solar system | | | | 1691 | | in weight % | sharp optical extinction, irregular fractures | sharp optical extinction, irregular fractures | unshocked | | less than 950 degree Celsius during its entire history since solidification | orthopyroxene for enstatite chondrite | based on the locale, region, or nearby town in which the fall occurred | before, during or after other types of metamorphism | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | | | S1 | in weight % | definition goes here | definition goes here | | in degrees, minutes and seconds of lattitude and longitude | | directly proportional to initial velocity | 485755 kg | in volume % | asteroid smaller than 100 km in diameter | small sphere of about 1 mm diameter of formerly melted minerals | which depends on degree of aqueous alteration and thermal metamorphism |
Murchison | in weight % | which depends on its composition | 0.8 to 2.6 % by weight | sharp optical extinction, irregular fractures | mostly fine, opaque | Mighei meteorite | the nature and degree of thermal metamorphism or aqueous alteration | less than 5 GPa | moderate | 70 % by volume | agglomeration of particles, many of which record individual, diverse histories |
 | negligible due to quick recovery of meteorite before corrosion begins | elemental carbon | providing insight into geological evolution of parent asteroid | minor primary grains only | 0.1 % by volume | 5 % by volume | | during meteor phase which depends on composition | 0.3 millimeters | shock metamorphism | September 28, 1969 10:45 am | contain amino acids | what witnesses saw or what was recorded by instruments | | rare | oldest and most primitive rock in solar system | greater than 0.5 % by weight | less than 20 % by weight; taenite minor or absent | | 1691 | 2 | 2 to 16 % by weight | sharp optical extinction, irregular fractures | sharp optical extinction, irregular fractures | unshocked | rare relative to other chondrite types | less than 950 degree Celsius during its entire history since solidification | orthopyroxene for enstatite chondrite | Murchison | before, during or after other types of metamorphism | Murchison, Victoria, Australia | S1 shock stage chondrite | friable | S1 | in weight % | definition goes here | predominantly monoclinic | higher because the fall was witnessed | 36° 37' S., 145° 12' E. | greater than 5 % deviations | directly proportional to initial velocity | 485755 kg | 20 % by volume | asteroid smaller than 100 km in diameter | chondrules very sharply defined | which depends on degree of aqueous alteration and thermal metamorphism |