Subject |
has sediment mechanism |
has oxidized iron content |
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 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 part chondrule |
has oxidation state |
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 matrix abundance |
has petrologic type range |
has fall coordinate |
has part carbon |
has petrologic type |
has part maximum bulk Ni in metal |
is a kind of |
has find date |
has part water |
has mass |
has image |
has number of find |
has synonym |
has definition |
has chondrule mean diameter |
has part sulfide Ni content |
EL6 chondrite | agglomeration of particles, many of which record individual, diverse histories | zero | 15 % 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, grains greater than 50 microns | 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 | chondrules poorly defined | highly reduced with very little FeO | | 59 kg | orthorhombic | less than 950 degree Celsius during its entire history since solidification | asteroid smaller than 100 km in diameter | transparent, recrystallized, coarse crystals | strong | less than 2 to 15 % by volume | which depends on degree of aqueous alteration and thermal metamorphism | in degrees, minutes and seconds of lattitude and longitude | less than 0.2 % by weight | 3 to 6 | greater than 20 % by weight, kamacite and taenite in exsolution relationship | E6 chondrite | | less than 1.5 % by weight | | | 8 | E chondrite | | 0.6 millimeters | less than 0.5 % by weight |
meteorite find | | | | | | | | | | | | | 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 | | a meteorite whose fall was not witnessed | | |
Yilmia | agglomeration of particles, many of which record individual, diverse histories | zero | 15 % 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, grains greater than 50 microns | in weight % | Western Australia | thermal metamorphism | providing insight into geological evolution of parent asteroid | Yilmia | devitrified, absent | can be severe due to long exposure time to environmental corrosion agents | definition goes here | 60 to 80 % by volume | chondrules poorly defined | highly reduced with very little FeO | lower because the fall was not witnessed | 485755 kg | orthorhombic | less than 950 degree Celsius during its entire history since solidification | asteroid smaller than 100 km in diameter | transparent, recrystallized, coarse crystals | strong | less than 2 to 15 % by volume | which depends on degree of aqueous alteration and thermal metamorphism | 31° 11' 30" S., 121° 32' E. | less than 0.2 % by weight | 3 to 6 | greater than 20 % by weight, kamacite and taenite in exsolution relationship | | 1969 | less than 1.5 % by weight | 24 kg |
 | 1691 | E chondrite | | 0.6 millimeters | less than 0.5 % by weight |