Mundrabilla | in weight % | low | 0.2 to 1 % by weight | 1.6 % by volume | clastic and minor opaque | 48.5 % by volume | Vigarano meteorite | 7.47 % by weight | weak | 40 % by volume | agglomeration of particles, many of which record individual, diverse histories |
 | elemental carbon | minor primary grains only | 0 to 5 % by volume | 10 % by volume | 8 % of meteorite falls | high because it is more friable than iron meteorite | 1.0 millimeters | 7.72% Ni, 59.5 ppm Ga, 196 ppm Ge, 0.87 ppm Ir | clear, isotropic, variable abundance | oldest and most primitive rock in solar system | less than 0.5 % by weight | greater than 20 % by weight, kamacite and taenite in exsolution relationship | 30.5 % by volume | Of | 36 | 3 | 1911 | 0.3 to 3 % by weight | 14.9 % by volume | none | rare relative to other chondrite types | 0.12 % by volume | less than 950 degree Celsius during its entire history since solidification | 0.69 % by volume | Mundrabilla | 0.6 mm (fine) | Mundrabilla, Nullarbor Plain, Western Australia | CV chondrite | % by volume | in weight % | definition goes here | 3.7 % by volume | iron-rich olivine, calcium aluminum inclusions | predominantly monoclinic | | Latitude 30 degrees 47 minutes South, Longitude 127 degrees 33 minutes East | greater than 5 % deviations | high because it is more friable than iron meteorite | 2577 kg | 45 % by volume | asteroid smaller than 100 km in diameter | chondrules very sharply defined | which depends on degree of aqueous alteration and thermal metamorphism |
Persimmon Creek | | high | | % by volume | | 23.4 % by volume | Mundrabilla meteorite | 6.4 % by weight | | | | | | | | | 5.7 % of meteorite falls | low because it is tougher than stony meteorite | | | | | | | 22.1 % by volume | | 532 | | | | 2.0 % by volume | | | 43.7 % by volume | | 6.8 % by volume | Persimmon Creek | | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | sulfide-rich IAB iron | 0.67 % by volume | | | 1.4 % by volume | high in troilite | | irregular masses | in degrees, minutes and seconds of lattitude and longitude | | low because it has higher tensile strength than stony meteorite | 454624 kg | | | | |
Pitts | | high | | % by volume | | 21.3 % by volume | Mundrabilla meteorite | 6.4 % by weight | | | | | | | | | 5.7 % of meteorite falls | low because it is tougher than stony meteorite | | | | | | | 51.7 % by volume | | 532 | | | | 1.9 % by volume | | | 11.5 % by volume | | 10.6 % by volume | Pitts | | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | sulfide-rich IAB iron | 0.15 % by volume | | | 2.8 % by volume | high in troilite | | irregular masses | in degrees, minutes and seconds of lattitude and longitude | | low because it has higher tensile strength than stony meteorite | 454624 kg | | | | |
Zagora | | high | | % by volume | | 22.2 % by volume | Mundrabilla meteorite | 6.4 % by weight | | | | | | | | | 5.7 % of meteorite falls | low because it is tougher than stony meteorite | | | | | | | 2.8 % by volume | | 532 | | | | 4.4 % by volume | | | 65.7 % by volume | | 2.8 % by volume | 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 | sulfide-rich IAB iron | 0.58 % by volume | | | 1.6 % by volume | high in troilite | | veins | in degrees, minutes and seconds of lattitude and longitude | | low because it has higher tensile strength than stony meteorite | 454624 kg | | | | |