Gibeon | | high | | | 200 microgram/gram | | | | 8.0 % by weight | | | 1.9 microgram/gram | | 0.88 milligram/gram | | planet or asteroid much larger than 100 km in diameter | 2.15 microgram/gram |
 | crystalline iron-nickel alloy | | | | 5.7 % of meteorite falls | low because it is tougher than stony meteorite | | pre-historic times | | greater than several tons | 90% iron, 7.93% Ni, 0.41% Co, 0.04% P, 2.0 ppm Ga, 0.12 ppm Ge, 2.3 ppm Ir | | 7.6 microgram/gram | | | | | 150 microgram/gram | | 39 | 9 nanogram/gram | | 1838 | | | | | | | 0.8 % by weight | | 0.6 microgram/gram | Gibeon | 0.3 ± 0.5 mm (fine) | Great Namaqualand, Namibia, Africa | 140 microgram/gram | type IVA iron meteorite | 8 to 49 kilometers | 11 to 500 degrees C per million years | | 4.0 milligram/gram | | | 4.6 microgram/gram | 0.124 microgram/gram | 5.9 microgram/gram | | | kamacite, taenite | | | Latitude 25 degrees 20 minutes North, Longitude 18 degrees East | | low because it has higher tensile strength than stony meteorite | 22254 kg |
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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 | % by volume | weak | 2.7 microgram/gram | 40 % by volume | 2.1 milligram/gram | agglomeration of particles, many of which record individual, diverse histories | asteroid wide partial melting | 96 microgram/gram |
 | 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 | recorded by eyewitness or inferred from dating methods | | which can over an order of magnitude greater than total mass of fragment(s) collected at the impact site | 7.72% Ni, 59.5 ppm Ga, 196 ppm Ge, 0.87 ppm Ir | | 11 microgram/gram | 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 | 132 microgram/gram | 30.5 % by volume | 36 | 270 nanogram/gram | 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 | 1.6 microgram/gram | Mundrabilla | 0.6 mm (fine) | Mundrabilla, Nullarbor Plain, Western Australia | 16 microgram/gram | CV chondrite | 33 kilometers | 25 degrees C per million years | % by volume | 4.6 milligram/gram | % by volume | in weight % | 3.5 microgram/gram | 400 microgram/gram | 8.2 microgram/gram | 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 | which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity | 45 % by volume | asteroid smaller than 100 km in diameter | chondrules very sharply defined | which depends on degree of aqueous alteration and thermal metamorphism |
type IVA iron meteorite | | high | | | 200 microgram/gram | | | | 8.0 % by weight | | | 1.9 microgram/gram | | 0.88 milligram/gram | | planet or asteroid much larger than 100 km in diameter | 2.15 microgram/gram | | crystalline iron-nickel alloy | | | | 5.7 % of meteorite falls | low because it is tougher than stony meteorite | | recorded by eyewitness or inferred from dating methods | | which can over an order of magnitude greater than total mass of fragment(s) collected at the impact site | | Of octahedrite | 7.6 microgram/gram | | | | | 150 microgram/gram | | 39 | 9 nanogram/gram | | | | | | | | | 0.8 % by weight | | 0.6 microgram/gram | based on the locale, region, or nearby town in which the fall occurred | 0.2 to 0.5 mm (fine) | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | 140 microgram/gram | | 8 to 49 kilometers | 11 to 500 degrees C per million years | | 4.0 milligram/gram | | | 4.6 microgram/gram | 0.124 microgram/gram | 5.9 microgram/gram | | | kamacite, taenite | | | in degrees, minutes and seconds of lattitude and longitude | | low because it has higher tensile strength than stony meteorite | 22254 kg | which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity | | | | |