Subject |
has solidification timescale |
has synonym |
has daubreelite |
has mafic mineral |
has prototype |
has nickel content |
has chr |
has iridium content |
has phosphor content |
has origin |
has gallium content |
has image |
has solidification mechanism |
has shape of inclusion |
have composition |
is a kind of |
has arsenic content |
has copper content |
has troilite |
has structural class |
has antimony content |
has find date |
has plagioclase |
has metal |
has W.P. |
has tungsten content |
has name |
has crystal size |
has fall location |
has chromium content |
is an instance of |
parent body radiu |
has formation cooling rate |
has schreibersite |
has cobalt content |
has cohenite |
has palladium content |
has germanium content |
has molydbenum content |
has gold content |
has graphite |
has metal content |
has troilite texture |
has fall coordinate |
Mundrabilla | | | 1.6 % by volume | 48.5 % by volume | Vigarano meteorite | 7.47 % by weight | % by volume | 2.7 microgram/gram | 2.1 milligram/gram | asteroid wide partial melting | 96 microgram/gram |
 | | | 7.72% Ni, 59.5 ppm Ga, 196 ppm Ge, 0.87 ppm Ir | | 11 microgram/gram | 132 microgram/gram | 30.5 % by volume | Of | 270 nanogram/gram | 1911 | 14.9 % by volume | 0.12 % by volume | 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 | 3.5 microgram/gram | 400 microgram/gram | 8.2 microgram/gram | 1.5 microgram/gram | 3.7 % by volume | higher than that of average solar system material | | Latitude 30 degrees 47 minutes South, Longitude 127 degrees 33 minutes East |
oxidized-Allende subgroup CV chondrite | | CV3OxA chondrite | | | Allende meteorite | | | | | meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal | | | | | | CV chondrite | | | | | | | | | | | 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 | | | | | | | | | | | | | | | in degrees, minutes and seconds of lattitude and longitude |
oxidized-Bali subgroup CV chondrite | | CV3OxB chondrite | | | Bali meteorite | | | | | meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal | | | | | | CV chondrite | | | | | | | | | | | 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 | | | | | | | | | | | | | | | in degrees, minutes and seconds of lattitude and longitude |
reduced subgroup CV chondrite | | CV3R chondrite | | | Vigarano meteorite | | | | | meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal | | | | | | CV chondrite | | | | | | | | | | | 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 | | | | | | | | | | | | | | | in degrees, minutes and seconds of lattitude and longitude |