Subject |
has sediment mechanism |
has weather resistance |
has metal abundance |
has part mean Ni content of sulfide |
has age |
has refractory inclusion abundance |
is an instance of |
has part feldspar |
has part metal maximum bulk |
has fragmentation probability |
has fall location |
has name |
has weather |
has homogeneity of olivine and low Ca pyroxene |
has acronym |
has chondrule abundance |
has relative abundance |
has part chondrule |
has prototype |
has petrologic subtype |
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 petrologic type range |
has matrix abundance |
has fall coordinate |
has part carbon |
has petrologic type |
has composition |
is a kind of |
has find date |
has part water |
has mass |
has image |
has number of find |
has ablative mass loss |
has synonym |
has chondrule mean diameter |
Dar al Gani meteorite | | which depends on its composition | | | | | | | | during meteor phase which depends on composition | Dar al Gani plateau, Libyan Sahara Desert | 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 | | DaG | | | | | | | lower because the fall was not witnessed | 485755 kg | | | | | | | in degrees, minutes and seconds of lattitude and longitude | | | often minerals not found on Earth | Sahara meteorite | when the meteorite was found | | | | 1691 | directly proportional to initial velocity | | |
R chondrite | agglomeration of particles, many of which record individual, diverse histories | low | 0.1 % by volume | in weight % | oldest and most primitive rock in solar system | 0 % by volume | | usually plagioclase tectosilicate | in weight % | high because it is more friable than iron meteorite | 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 | | definition goes here | | greater than 40 % by volume | 85.7 % of meteorite falls | small sphere of about 1 mm diameter of formerly melted minerals | Rumuruti meteorite | | highly oxidized | | 20461 kg | definition goes here | less than 950 degree Celsius during its entire history since solidification | asteroid smaller than 100 km in diameter | fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents | which depends on degree of aqueous alteration and thermal metamorphism | 36 % by volume | in degrees, minutes and seconds of lattitude and longitude | in weight % | 3 to 6 | enriched in 17O isotope | anhydrous chondrite | | 0 % by weight (approximately) | | | 1030 | high because it is more friable than iron meteorite | rumurutiite | 0.4 millimeters |
DaG 013 | agglomeration of particles, many of which record individual, diverse histories | which depends on its composition | 0.1 % by volume | in weight % | oldest and most primitive rock in solar system | 0 % by volume | Dar al Gani meteorite | usually plagioclase tectosilicate | in weight % | during meteor phase which depends on composition | Dar al Gani plateau, Libyan Sahara Desert | DaG 013 | can be severe due to long exposure time to environmental corrosion agents | definition goes here | DaG | greater than 40 % by volume | | small sphere of about 1 mm diameter of formerly melted minerals | Rumuruti meteorite | 3.5 | highly oxidized | lower because the fall was not witnessed | 485755 kg | definition goes here | less than 950 degree Celsius during its entire history since solidification | asteroid smaller than 100 km in diameter | fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents | which depends on degree of aqueous alteration and thermal metamorphism | 36 % by volume | 27° 07.77' N., 16° 20.61' E. | in weight % | 3 to 6 | enriched in 17O isotope | | 1994-1995 | 0 % by weight (approximately) | 0.205 kg |
 | 1691 | directly proportional to initial velocity | rumurutiite | 0.4 millimeters |