Subject |
is paired with |
has weather resistance |
has reference |
has minerology |
is an instance of |
has distinguishing feature |
has fragmentation probability |
has olivine grain characteristic |
has likely origin |
has solidification mechanism |
has name |
has olivine composition |
has weather |
has letter designation |
has relative abundance |
has value |
has total mass of find |
has pronunciation |
has matrix composition |
has characteristic mineral |
has composition |
is a kind of |
has find date |
has number of find |
has origin |
has ablative mass loss |
has solidification timescale |
has plagioclase |
has lithic clast composition |
has pigeonite composition |
has definition |
has pyroxene content |
has petrology |
meteorite find | | which depends on its composition | | | | | during meteor phase which depends on composition | | | | 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 | | | | often minerals not found on Earth | meteorite | when the meteorite was found | 1691 | meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal | directly proportional to initial velocity | | | | | a meteorite whose fall was not witnessed | | |
polymict ureilite | | low | | olivine, pyroxene (some combination of pigeonite, orthopyroxene, augite) | | no chondrules | high because it is more friable than iron meteorite | reduced rims contacting carbonaceous matrix material 0.1 mm FeO-free olivine and/or enstatite rims riddled with tiny inclusions of low-Ni metal | partial melting residue | cooling in deep underground chambers | based on the locale, region, or nearby town in which the fall occurred | | | AURE | 7.1 % of meteorite falls | | 9 kg (out of date) | bre - chia | smaller mineral fragments, carbon, suessite (Fe3Si), sulfides, minor chromite and minor apatite | olivine-pigeonite about 90% by volume | silicates (with very few exceptions) | polymict breccia | | 6 (out of date) | asteroid | high because it is more friable than iron meteorite | very slow | common in clasts | typical monomict ureilite material plus a variety of other lithic clasts | | fragmental breccias containing lithic clasts of typical monomict ureilite material plus a variety of other lithic clasts | | coarse-grained granular |
North Haig | Nilpena meteorite (possibly) | which depends on its composition | Berkley et. al (1980) | olivine, pyroxene (some combination of pigeonite, orthopyroxene, augite) | polymict ureilite | no chondrules | during meteor phase which depends on composition | reduced rims contacting carbonaceous matrix material 0.1 mm FeO-free olivine and/or enstatite rims riddled with tiny inclusions of low-Ni metal | partial melting residue | cooling in deep underground chambers | North Haig | Fo% 76-92 | can be severe due to long exposure time to environmental corrosion agents | AURE | | lower because the fall was not witnessed | 485755 kg | bre - chia | smaller mineral fragments, carbon, suessite (Fe3Si), sulfides, minor chromite and minor apatite | olivine-pigeonite about 90% by volume | often minerals not found on Earth | | when the meteorite was found | 1691 | meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal | directly proportional to initial velocity | very slow | common in clasts | typical monomict ureilite material plus a variety of other lithic clasts | Wo% variable En% variable | | 0.26 in modal pyroxene/(pryroxene+olivine) | coarse-grained granular |