Subject |
has weather resistance |
has minerology |
is an instance of |
has distinguishing feature |
has fragmentation probability |
has fall location |
has likely origin |
has name |
has weather |
has letter designation |
has relative abundance |
has value |
has total mass of find |
has fall coordinate |
has characteristic mineral |
has composition |
is a kind of |
has find date |
has mass |
has image |
has number of find |
has origin |
has ablative mass loss |
has definition |
be an acronym for |
has petrology |
howardite | low | orthopyroxene, olivine, chromite; pigeonite, calcic plagioclase, silica | | no chondrules | high because it is more friable than iron meteorite | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | cumulates, crystallized melts, impact mixing | based on the locale, region, or nearby town in which the fall occurred | | AHOW | 7.1 % of meteorite falls | | 41 kg | in degrees, minutes and seconds of lattitude and longitude | eucrite-diogenite mixture | silicates (with very few exceptions) | HED meteorite | | | | 19 | 4 Vesta | high because it is more friable than iron meteorite | | Howardite, Eucrite, Diogenite | coarse-grained orthopyroxenites, gabbros, fine- to coarse-grained basalts, brecciated |
meteorite find | which depends on its composition | | | | during meteor phase which depends on composition | 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 | can be severe due to long exposure time to environmental corrosion agents | | | lower because the fall was not witnessed | 485755 kg | in degrees, minutes and seconds of lattitude and longitude | | 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 | | |
Old Homestead 001 | which depends on its composition | orthopyroxene, olivine, chromite; pigeonite, calcic plagioclase, silica | meteorite find | no chondrules | during meteor phase which depends on composition | Nullarbor Plain, Western Australia | cumulates, crystallized melts, impact mixing | Homestead 001 | can be severe due to long exposure time to environmental corrosion agents | AHOW | | lower because the fall was not witnessed | 41 kg | 31° 10' S., 127° 45' E. | eucrite-diogenite mixture | often minerals not found on Earth | | June 1991 | 0.783 kg |
 | 19 | meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal | directly proportional to initial velocity | | Howardite, Eucrite, Diogenite | coarse-grained orthopyroxenites, gabbros, fine- to coarse-grained basalts, brecciated |