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 prototype |
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 |
has petrology |
angrite | low | Al-Ti-diopside, anorthite, calcic olivine | | no chondrules | high because it is more friable than iron meteorite | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | crystallized melts, cumulates (?) | based on the locale, region, or nearby town in which the fall occurred | | ACANOM | 7.1 % of meteorite falls | Angra dos Reis meteorite | | 1606 kg | in degrees, minutes and seconds of lattitude and longitude | augite | silicates (with very few exceptions) | asteroidal achondrite | | | | 70 | asteroid | high because it is more friable than iron meteorite | | fine- to coarse-grained igneous |
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 | |
Sahara 99555 | which depends on its composition | Al-Ti-diopside, anorthite, calcic olivine | meteorite find | no chondrules | during meteor phase which depends on composition | Sahara Desert | crystallized melts, cumulates (?) | Sahara 99555 | can be severe due to long exposure time to environmental corrosion agents | ACANOM | | Angra dos Reis meteorite | lower because the fall was not witnessed | 485755 kg | | augite | often minerals not found on Earth | | May 1999 | 2.710 kg |
 | 1691 | meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal | directly proportional to initial velocity | | fine- to coarse-grained igneous |