Subject |
has weather resistance |
has sediment mechanism |
has minerology |
has age |
is an instance of |
has distinguishing feature |
has fragmentation probability |
has fall location |
has likely origin |
has name |
has weather |
has relative abundance |
has texture |
has prototype |
has value |
has total mass of find |
has peak temperature |
has parent body |
has fall coordinate |
has composition |
is a kind of |
has find date |
has mass |
has image |
has number of find |
has ablative mass loss |
has definition |
has petrology |
acapulcoite | low | agglomeration of particles, many of which record individual, diverse histories | olivine, orthopyroxene, clinopyroxene, metal with some troilite and some sodic plagioclase | oldest and most primitive rock in solar system | | no chondrules | high because it is more friable than iron meteorite | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | ultrametamorphism, partial melting with some melt migration | based on the locale, region, or nearby town in which the fall occurred | | 7.1 % of meteorite falls | medium grained | Acapulco meteorite | | 1606 kg | less than 950 degree Celsius during its entire history since solidification | asteroid smaller than 100 km in diameter | in degrees, minutes and seconds of lattitude and longitude | chondritic abundances of plagioclase and troilite; | primitive achondrite | | | | 70 | high because it is more friable than iron meteorite | | fine- to coarse-grained equigranular |
Antarctic meteorite | which depends on its composition | | | | | | during meteor phase which depends on composition | indicated by letters in the beginning of name | | 3 or 4 letter contracted from find location then last two digits of year then id number | | | | | | 485755 kg | | | in degrees, minutes and seconds of lattitude and longitude | often minerals not found on Earth | meteorite | recovery year is first 2 numbers in name | | | 1691 | directly proportional to initial velocity | | |
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 | directly proportional to initial velocity | a meteorite whose fall was not witnessed | |
Monument Draw | which depends on its composition | agglomeration of particles, many of which record individual, diverse histories | olivine, orthopyroxene, clinopyroxene, metal with some troilite and some sodic plagioclase | oldest and most primitive rock in solar system | Antarctic meteorite | no chondrules | during meteor phase which depends on composition | 18 miles NW of Andrews, Texas | ultrametamorphism, partial melting with some melt migration | Monument Draw | can be severe due to long exposure time to environmental corrosion agents | | medium grained | Acapulco meteorite | lower because the fall was not witnessed | 485755 kg | less than 950 degree Celsius during its entire history since solidification | asteroid smaller than 100 km in diameter | 32° 30.2' N., 102° 44.6' W. | chondritic abundances of plagioclase and troilite; | | 1985 | 0.5245 kg |
 | 1691 | directly proportional to initial velocity | | fine- to coarse-grained equigranular |