Subject |
has weather resistance |
is an instance of |
has fragmentation probability |
has fall location |
has name |
has weather |
has identification date |
has relative abundance |
has value |
has total mass of find |
has fall coordinate |
has find date |
has mass |
has image |
has number of find |
has ablative mass loss |
Acapulco | low | acapulcoite | 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 | | | 7.1 % of meteorite falls | | 1606 kg | in degrees, minutes and seconds of lattitude and longitude | | | | 70 | high because it is more friable than iron meteorite |
ALH 81187 | low | acapulcoite | 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 | | | 7.1 % of meteorite falls | | 1606 kg | in degrees, minutes and seconds of lattitude and longitude | | | | 70 | high because it is more friable than iron meteorite |
Monument Draw | which depends on its composition | Antarctic meteorite | during meteor phase which depends on composition | 18 miles NW of Andrews, Texas | Monument Draw | can be severe due to long exposure time to environmental corrosion agents | | | lower because the fall was not witnessed | 485755 kg | 32° 30.2' N., 102° 44.6' W. | 1985 | 0.5245 kg |
 | 1691 | directly proportional to initial velocity |
Y-74063 | low | acapulcoite | 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 | | | 7.1 % of meteorite falls | | 1606 kg | in degrees, minutes and seconds of lattitude and longitude | | | | 70 | high because it is more friable than iron meteorite |