Subject |
has augite grain size |
has weather resistance |
is an instance of |
has fragmentation probability |
has fall location |
has name |
has genesi |
has weather |
has identification date |
has relative abundance |
has texture |
has value |
has total mass of find |
has fall coordinate |
has composition |
has olivine grain size |
has find date |
has mass |
has grain size |
has image |
has number of find |
has origin |
has ablative mass loss |
ALH 84025 | up to 2.7 millimeters | which depends on its composition | Antarctic meteorite | during meteor phase which depends on composition | indicated by letters in the beginning of name | ALH 84025 | | | | | | | 485755 kg | in degrees, minutes and seconds of lattitude and longitude | often minerals not found on Earth | up to 1.8 millimeters | 1984 | | | | 1691 | meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal | directly proportional to initial velocity |
Brachina | | low | brachinite | high because it is more friable than iron meteorite | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | Brachina | fractional crystallization | | | 7.1 % of meteorite falls | equigranular | | 1606 kg | in degrees, minutes and seconds of lattitude and longitude | olivine and some clinopyroxene | | | | 0.1 to 0.3 millimeters | | 70 | asteroid | high because it is more friable than iron meteorite |
Eagles Nest | | low | brachinite | high because it is more friable than iron meteorite | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | Eagles Nest | fractional crystallization | | | 7.1 % of meteorite falls | | | 1606 kg | in degrees, minutes and seconds of lattitude and longitude | olivine and some clinopyroxene | | | | | | 70 | asteroid | high because it is more friable than iron meteorite |
Hughes 026 | | low | brachinite | high because it is more friable than iron meteorite | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | Hughes 026 | fractional crystallization | | | 7.1 % of meteorite falls | equigranular | | 1606 kg | in degrees, minutes and seconds of lattitude and longitude | olivine and some clinopyroxene | | | | 0.65 millimeters | | 70 | asteroid | high because it is more friable than iron meteorite |
Nova 003 | | low | brachinite | high because it is more friable than iron meteorite | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | Nova 003 | fractional crystallization | | | 7.1 % of meteorite falls | | | 1606 kg | in degrees, minutes and seconds of lattitude and longitude | olivine and some clinopyroxene | | | | | | 70 | asteroid | high because it is more friable than iron meteorite |
Reid 013 | | which depends on its composition | meteorite find | during meteor phase which depends on composition | Nullarbor, Western Australia | Reid 013 | | can be severe due to long exposure time to environmental corrosion agents | | | | lower because the fall was not witnessed | 485755 kg | 30° 05' S., 128° 55' E. | often minerals not found on Earth | | 1991 | 0.330 kg | |
 | 1691 | meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal | directly proportional to initial velocity |