Subject |
has weather resistance |
has olivine shock metamorphism |
is independent of |
has shock pressure |
has acronym |
has petrologic subtype |
has image |
has weather |
has degree of secondary process |
has relative abundance |
has fragmentation probability |
has metamorphism mechanism |
has weathering stage |
has number of fragment |
has number of find |
has find date |
has orthopyroxene shock metamorphism |
has plagioclase shock metamorphism |
has identification date |
has degree of shock metamorphism |
has mass |
has shock diagnostic mineral |
has name |
be shock |
has fall location |
is an instance of |
has shock stage |
has distribution ellipse |
has value |
has fall coordinate |
has ablative mass loss |
has total mass of find |
classified by |
DaG 005 | which depends on its composition | undulatory extinction, irregular fractures | the nature and degree of thermal metamorphism or aqueous alteration | 5 to 10 GPa | DaG | |
 | can be severe due to long exposure time to environmental corrosion agents | providing insight into geological evolution of parent asteroid | 8 % of meteorite falls | during meteor phase which depends on composition | shock metamorphism | W2 | | 36 | 1995 | undulatory extinction, irregular fractures, some planar fractures | undulatory extinction, irregular fractures | | very weakly shocked | | orthopyroxene for enstatite chondrite | DaG 005 | before, during or after other types of metamorphism | Dar al Gani plateau, Libyan Sahara Desert | S2 shock stage chondrite | S2 | | lower because the fall was not witnessed | 27° 09.39' N., 15° 57.15' E. | directly proportional to initial velocity | 2577 kg | |
Isna | which depends on its composition | | | | | 3.7 |
 | can be severe due to long exposure time to environmental corrosion agents | | | during meteor phase which depends on composition | | | | 1691 | 1970 | | | | | | | Isna | | Nile River near Luxor, Egypt | Antarctic meteorite | | | lower because the fall was not witnessed | 24° 50' N., 31° 40' E. | directly proportional to initial velocity | 485755 kg | |
Ornans | low | | | | | | | | | 8 % of meteorite falls | high because it is more friable than iron meteorite | | | | 36 | | | | | | | | based on the locale, region, or nearby town in which the fall occurred | | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | CO chondrite | | | | in degrees, minutes and seconds of lattitude and longitude | high because it is more friable than iron meteorite | 2577 kg | |
UK 43 | which depends on its composition | | | | DaG | |
 | can be severe due to long exposure time to environmental corrosion agents | | 8 % of meteorite falls | during meteor phase which depends on composition | | | 2000 or more | 36 | 1999 | | | | | 177 kg | | based on the locale, region, or nearby town in which the fall occurred | | Dar al Gani plateau, Libyan Sahara Desert | CO chondrite | |
 | lower because the fall was not witnessed | in degrees, minutes and seconds of lattitude and longitude | directly proportional to initial velocity | 2577 kg | Open University, UK. Meteoritical Bulletin No 84 |