| DaG 222 | has image
 |  |
| is an instance of LL5 chondrite |  |
| is an instance of Dar al Gani meteorite |  |
| has name DaG 222 |  |
| is an instance of S3 shock stage chondrite |  |
| has comment breccia |  |
| has find date 1996 |  |
| has fall coordinates 27° 27.20' N., 16° 18.76' E. |  |
| has mass 0.837 kg |  |
| has weathering stage W3 |  |
| LL5 chondrite | has total mass of finds 184 kg |  |
| has number of finds 9 |  |
| Dar al Gani meteorite | has fall location Dar al Gani plateau, Libyan Sahara Desert |  |
| has acronym DaG |  |
| S3 shock stage chondrite | has olivine shock metamorphism planar fractures, undulatory extinction, irregular fractures |  |
| has plagioclase shock metamorphism undulatory extinction |  |
| has orthopyroxene shock metamorphism clinoenstatite lamellae on (100), undulatory extinction, planar fractures, irregular fractures |  |
| LL chondrite | has synonym amphoterite |  |
| has composition bronzite, olivine and minor oligoclase |  |
| has chondrule abundance 60 to 80 % by volume |  |
| has matrix abundance 10 to 15 % by volume |  |
| has refractory inclusion abundance 0.1 to 1 % by volume |  |
| has metal abundance 2 % by volume |  |
| has chondrule mean diameter 0.9 millimeters |  |
| has total iron content low |  |
| has metal iron content about 2 % |  |
| has iron metal and iron sulfide 20 % of total iron |  |
| type 5 chondrite | has petrologic type 5 |  |
| has degree of thermal metamorphism moderate |  |
| has olivine and low Ca pyroxene homogeneity homogeneous |  |
| has structural state of low Ca pyroxene less than 20 % monoclinic |  |
| has chondrule glass type devitrified, absent |  |
| has part feldspar secondary, 2 to 50 micron grains |  |
| has part maximum bulk Ni in metal greater than 20 % by weight, kamacite and taenite in exsolution relationship |  |
| has part sulfide Ni content less than 0.5 % by weight |  |
| has part matrix transparent, recrystallized, moderate size crystals |  |
| has part chondrule chondrules readily delineated |  |
| has part carbon less than 0.2 % by weight |  |
| has part water less than 1.5 % by weight |  |
| shocked chondrite | is independent of the nature and degree of thermal metamorphism or aqueous alteration |  |
| can be shocked before, during or after other types of metamorphism |  |
| has shock pressure the equilibration peak shock pressure in GPa (gigapascals) for ordinary chondrites only |  |
| has shock diagnostic mineral olivine and plagioclase for ordinary chondrite |  |
| has shock diagnostic mineral olivine for carbonaceous chondrite |  |
| has shock diagnostic mineral orthopyroxene for enstatite chondrite |  |
| S3 shock stage meteorite | has shock stage S3 |  |
| has shock pressure 15 to 20 GPa |  |
| has degree of shock metamorphism weakly shocked |  |
| ordinary chondrite | has abundance most common chondrite observed from falls |  |
| thermally altered chondrite | has metamorphism mechanism thermal metamorphism |  |
| has alteration temperature range the range over at which the alteration took place |  |
| meteorite | has fall date recorded by eyewitness or inferred from dating methods |  |
| has fall map which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity |  |
| can have crater image |  |
| has original mass which can over an order of magnitude greater than total mass of fragment(s) collected at the impact site |  |
| has relative abundance |  |
| has impact velocity when it hits the ground which is smaller than its velocity before it enters the atmosphere |  |
| has impact angle |  |
| has weather resistance which depends on its composition |  |
| has monetary value large if the fall was witnessed |  |
| often produce power outages and failures in electrical equipment due to EMP (electromagnetic pulse) |  |
| can be associated with crater |  |
| has origin meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal |  |
| vaporizes completely if size is between 3 micrometers and 3 millimeters |  |
| can survive fall if size is larger than 3 mm and velocity is less than 24 km per second |  |
| can survive fall if it fragments because smaller pieces with less mass are more easily slowed by the atmosphere |  |
| has ablative mass loss depending on composition, more friable stony meteoroids loses more mass than iron meteoroid |  |
| has ablative mass loss directly proportional to initial velocity |  |
| can shatter during impact phase |  |
| can fragment during meteor phase |  |
| has fragmentation probability during meteor phase which depends on composition |  |
| meteorite find | has value lower because the fall was not witnessed |  |
| has weathering can be severe due to long exposure time to environmental corrosion agents |  |
| altered chondrite | has degree of secondary processing providing insight into geological evolution of parent asteroid |  |
| shocked meteorite | has metamorphism mechanism shock metamorphism |  |
| chondrite | has petrologic type range which depends on degree of aqueous alteration and thermal metamorphism |  |
| has homogeneity of olivine and low Ca pyroxene definition goes here |  |
| has part metal maximum bulk in weight % |  |
| has part mean Ni content of sulfides in weight % |  |
| rock | has part mineral |  |
| has texture |  |
| has genesis |  |
| undifferentiated meteorite | has peak temperature less than 950 degree Celsius during its entire history since solidification |  |
| has parent body asteroid smaller than 100 km in diameter |  |
| has age oldest and most primitive rock in solar system |  |
| conglomerate | has sediment mechanism agglomeration of particles, many of which record individual, diverse histories |  |