| Gao-Guenie | has image
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| has name Gao-Guenie |  |
is an instance of H5 chondrite  |  |
| has fall date March 5, 1960, 17:00 local time |  |
| has fall location Burkina Faso (formerly Upper Volta), Africa |  |
| has fall coordinates Latitude 11 degrees 39 minutes North, Longitude 2 degrees 11 minutes West |  |
has fall map
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| H5 chondrite | has total mass of finds 1267 kg |  |
| has number of finds 76 |  |
| H chondrite | has synonym bronzite chondrite |  |
| 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 10 % by volume |  |
| has chondrule mean diameter 0.3 millimeters |  |
| has total iron content high |  |
| has metal iron content 12 to 21 % |  |
| has iron metal and iron sulfide 75 % 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 |  |
| 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 |  |
| altered chondrite | has degree of secondary processing providing insight into geological evolution of parent asteroid |  |
| chondrite | has petrologic type range which depends on degree of aqueous alteration and thermal metamorphism |  |
| has relative abundance 85.7 % of meteorite falls |  |
| 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 % |  |
| stony meteorite | has weather resistance low |  |
| has fragmentation probability high because it is more friable than iron meteorite |  |
| has ablative mass loss high because it is more friable than iron meteorite |  |
| 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 |  |
| rock | has part mineral |  |
| has texture |  |
| has genesis |  |
| meteorite | 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 composition often minerals not found on Earth |  |
| has impact velocity when it hits the ground which is smaller than its velocity before it enters the atmosphere |  |
| has impact angle |  |
| 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 |  |
| can shatter during impact phase |  |
| can fragment during meteor phase |  |
| conglomerate | has sediment mechanism agglomeration of particles, many of which record individual, diverse histories |  |