| Renazzo | has image
 |  |
| is an instance of CR chondrite |  |
| is an instance of meteorite fall |  |
| has name Renazzo |  |
| is an instance of S2 shock stage chondrite |  |
| has mass 10 kg |  |
| has fall coordinates 44° 46' N., 11° 17' E. |  |
| has fall date January 15, 1824 8:30 pm |  |
| has fall location Renazzo, Italy |  |
| CR chondrite | has prototype ??? meteorite |  |
| has chondrule abundance 50 to 60 % by volume |  |
| has matrix abundance 30 to 50 % by volume |  |
| has refractory inclusion abundance 0.5 % by volume |  |
| has metal abundance 5 to 8 % by volume |  |
| has chondrule mean diameter 0.7 millimeters |  |
| has chondrule glass type preserved |  |
| meteorite fall | has value higher because the fall was witnessed |  |
| has fall description what witnesses saw or what was recorded by instruments |  |
| has weathering negligible due to quick recovery of meteorite before corrosion begins |  |
| S2 shock stage chondrite | has olivine shock metamorphism undulatory extinction, irregular fractures |  |
| has plagioclase shock metamorphism undulatory extinction, irregular fractures |  |
| has orthopyroxene shock metamorphism undulatory extinction, irregular fractures, some planar fractures |  |
| carbonaceous chondrite | has relative abundance 8 % of meteorite falls |  |
| has total mass of finds 2577 kg |  |
| has number of finds 36 |  |
| has distinguishing feature elemental carbon |  |
| has abundance rare relative to other chondrite types |  |
| type 2 chondrite | has petrologic type 2 |  |
| has degree of aqueous alteration moderate |  |
| has olivine and low Ca pyroxene homogeneity greater than 5 % deviations |  |
| has structural state of low Ca pyroxene predominantly monoclinic |  |
| has part feldspar minor primary grains only |  |
| has part maximum bulk Ni in metal less than 20 % by weight; taenite minor or absent |  |
| has part sulfide Ni content greater than 0.5 % by weight |  |
| has part matrix mostly fine, opaque |  |
| has part chondrule chondrules very sharply defined |  |
| has part carbon 0.8 to 2.6 % by weight |  |
| has part water 2 to 16 % by weight |  |
| meteorite | 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 composition often minerals not found on Earth |  |
| has relative abundance |  |
| has total mass of finds 485755 kg |  |
| has number of finds 1691 |  |
| 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 |  |
| 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 |  |
| S2 shock stage meteorite | has shock stage S2 |  |
| has shock pressure 5 to 10 GPa |  |
| has degree of shock metamorphism very weakly shocked |  |
| 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 % |  |
| water altered chondrite | has metamorphism mechanism aqueous altermation |  |
| rock | has part mineral |  |
| has texture |  |
| has genesis |  |
| altered chondrite | has degree of secondary processing providing insight into geological evolution of parent asteroid |  |
| shocked meteorite | has metamorphism mechanism shock metamorphism |  |
| 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 |  |