| Indarch | has image
 |  |
| is an instance of EH4 chondrite |  |
| is an instance of meteorite fall |  |
| has name Indarch |  |
| is an instance of S3 shock stage chondrite |  |
| has fall date 8:10 pm April 7, 1891 |  |
| has fall coordinates 39° 45' N., 46° 40' E. |  |
| has fall location Azerbaydzhan SSR, USSR |  |
| has mass 27 kg |  |
| 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 |  |
| 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 |  |
| EH chondrite | has petrologic type 3 to 5 |  |
| has chondrule abundance 60 to 80 % by volume |  |
| has matrix abundance less than 2 to 15 % by volume |  |
| has refractory inclusion abundance 0.1 to 1 % by volume |  |
| has metal abundance 8 % by volume |  |
| has chondrule mean diameter 0.2 millimeters |  |
| has total iron content high |  |
| E4 chondrite | has total mass of finds 143 kg |  |
| has number of finds 5 |  |
| 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 |  |
| S3 shock stage meteorite | has shock stage S3 |  |
| has shock pressure 15 to 20 GPa |  |
| has degree of shock metamorphism weakly shocked |  |
| enstatite chondrite | has synonym E chondrite |  |
| has oxidized iron content zero |  |
| type 4 chondrite | has degree of thermal metamorphism weak |  |
| has olivine and low Ca pyroxene homogeneity less than 5 % mean deviations |  |
| has structural state of low Ca pyroxene greater than 20 % monoclinic |  |
| has chondrule glass type devitrified, absent |  |
| has part feldspar secondary, grains than 2 microns |  |
| 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, small crystals |  |
| has part chondrule chondrules well defined |  |
| has part carbon less than 0.2 % by weight |  |
| has part water less than 1.5 % by weight |  |
| 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 |  |
| highly reduced meteorite | has oxidation state highly reduced with very little FeO |  |
| thermally altered chondrite | has alteration temperature range the range over at which the alteration took place |  |
| 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 % |  |
| 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 |  |