Subject |
has weather resistance |
has olivine shock metamorphism |
is independent of |
has shock pressure |
has petrologic subtype |
has image |
has weather |
has degree of secondary process |
has relative abundance |
has fragmentation probability |
has metamorphism mechanism |
has fall date |
has fall description |
has number of find |
has orthopyroxene shock metamorphism |
has plagioclase shock metamorphism |
has degree of shock metamorphism |
has mass |
has shock diagnostic mineral |
has name |
be shock |
is an instance of |
has shock stage |
has composition |
has value |
has fall coordinate |
has ablative mass loss |
has total mass of find |
Bali | low | | | | | | | | 8 % of meteorite falls | high because it is more friable than iron meteorite | | recorded by eyewitness or inferred from dating methods | | 36 | | | | | | based on the locale, region, or nearby town in which the fall occurred | | oxidized-Bali subgroup CV chondrite | | iron-rich olivine, calcium aluminum inclusions | | in degrees, minutes and seconds of lattitude and longitude | high because it is more friable than iron meteorite | 2577 kg |
Grosnaja | which depends on its composition | planar fractures, undulatory extinction, irregular fractures | the nature and degree of thermal metamorphism or aqueous alteration | 15 to 20 GPa | 3.3 |
 | negligible due to quick recovery of meteorite before corrosion begins | providing insight into geological evolution of parent asteroid | | during meteor phase which depends on composition | shock metamorphism | June 28, 1861 7:00 pm | what witnesses saw or what was recorded by instruments | 1691 | clinoenstatite lamellae on (100), undulatory extinction, planar fractures, irregular fractures | undulatory extinction | weakly shocked | 3.5 kg | orthopyroxene for enstatite chondrite | Grosnaja | before, during or after other types of metamorphism | S3 shock stage chondrite | S3 | often minerals not found on Earth | higher because the fall was witnessed | 43° 40' N., 45° 23' E. | directly proportional to initial velocity | 485755 kg |
Kaba | low | | | | | | | | 8 % of meteorite falls | high because it is more friable than iron meteorite | | recorded by eyewitness or inferred from dating methods | | 36 | | | | | | based on the locale, region, or nearby town in which the fall occurred | | oxidized-Bali subgroup CV chondrite | | iron-rich olivine, calcium aluminum inclusions | | in degrees, minutes and seconds of lattitude and longitude | high because it is more friable than iron meteorite | 2577 kg |
Mokoia | low | | | | | | | | 8 % of meteorite falls | high because it is more friable than iron meteorite | | recorded by eyewitness or inferred from dating methods | | 36 | | | | | | based on the locale, region, or nearby town in which the fall occurred | | oxidized-Bali subgroup CV chondrite | | iron-rich olivine, calcium aluminum inclusions | | in degrees, minutes and seconds of lattitude and longitude | high because it is more friable than iron meteorite | 2577 kg |