Subject |
has sediment mechanism |
has weather resistance |
has minerology |
has age |
is an instance of |
has distinguishing feature |
has fragmentation probability |
has fall location |
has fall date |
has likely origin |
has name |
has weather |
has fall description |
has letter designation |
has relative abundance |
has texture |
has prototype |
has value |
has total mass of find |
has peak temperature |
has parent body |
has fall coordinate |
has composition |
is a kind of |
has mass |
has image |
has number of find |
has ablative mass loss |
has definition |
has petrology |
lodranite | agglomeration of particles, many of which record individual, diverse histories | low | olivine, orthopyroxene, clinopyroxene, metal with some troilite and some sodic plagioclase | oldest and most primitive rock in solar system | | no chondrules | high because it is more friable than iron meteorite | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | recorded by eyewitness or inferred from dating methods | ultrametamorphism, partial melting with some melt migration | based on the locale, region, or nearby town in which the fall occurred | | | LOD | 7.1 % of meteorite falls | coarse grained | Lodran meteorite | | 1606 kg | less than 950 degree Celsius during its entire history since solidification | asteroid smaller than 100 km in diameter | in degrees, minutes and seconds of lattitude and longitude | iron, pyroxene, olivine subcondritic abundances of plagioclase and troilite; | primitive achondrite | | | 70 | high because it is more friable than iron meteorite | | fine- to coarse-grained equigranular |
meteorite fall | | which depends on its composition | | | | | during meteor phase which depends on composition | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | recorded by eyewitness or instruments | | based on the locale, region, or nearby town in which the fall occurred | negligible due to quick recovery of meteorite before corrosion begins | what witnesses saw or what was recorded by instruments | | | | | higher because the fall was witnessed | 485755 kg | | | in degrees, minutes and seconds of lattitude and longitude | often minerals not found on Earth | meteorite | | | 1691 | directly proportional to initial velocity | a meteorite whose fall was witnessed by human or electronic means | |
Lodran | agglomeration of particles, many of which record individual, diverse histories | which depends on its composition | olivine, orthopyroxene, clinopyroxene, metal with some troilite and some sodic plagioclase | oldest and most primitive rock in solar system | meteorite fall | no chondrules | during meteor phase which depends on composition | 12 miles east of Lodhran, Pakistan | 2:00 pm October 1, 1868 | ultrametamorphism, partial melting with some melt migration | Lodran | negligible due to quick recovery of meteorite before corrosion begins | what witnesses saw or what was recorded by instruments | LOD | | coarse grained | Lodran meteorite | higher because the fall was witnessed | 485755 kg | less than 950 degree Celsius during its entire history since solidification | asteroid smaller than 100 km in diameter | 29° 32' N., 71° 48' E. | iron, pyroxene, olivine subcondritic abundances of plagioclase and troilite; | | 1 kg |
 | 1691 | directly proportional to initial velocity | | fine- to coarse-grained equigranular |